"Can selfinteraction in supernova neutrinos cause changes in gravitational memory signals?"Indranil Chakraborty , Indian Institute of Technology Bombay [Host: David Nichols]
ABSTRACT:
Gravitational wave memory is a persistent nonoscillatory shift in the gravitational wave amplitude. Such effects are ubiquitous in astrophysical and cosmological cataclysmic events involving gravitational radiation. In this talk, we turn our attention to the case of a supernova neutrino burst generating gravitational radiation. Previous studies along this line have demonstrated that a neutrino burst in such scenarios gives rise to a gravitational memory signal. Here, we specifically inquire about the alterations to the memory signal when neutrinos emitted from a supernova undergo selfinteraction, presenting an avenue for indirectly detecting neutrino selfinteraction. 
Gravity Seminar Thursday, June 6, 2024 2:00 PM Physics, Room 031 Join Zoom Meeting: https://virginia.zoom.us/j/99737910818?pwd=kW5bNj2Iwh2XmEaZuamMbWZ6AjsH8a.1 Meeting ID: 997 3791 0818 Passcode: 609195 
"Unraveling the mysteries of strong gravity by employing electromagnetic and gravitational memory."Susmita Jana , Indian Institute of Technology Bombay [Host: David Nichols]
ABSTRACT:
The gravitational memory effect and its electromagnetic (EM) analog are potential probes in the strong gravity regime. In the literature, this effect is derived for static observers at asymptotic infinity. While this is a physically consistent approach, it restricts us to deriving memory for an asymptotically flat spacetime. In this talk, I will discuss how we evaluate EM and gravitational memory with respect to a comoving observer (defined by timelike 4velocity u_{a}). We split 4D the spacetime into 1+1+2 parts, consisting of one timelike, one preferred spacelike, and one 2D hypersurface. It allows us to obtain EM memory in an arbitrary curved background spacetime and gravitational memory in a class of spacetime with spherical symmetry often referred to as Locally Rotationally Symmetric(LRS) type II in covariant formalism. The master equation corresponding to the acceleration of the comoving observer in the 2D surface provides a physical understanding of the EM memory. The leading order contribution to the EM memory comes from the total energy density of the EM field, while the subleading contributions contain the spacetime geometry and the other components of the energymomentum tensor of the EM field. In the case of gravitational memory, we show it is manifested in the integral of the shear tensor of the 2D hypersurface. We obtain the master equation of gravitational memory in LRSII spacetime and finally, we show that the memory exhibits distinct signatures between accelerated and decelerated universes, potentially enabling the identification of the transition redshift from a matterdominated to a darkenergydominated universe. In the end(if time permits), I will briefly discuss the generation of detectable GW from the interaction of very high energized EM wave and stellarmass Schwarzschild black holes in the Milky Way galaxy. 
Gravity Seminar Tuesday, June 4, 2024 10:00 AM Physics, Room 323 Join Zoom Meeting https://virginia.zoom.us/j/99737910818?pwd=kW5bNj2Iwh2XmEaZuamMbWZ6AjsH8a.1 Meeting ID: 997 3791 0818 Passcode: 609195 
"Tidal Love numbers: from black holes to exotic physics"Valerio De Luca , University of Pennsylvania [Host: Kent Yagi]
ABSTRACT:
Tidal Love numbers describe the linear response of compact objects to external tidal perturbations, and they are found to vanish exactly for black holes within General Relativity. We first discuss the robustness of this property when nonlinearities in the theory are taken into account, and then investigate the scenario of black holes dressed with an ultralight scalar field, addressing their detectability at future gravitational wave experiments. Finally, we discuss the tidal deformability of more exotic compact objects, showing the relevance of universality relations as a way to distinguish between them. 
Gravity Seminar Monday, June 3, 2024 1:30 PM Physics, Room 323 Join Zoom Meeting https://virginia.zoom.us/j/92692915873?pwd=RBHqSluEzZauAN6a40yhaDnyq2q0eh.1 Meeting ID: 926 9291 5873 Passcode: 503528 
"Taming eccentricity in binary black hole mergers"Tousif Islam , Kavli Institute for Theoretical Physics, University of California Santa Barbara [Host: Kent Yagi]
ABSTRACT:
Accurate characterization of gravitational wave signals from binary black hole (BBH) mergers require efficient models for the waveform and remnant quantities. While we have accurate models for quasicircular BBH mergers, modelling eccentric binaries is still in its nascent stage. Using both numerical relativity (NR) and black hole perturbation theory (BHPT), we study the phenomenology of eccentric BBH waveforms. We present convincing evidence that the waveform phenomenology in eccentric BBH mergers is significantly simpler than previously thought. We find that the eccentric modulations in the amplitudes and frequencies in different spherical harmonic modes are all related and can be modeled using a single time series modulation. Using this universal eccentric modulation, we provide a model named gwNRHME to seamlessly convert a multimodal (i.e with several spherical harmonic modes) quasicircular waveform into multimodal eccentric waveform if the quadrupolar eccentric waveform is known. This reduces the modelling complexity of eccentric BBH mergers drastically as we now have to model only a single eccentric modulation timeseries instead of modelling the effect of eccentricity in all modes. We use gwNRHME to include eccentricity in current NR surrogate waveform models for quasicircular mergers. Additionally, we discuss efforts in building dedicated surrogate models for eccentric BBH mergers using both NR and BHPT. 
Gravity Seminar Monday, April 22, 2024 1:30 PM Physics, Room 031 
"Probing new physics from tests of gravity and pulsar kick"Tanmay Poddar , Istituto Nazionale di Fisica Nucleare [Host: Kent Yagi]
ABSTRACT:
Ultralight axionlike particles, an excellent candidate for dark matter, can mediate a longrange macroscopic force with monopolemonopole and monopoledipole interactions between the planets and the Sun. The presence of these longrange potentials affects the perihelion precession of planets, gravitational light bending and Shapiro time delay. From the precision studies of these tests of gravity, we obtain new constraints on the macroscopic forces. The bound is three orders of magnitude stronger than the EotWash experiment. The ultralight scalar and vector dark matter also influence activesterile neutrino oscillation in the supernova core which is one of the solutions to explain the longstanding problem of the pulsar kick. The signal from the asymmetric emission of neutrinos in the presence of an ultralight dark matter background can be probed by future gravitational wave detectors. The effects of ultralight dark matter in explaining pulsar kick are equivalent to the Lorentz and CPT invariance violation in the theory and we obtain an equivalent bounds on these parameters. 
Gravity Seminar Monday, April 15, 2024 1:00 PM Online, Room Zoom Join Zoom Meeting: Meeting ID: 939 1525 6097 
"Gravitational and Electromagnetic Love Numbers of Magnetar Systems: an Effective Field Theory Approach"Siddarth Ajith , University of Virginia [Host: Kent Yagi]
ABSTRACT:
With the advent of gravitational wave astronomy, our view of the universe has expanded to new and exciting frontiers. One especially promising avenue to explore in fundamental physics through gravitational waves is probing dense nuclear matter contained in neutron stars; observations of gravitational waves sourced by these extremely compact objects allow one to study matter in regimes that we could never replicate on Earth. Compact stars contain finitesize effects, such as tidal deformations, which leave imprints on the gravitational wave signal that describe the internal stellar structure, so studying such effects is crucial to expanding our understanding of matter at the most extreme scales. In this seminar, I shall describe how tidal fields in magnetar systems (neutron stars with incredibly strong magnetic fields) can lead to an interesting interplay between tidal fields and magnetic fields. This interaction is encapsulated in how the tidal field changes the magnetic properties of the star and, in turn, in how the magnetic field of the star changes its tidal deformability properties. I shall also outline an effective field theory formalism to study tidal fields alongside the conventional general relativity formalism. This effective field theory approach proves to be a natural arena to identify features of this system which can be difficult to study with the usual spacetime geometric approach alone. 
Gravity Seminar Monday, April 1, 2024 1:30 PM Zoom and inperson, Room 323, JBL Join Zoom Meeting 
"Gravitationalwaves: from black holes to the cosmos"Maximiliano Isi , Flatiron Institute [Host: Sayantani Datta]
ABSTRACT:
With the LIGOVirgo detectors currently undergoing their 4th observing round, gravitationalwave astronomy has matured into a fastdeveloping field with broad implications for astrophysics, nuclear physics, gravity and cosmology. In this talk, I will focus on recent developments in probing the physics of black holes and their mergers with gravitational waves. This includes measurements of black hole spins and merger kicks, their use as cosmological probes, and the spectroscopic study of ringing black holes. I will outline some of the theoretical and observational questions driving this field: how do black holes form? Can we leverage them as probes of new fundamental fields, dark matter or cosmic expansion? I will conclude by arguing that we are at the cusp of observationally tackling these and many other fascinating questions as we enter the era of precision gravitationalwave science, with current and future observatories in space and on the ground. 
Gravity Seminar Monday, March 25, 2024 1:30 PM Physics, Room 323 
"Gravitationalwave signatures of the darkmatter environments around black hole binaries"Benjamin Wade , UVAPhysics [Host: David Nichols]
ABSTRACT:
Massive black holes can grow in the presence of darkmatter environments and form darkmatter spikes with large densities. When a massive black hole within a darkmatter environment is part of an inspiral with a second compact object, the environmental effects will be imprinted on the system's dynamics. Past work studying these systems has demonstrated that gravitational effects like dynamical friction and accretion effects from the darkmatter distribution can have measurable impacts on the binary inspiral rate. The emitted gravitational waves will be affected in turn; given that they will be in the observable band for upcoming spacebased detectors like LISA, the dynamics of dark matter on these scales can be understood precisely. In this talk, I discuss progress in evolving these systems on three fronts. First, I will overview a generalization of dynamical friction suitable for spherical systems, and its applications to inspirals. Second, I will present refinements on the effects of darkmatter accretion in a selfconsistent framework. Finally, I will discuss the impacts of the formation history of the system on both the resulting darkmatter distribution and the gravitational waveform we would detect from such a binary. 
Gravity Seminar Monday, March 18, 2024 1:30 PM Physics, Room 031 
ABSTRACT:
Neutron stars are some of the most compact objects in the universe, second only to black holes. Their interior composition remains a mystery, but studies of neutron stars and pulsars can allow scientists to probe the dense nuclear regions within. These investigations often lead to bounds on a neutron star mass, which can be compared with a given equation of state to provide the physical characteristics of a star. In this talk, I'll speak about some work following up one of the most massive neutron stars ever measured, J0348+0432, and provide an update into the mass estimates. This work was carried out with the Canadian Hydrogen Intensity Mapping Experiment (CHIME) telescope as well as archival data provided by the Arecibo Observatory and the Green Bank Telescope. We have found that new estimates place a mass considerably lower than the original estimate likely due to a mismodeling of the white dwarf companion mass. A discussion of how this happened as well as the consequences of this new revelation will also be discussed. 
Gravity Seminar Monday, March 11, 2024 1:30 PM Physics, Room 323 
"Towards Tests of General Relativity with Gravitational Waves from Precessing Binaries"Nicholas Loutrel , University of MilanoBicocca) [Host: Kent Yagi]
ABSTRACT:
Compact objects possessing complicated multipole structure will generally cause precession of the orbital plane when present in a binary system. The most common example of this within general relativity is socalled spin precession, which is caused when the spin angular momentum of the compact object couple to each other, as well as the orbital angular momentum. The precession of the latter of these induces modulations in both the frequency and amplitude of the observed gravitational wave emission of the binary, effects which play a crucial role in parameter estimation. However, if general relativity is not the correct theory of gravity at astrophysical scales and must be modified, or the compact objects have significantly more complicated multipole structure beyond that of a simple poledipole, the precession dynamics of the binary will also be modified from that of standard spin precession. Such modifications will necessarily be imprinted in the waveform generated by the precessing binary, opening the door to performing tests of general relativity within the precessing sector of binary dynamics. 
Gravity Seminar Monday, January 22, 2024 12:30 PM , Room Zoom Join Zoom Meeting https://virginia.zoom.us/j/96623644155?pwd=MzFGMnEvTWwrVDU5L3JRdnVqOVJnUT09
Meeting ID: 966 2364 4155 Passcode: 813439 
"Black hole dynamics in Effective Field Theory extensions to General Relativity"Ramiro Cayuso , Perimeter Institute [Host: Kent Yagi]
ABSTRACT:
Gravitational wave (GW) astronomy has opened a new window for studying gravitational phenomena in its strongfield and highly dynamical regime. In this regime, the detection of GWs originating from the mergers of compact binary systems represents the most compelling probe to explore the extreme manifestations of gravity and possible deviations from GR. In this talk, I will present the formal and practical challenges that arise in nonlinear studies of modified gravity theories. In particular, I will present the results from numerical simulations where the implementation of novel methods can help us get accurate predictions in the nonlinear regime for modified gravity theories motivated by Effective Field Theory arguments. 
Gravity Seminar Monday, December 4, 2023 1:30 PM , Room Zoom Join Zoom Meeting: https://virginia.zoom.us/j/91362126597?pwd=NlpubmZLeXJRNGpXa1lNdFdGSjJtdz09 Meeting ID: 913 6212 6597 Passcode: 335724 
"Gravitational wave memory, soft gravitons theorems and looking for gravitons in gravitational waves"Subhendra Mohanty , IIT Kanpur [Host: David Nichols]
ABSTRACT:
I will discuss a field theory treatment of standard gravitational waves calculations. Using the QFT formalism we can connect the gravitational memory signal with what are called 'softgraviton theorems' which gives an insight into the origin of the memory signal and makes the calculations easier in some cases. I will also discuss if the graviton nature of gravitational waves can be proved using the existing gravitational wave detection experiments. 
Gravity Seminar Thursday, November 30, 2023 2:00 PM Astronomy Building, Room 201 
"Interpreting the multimessenger picture drawn by compact binary mergers"Tim Dietrich , University of Potsdam [Host: David Nichols]
ABSTRACT:
Neutron stars are among the most compact objects in the Universe, and the collision of two neutron stars is among the most energetic events in our Universe. In 2017, the multimessenger detection of gravitational waves and electromagnetic signals from such a collision has been a revolution in astronomy and provided a wealth of information about fundamental physics principles. Essential for an accurate interpretation of binary neutron star mergers are reliable models describing the last stages of their coalescence. We show how numericalrelativity simulation can be used to derive such theoretical models for the gravitationalwave and electromagnetic signatures. We employ these models together with nuclearphysics computations and experimental data to measure the equation of state of neutron stars, understand heavy element production, and to provide new constraints on the Hubble constant. 
Gravity Seminar Monday, November 6, 2023 1:30 PM , Room Zoom Join Zoom Meeting https://virginia.zoom.us/j/99489466312?pwd=SUVJdXJSNWFObXVJMDJZUml2aUE3QT09
Meeting ID: 994 8946 6312 Passcode: 237833 
"Neutron Stars and White Dwarf Mergers: An Emerging Multimessenger View"Rahul Kashyap , Penn State University [Host: Sayantani Datta]
ABSTRACT:
Neutron stars and white dwarfs contain densest matter known to us in the universe. This brings gravity in a tug of war with nuclear, electromagnetic and weak interactions which keep these stars from collapsing. The merging of these compact objects in binary systems generates signals detectable across various observational windows, thereby broadening and enriching the realm of multimessenger astronomy. In this talk, I will illustrate how largescale computational frameworks serve as valuable tools for exploring the intricate interplay of these fundamental interactions and aiding in scientific discovery. I will also present the data analysis techniques to extract information from current and future gravitational wave observations. We will focus on kilonovae and gravitational waves produced by colliding neutron stars, as well as Type Ia supernovae triggered by the mergers of binary white dwarfs. I will present our evolving understanding of these systems and some future directions that the field is going towards. 
Gravity Seminar Monday, October 23, 2023 1:30 PM , Room Zoom Join Zoom Meeting https://virginia.zoom.us/j/96998855899?pwd=dzhsUG5qRHVacDZoOWdMUFlMeVJMZz09
Meeting ID: 969 9885 5899 Passcode: 495311 
"Gravitational Wave Memory Beyond General Relativity"Jann Zosso , ETH Zurich; University of Illinois UrbanaChampaign [Host: Kent Yagi]
ABSTRACT:
The gravitational wave memory effect that manifests itself as a permanent distortion of space after a gravitational wave burst, is a prediction of GR, whose detection is expected to be around the corner. In this talk, I will present recent work, in which the memory effect of a broad class of beyond GR metric theories of gravity is shown to be modified primarily through the presence of additional propagating modes in the theory. This strongly suggests the possibility of using memory observations as a model independent test of the number of dynamical gravitational degrees of freedom. Such a general statement rests upon a reinterpretation of the memory effect as naturally arising within the broadly applicable Isaacson approach to gravitational waves. 
Gravity Seminar Thursday, April 27, 2023 2:00 PM , Room Virtual https://us02web.zoom.us/j/83990634739?pwd=SnQ4M09wd0NYQzFld2Zzc08raElRdz09 Meeting ID: 839 9063 4739 Passcode: 576874 
"Astrophysical Lessons from LIGOVirgoKAGRA's Black Holes"Maya Fishbach , University of Toronto [Host: Kent Yagi]
ABSTRACT:
The LIGOVirgoKAGRA Collaboration has observed over 70 gravitationalwave sources to date, including mergers between black holes, neutron stars, and mixed neutron star—black holes. Focusing on the black hole mergers, I will describe some recent lessons into how, when, and where black holes are made. These questions are connected to several astrophysical puzzles, including the deaths of massive stars, the growth of black holes across cosmic time, highredshift star formation, and properties of globular clusters. 
Gravity Seminar Monday, April 10, 2023 1:30 PM , Room Zoom https://us02web.zoom.us/j/86764277969?pwd=UnJDOVVlalU3bTdwZFptbzBqQkJnQT09 Meeting ID: 867 6427 7969 Passcode: 906268 
"Towards Gravitational Wave Asteroseismology with Compact Binary Inspirals"Geraint Pratten , University of Birmingham [Host: David Nichols]
ABSTRACT:
Gravitational wave observations of neutron star mergers are one of the most exciting prospects for constraining the incredibly uncertain equation of state of cold supranuclear matter. Signatures of the stellar interior are directly imprinted in the gravitationalwave signal through characteristic tidal interactions, providing a vital observational playground in our quest to understand fundamental physics interactions deep in the cores of neutron stars. In this talk I will discuss the underlying physics behind binary neutron star mergers and how recent developments are showcasing the importance of describing the dynamical response of neutron stars when studying gravitationalwave observations. Finally, I will highlight the prospects for performing gravitationalwave asteroseismology with binary neutron star inspirals in current and future detector networks. 
Gravity Seminar Monday, March 27, 2023 1:30 PM , Room Zoom Meeting ID: 979 7765 8329
https://virginia.zoom.us/j/97977658329?pwd=cDluSDJ0QlUzV3M0dWhHODVGc1FFQT09 
"A study of gravitational wave memory effects in radiative geometries and wormholes "Indranil Chakraborty , IIT Kharagpur [Host: David Nichols]
ABSTRACT:
Gravitational memory effects are persistent deformations caused due to the passage of a gravitational wave pulse. It is a nonlinear effect in General Relativity that remains yet to be detected. In this talk, primarily from a theoretical perspective, we study memory effects in two different settings: i) Radiative geometries, ii) Lorentzian wormholes. In radiative geometries, we show how geodesic and geodesic deviation equations encode the gravitational wave memory. In the latter case, we perform a BondiSachs analysis and try to show how the Bondi mass loss depends on the wormhole hair. 
Gravity Seminar Monday, March 20, 2023 1:30 PM , Room Zoom Join Zoom Meeting https://virginia.zoom.us/j/97977658329?pwd=cDluSDJ0QlUzV3M0dWhHODVGc1FFQT09
Meeting ID: 979 7765 8329 Passcode: 357957 
"Hypermassive neutron stars and short gamma ray bursts"Cecilia Chirenti , University of Maryland [Host: Kent Yagi]
ABSTRACT:
Gamma ray bursts (GRBs) are the most luminous electromagnetic events in the universe. Short GRBs, typically lasting less than 2 seconds, have already been associated with binary neutron star (BNS) mergers, which are also sources of gravitational waves (GWs). The ultimate fate of a BNS, after coalescence, is usually expected to be a black hole (BH) with 23 solar masses. However, numerical relativity simulations indicate the possible formation of a shortlived hypermassive neutron star (HMNS), lasting for tens to hundreds of milliseconds after the BNS merger and before gravitational collapse forms a BH. The HMNS is expected to emit GWs with kHz frequencies that will be detectable by third generation groundbased GW detectors in the 2030s. I will present results from a recent analysis that revealed evidence for HMNSs by looking for kHz qusiperiodic oscillations in gammaray observations obtained in the 1990s with the Compton Gamma Ray Observatory. 
Gravity Seminar Monday, March 13, 2023 1:30 PM Physics, Room 313 
"Gravitational Faraday rotation of gravitational waves by a Kerr black hole"Zhao Li , University of Science and Technology of China [Host: Kent Yagi]
ABSTRACT:
Gravitational Faraday Rotation (GFR) is a framedragging effect induced by rotating massive objects, which is one of the important characteristics of lensed gravitational waves (GWs). In my previous work, we calculate the GFR angle of GWs in the weak deflection limit, assuming it is lensed by a Kerr black hole (BH). We find that the GFR effect changes the initial polarization state of the lensed GW. Compared with the Einstein deflection angle, the dominant term of the rotation angle is a secondorder correction to the polarization angle, which depends on the lightofsight component of BH angular momentum. Such a rotation is tiny and degenerates with the initial polarization angle. In some critical cases, the GFR angle is close to the detection capability of the thirdgeneration GW detector network, although the degeneracy has to be broken. 
Gravity Seminar Monday, March 6, 2023 1:30 PM , Room Zoom https://us02web.zoom.us/j/86544012000?pwd=ckJpMTY5L0dIbHc5WTZxNFMvM1lkdz09 Meeting ID: 865 4401 2000 Passcode: 033748 
"Gravitational waves from a particle physics perspective"Jan Steinhoff , Max Planck Institute for Gravitational Physics [Host: David Nichols]
ABSTRACT:
Continuing the success of gravitational wave observations demands considerable improvements of their theoretical predictions in the next decade, in order to keep their accuracy on par with upgrades of the detectors. This urges innovations on the methods by which gravitational waves from compact binaries are calculated. In this talk, we focus on approaches to analytic, perturbative predictions for relativistic binaries inspired by highenergy physics. In this area, effective field theories are highly useful and scattering amplitudes (the primary observable) can be calculated very efficiently using novel tools. These methods can indeed be applied the classical binaries and their gravitational waves. We give a basic introduction to the ideas of these approaches and recent progress. 
Gravity Seminar Monday, February 27, 2023 1:30 PM Clark Hall  Virtual talk, Room 108 Join Zoom Meeting https://virginia.zoom.us/j/97977658329?pwd=cDluSDJ0QlUzV3M0dWhHODVGc1FFQT09
Meeting ID: 979 7765 8329 Passcode: 357957 
"NextGeneration Black Hole and Neutron Star Collision Simulations"Zachariah Etienne , University of Idaho [Host: Alexander Grant]
ABSTRACT:
Perhaps the most significant astronomical discovery of our lifetimes, codenamed GW170817, involved the collision of two neutron stars. The collision was detected both by gravitational wave observatories, and traditional electromagnetic telescopes. As neutron stars are made of the densest form of matter in our current Universe, this single "multimessenger" event was a watershed moment in our understanding as to how matter and gravity behave at their most extreme, far beyond what we can study in laboratories on Earth. For the most part, we compare observations against theoretical models to extract science from events like this. Unfortunately, these theoretical models are severely limited both in quality and quantity, leading to a critical need to improve them. Such improvements pose a key challenge to computational astrophysics, as our most detailed models require expensive supercomputer simulations that generate full, nonperturbative solutions of the general relativistic field equations (numerical relativity). After a gentle introduction to multimessenger astrophysics and the challenges associated with multimessenger source modeling, I will outline a new approach aimed at greatly reducing the cost of these simulations. With the reduced cost comes the potential to both perform colliding black hole simulations on the consumergrade desktop computer, as well as add unprecedented levels of physical realism to colliding neutron star simulations on supercomputers. 
Gravity Seminar Monday, February 13, 2023 1:30 PM Physics, Room Zoom Zoom link: https://virginia.zoom.us/j/99508589926?pwd=TUFNMDJZMjZRUTJnaFd3TDgxNi9KZz09 Meeting ID: 995 0858 9926 Password: 441596 
"Observational consequences of nonlinear memory of gravitational waves"Shubhanshu Tiwari , University of Zurich [Host: Alexander Grant]
ABSTRACT:
Nonlinear memory is one of the most intriguing predictions of general relativity which is generated by the passage of gravitational waves (GWs) leaving the spacetime permanently deformed. For example a GW signal from binary black hole (BBH) will have two parts the oscillatory part which is known as the “chirp” and a much fainter nonoscillatory (DC like) part which is nonlinear memory. A nonlinear memory is produced by all the sources of GWs and has the peculiarity that even if the oscillatory part of the source lies at high frequency the nonlinear memory will be available at low frequency. This property of nonlinear memory makes it a valuable resource for GW astronomy. In this talk I will provide and introduction to how we can use gravitational waves memory as a resource for the current and future ground based detectors. To do this I will show examples of how one can creatively use the nonlinear memory to probe seemingly inaccessible sources of GWs like ultra low mass compact binary mergers where the oscillatory part lies at outside the reach of any current detectors and only nonlinear memory could be detected if these sources exist. Another example will be the matter effects from binary neutron stars and black hole neutron star binaries which are at high frequency but the nonlinear memory is accessible. I will also discuss the postmerger neutron star memory and the prospects of its detection. 
Gravity Seminar Monday, January 30, 2023 1:30 PM Physics, Room Zoom Zoom link: https://virginia.zoom.us/j/96960494406?pwd=MFBMaDRvb1BQc1V3RVRpcm14eVdCQT09 Meeting ID: 969 6049 4406 Passcode: 287180 
"Machine Learning for Gravitational Wave Astronomy "Stephen Green , University of Nottingham [Host: Alexander Grant]
ABSTRACT:
Since 2015, the LIGOVirgoKAGRA Collaboration has detected 90 signals from merging compact objects such as black holes and neutron stars. Each of these is analyzed using Bayesian inference, employing a stochastic algorithm such as Markov Chain Monte Carlo to compare data against models—thereby characterizing the source. However, this is becoming extremely costly as event rates grow with improved detector sensitivity. In this talk I will describe a powerful alternative using probabilistic deep learning to analyze each event in orders of magnitude less time while maintaining strict accuracy requirements. This uses simulated data to train a normalizing flow to model the posterior distribution over source parameters given the data—amortizing training costs over all future detections. I will also describe the use of importance sampling to establish complete confidence in these deep learning results. Finally I will describe prospects going forward for simulationbased inference to enable improved accuracy in the face of nonstationary or nonGaussian noise. 
Gravity Seminar Monday, December 5, 2022 1:30 PM Physics, Room via Zoom (Zoom link and meeting ID provided below) Meeting link: https://virginia.zoom.us/j/94422619812?pwd=L3RCS1FoZXliZzJ0Q3FQNDl3c0RUdz09
Passcode: 507640

"Ringdown overtones in black hole binary mergers"Roberto Cotesta , John Hopkins University [Host: Kent Yagi]
ABSTRACT:
The gravitationalwave signal emitted by the blackhole remnant resulting from a binary merger such as GW190514 consists in a superposition of damped sinu soids known as quasinormal modes. Besides the “fundamental" mode (the one with the longest damping time), it is important to detect the socalled “over tones" (modes with shorter damping time), because a measurement of their frequencies could allow us to identify the remnant as a Kerr black hole. We discuss theoretical and observational issues in the analysis of ringdown over tones. We present theoretical arguments showing that the spacetime is not well described as a linearly perturbed black hole close to the peak of the waveform amplitude. Then we analyze GW150914 postmerger data to understand if recent ringdown overtone detection claims are robust. We find no evidence in favor of an overtone in the data after the waveform peak. Around the peak, the logBayes factor does not indicate the presence of an overtone, while the support for a nonzero amplitude is sensitive to changes in the starting time much smaller than the overtone damping time. This suggests that claims of an overtone detection are noisedominated. We perform GW150914like injections in neighboring segments of the real detector noise, and we show that noise can indeed induce artificial evidence for an overtone.

Gravity Seminar Monday, November 21, 2022 1:30 PM Physics, Room 313 
"Surrogate models, methods, and applications: Learning highfidelity gravitationalwave models from numerical relativity data"Scott Field , University of Massachusetts [Host: Alexander Grant]
ABSTRACT:
Recently there has been significant interest in building datadriven gravitationalwave models directly from numerically generated data. These surrogate (or reducedorder) models can faithfully reproduce a parameterized gravitational wave model specified through computationally expensive ordinary or partial differential equations with significant speedups. Surrogates can be used, for example, to accelerate the generation of effective onebody or numerical relativity (NR) waveform models, thereby reducing the overall runtime of a multiquery data analysis study. In this talk, I will summarize the key algorithms and approaches toward building surrogate models as well as survey recent models that cover more of the binary black hole parameter space, including precession, eccentricity, and large to extrememass ratio systems. For surrogates to be useful, it is necessary that they be publicly available, easytouse, and decoupled from the building codes which produce them. In this talk, I will also describe a lightweight opensource code, GWSurrogate, which addresses this issue and enables surrogate models to be used in gravitationalwave data analysis studies. Some preliminary results for reanalyzing GWTC3 will also be shown. 
Gravity Seminar Monday, November 7, 2022 1:30 PM Physics, Room 313 
Available
ABSTRACT:
Available 
Gravity Seminar Monday, October 31, 2022 1:30 PM Physics, Room https://virginia.zoom.us/j/92309274285?pwd=WU9IS3NGa3hKRUdnanN6N 
"Infrared Finite Scattering Theory in QFT and Quantum Gravity"Gautam Satishchandran , Princeton University [Host: Alexander Grant]
ABSTRACT:
A longstanding problem in QFT and quantum gravity is the construction of an "IRfinite" Smatrix. In the gravitational case, the existence of these "infrared divergences" is intimately tied to the "memory effect" (i.e. the permanent displacement of test masses due to the passage of a gravitational wave) and the existence of an infinite number of conserved charges at spatial infinity. In this talk, I shall explain the origin of these connections and illustrate that the construction of an IRfinite Smatrix requires the inclusion of states with memory (which do not lie in the standard Fock space). In massive QED an elegant solution to this problem was provided by Faddeev and Kulish who constructed an incoming/outgoing Hilbert space of charged particles "dressed" with memory. However, we show that this construction fails in the case of massless QED, YangMills theories, linearized quantum gravity with massless/massive sources, and in full quantum gravity. In the case of quantum gravity, we prove that the only "FaddeevKulish" state is the vacuum state. We also show that "nonFaddeevKulish" representations are also unsatisfactory. Therefore, in full quantum gravity, it seems that there does not appear to be any (separable) Hilbert space of incoming/outgoing states that can accommodate all scattering states. Therefore we argue that, if one wants to treat scattering theory at a fundamental level, one must take an "algebraic approach" which does not require an a priori choice of Hilbert space. We outline the framework of such a manifestly IRfinite scattering theory. 
Gravity Seminar Monday, October 24, 2022 1:30 PM Physics, Room 313 
ABSTRACT:
The final phase of gravitational radiation from black hole binaries is the ringdown of the merged black holes, which occurs at a characteristic set of frequencies. Measurements of the ringdown spectrum can provide especially clean tests of the nature of the final black hole, potentially revealing violations of the famous "nohair" theorem. The large number of gravitational wave observations that will be made in the coming years together with recent advances in the analysis of ringdown indicate that precision tests will be possible in the near future. Going beyond null tests, however, requires predictions of the ringdown spectrum in theories beyond GR and in spacetimes beyond Kerr. In this talk I will outline a flexible approach for calculating the ringdown spectrum of spinning black holes in theories where deviations from GR are small, and discuss future prospects for precision ringdown tests. 
Gravity Seminar Monday, October 10, 2022 1:30 PM Physics, Room 313 
"Observational signatures of tidal deformability in compact objects"CarlJohan Haster , MIT Kavli Institute for Astrophysics and Space Research [Host: Alexander Saffer]
ABSTRACT:
After having observed gravitational waves from a population of nearly 100 compactobject binaries, we are now in a position where we can start probing their internal structure and how they can be deformed by the strong tidal fields in which the binaries exist. I will present current observational constraints of the Neutron Star Equation of State from gravitationalwave observations, and discuss some of the potential complications and limitations the observations over the coming years might bring as the sensitivity of the gravitationalwave detectors are improved. I will also showcase a study about what possibilities the next generation of gravitationalwave detectors will bring, and what being able to observe a population of neutron stars at cosmological distances will teach us. Finally, I will present a study focusing on the observed “nonNeutron Stars”, and if they can be described as compact objects other than Black Holes. This can be done by extending the Black Hole description to also allow for them to be tidally deformed following the behavior of a uniformdensity ultracompact star (Schwarzschild star). Assuming that the population of Binary Black Holes, as observed in gravitational waves instead can be described as binaries of these Schwarzschild stars I present strong constraints on their compactness and tidal deformability, both as individual objects and for the population at large. Through these constraints, I comment on the viability of other categories of Black Hole mimickers as constituents of the ultracompactobject binaries observed so far. 
Gravity Seminar Monday, May 2, 2022 1:30 PM Physics, Room 313 
"Gravitationalwave multimessenger observations: from the production of gold to the age of the Universe"HsinYu Chen , MIT  Massachusetts Institute of Technology [Host: Alexander Saffer]
ABSTRACT:
The detections of gravitational waves from compact binary mergers and the followup observations of electromagnetic emissions together provide a powerful and independent tool to explore the Universe. With successive upgrades to the LIGO and Virgo sensitivities, and hence a growing number of detections, we are prepared to address a number of major questions in astrophysics. In this talk, I will discuss two topics in which I expect critical progress will be made in the next few years: (i) How do we make precise and accurate Hubble constant measurements with gravitationalwave events? (ii) What can we learn about neutron star nuclear physics from gravitationalwave observations? I will close with my outlook on the immense scientific opportunities that the nextgeneration gravitationalwave detectors will provide. 
Gravity Seminar Monday, April 18, 2022 11:00 AM Physics Building, Room 313 
"Binaryblackhole systems in general relativity"Arwa Elhashash , University of Virginia  Department of Physics [Host: Prof. David Nichols]
ABSTRACT:
Studying binaryblackhole systems has long been of great interest in general relativity, and is even more so after the first observed event in 2015 discovered by LIGO. 
Gravity Seminar Monday, April 4, 2022 1:30 PM Physics, Room 313 
"Black Holes and Compact Objects in GravitationalWave Astronomy"Horng Sheng Chia , Institute for Advanced Study [Host: Alexander Grant]
ABSTRACT:
Gravitational wave astronomy offers us a unique probe onto the nature of astrophysical bodies in coalescing binary systems. As a binary approaches merger, its dynamics is sensitive to various socalled "finitesize effects" of the binary constituents, which leave measurable imprints on waveforms. In this talk, I will first discuss the finitesize effects of Kerr black holes, focusing on their tidal response to a perturbing companion where most of recent progress has been made. I will then describe recent efforts to use these finitesize effects to detect new types of compact objects in the data. 
Gravity Seminar Monday, March 28, 2022 1:30 PM Online, Room via Zoom Join Zoom Meeting: https://virginia.zoom.us/j/98187156266Meeting ID: 981 8715 6266 Passcode: 569653 
"The imprints of stellar oscillations in gravitational wave signals from binary compact stars"Shu Yan Lau , University of Virginia  Department of Physics [Host: Prof. Kent Yagi]
ABSTRACT:
In this talk, I will present two separate projects related to the imprints of stellar oscillations on the gravitational wave (GW) signals. In the first project, we consider the signals from binary hybrid star (HS) coalescence events. The HS is a special type of neutron star which core is made of deconfined quark matter. We show that the HSs have a special oscillation mode associated with the nuclear matterquark matter phase transition that can potentially resonate during the inspiral stage, producing effects in the GW signal measurable by the groundbased detectors. In the second project, we study the effect of dynamical tide on eccentric binary white dwarf systems. We show that the nonresonant buildup of the oscillation modes can produce an orbit precession resolvable by the upcoming spacebased GW detector. For orbits with high eccentricities and small pericenter separations, it can even cause the waveform to become chaotic. 
Gravity Seminar Monday, March 21, 2022 1:30 PM Physics, Room 313 
ABSTRACT:
Gravitational waves (GWs) allow us to probe the content of the Universe and the behaviour of gravity on cosmological scales, through information contained in their propagation. In this talk, I will discuss particular cosmological scenarios where GWs interact with another tensorlike field, such as in the theory of massive bigravity. I will illustrate explicitly how the GW signal from a coalescence of black holes evolves during cosmological propagation, which could exhibit phase distortions and echoes of the GW signal emitted. These strong features suggest that stringent constraints on interacting GWs can be placed with current and future GW detectors. 
Gravity Seminar Monday, March 14, 2022 1:30 PM Physics, Room 313 
"Probing subatomic physics with gravitational waves from neutron star binary inspirals"Dr. Tanja Hinderer , Utrecht University [Host: Alexander Saffer]
ABSTRACT:
The gravitational waves from merging binary systems carry unique information about the internal structure of compact objects. This is of key interest for neutron stars, whose material is compressed by their tremendous gravity to supranuclear densities. Under such extreme conditions we expect novel, unexplored phases of matter to emerge. In this talk, I will describe examples of how the matter properties and their interplay with strongfield gravity leads to characteristic signatures in the gravitational waves. I will also highlight new insights gained from recent gravitationalwave discoveries, and conclude with an outlook onto the remaining challenges and exciting prospects for the next years, as gravitationalwave science continues to move towards an era of precision physics. 
Gravity Seminar Monday, February 28, 2022 1:30 PM Online, Room via Zoom Join Zoom Meeting:https://virginia.zoom.us/j/97128942029Meeting ID: 971 2894 2029 Passcode: 200012 
ABSTRACT:
TBA 
Gravity Seminar Monday, February 14, 2022 1:30 PM Physics, Room 313 
"Gravitational waveforms for compact binaries from secondorder selfforce theory "Barry Wardell , University College Dublin [Host: Alexander Grant]
ABSTRACT:
Extreme mass ratio inspirals (EMRIs) are expected to be a key source of gravitational waves for the LISA mission. In order to extract the maximum amount of information from EMRI observations by LISA, it is important to have an accurate prediction of the expected waveforms. In particular, it will be necessary to have waveforms that incorporate effects that appear at second order in the mass ratio. In this talk I will present the latest progress towards this goal, including recent results for the secondorder gravitationalwave energy flux and for the gravitational waveform. 
Gravity Seminar Monday, January 31, 2022 1:30 PM Online, Room via Zoom Join Zoom Meeting:https://virginia.zoom.us/j/97270745862Meeting ID: 972 7074 5862 Passcode: 567149 
"Test of black hole firewall hypothesis by electromagnetic emissions"Sudipta Hensh , Silesian University [Host: Prof. Kent Yagi]
ABSTRACT:
A recent "firewall" proposal claims to have settled the black hole information paradox. It suggests that an infalling observer is expected to encounter highenergy quanta in a region near the horizon. The fate of the observers or the very existence of the ‘’firewall’’ itself is still up for debate. Leaving those aside, we are interested in understanding observational signatures of the ‘’firewall’’ at the classical level. With this motivation, we consider a reflective ‘’firewall’’ just outside the event horizon of a Kerr black hole. I will discuss the results of our model and imprint of the ‘’firewall’’ leaves on the emissionline profile of a radiating Keplerian disk. The optical appearance of the black holeaccretion disk system will also be discussed in this context. 
Gravity Seminar Monday, January 24, 2022 1:30 PM Online, Room via Zoom Join Zoom Meeting:https://us02web.zoom.us/j/84365378162Meeting ID: 843 6537 8162 Passcode: 881928 
"Probing neutron star matter with gravitational waves"Philippe Landry , Canadian Institute for Theoretical Astrophysics [Host: Alexander Grant]
ABSTRACT:
Neutron stars harbor the densest matter in the Universe. Its precise composition and structure are unknown because laboratory experiments cannot reproduce the extreme conditions in neutron star cores. Gravitational waves from neutron star mergers, on the other hand, directly probe the core matter as they carry imprints of tidal interactions that depend on the stars' internal structure. In this talk, I will describe how gravitationalwave observations, complemented by radio and xray pulsar measurements, are shedding light on the neutron star interior, revealing hints about nuclear interactions, phase transitions and exotic matter. I will also discuss applications of improved dense matter knowledge towards open questions in astrophysics. 
Gravity Seminar Monday, December 6, 2021 1:00 PM Online, Room via Zoom Join Zoom Meeting: https://virginia.zoom.us/j/95625108281Meeting ID: 956 2510 8281 Passcode: 864174 
"Symmetries and Charges of Gravitational Subsystems"Venkatesa Chandrasekaran , Institute for Advanced Study [Host: Alexander Grant]
ABSTRACT:
Gravitational subsystems, such as black holes, are important objects of study in both classical and quantum gravity. Insight into the gravitational degrees of freedom of a subsystem can be gained by analyzing the symmetries and charges of gravity in the associated spacetime subregion. In this talk, I will use the covariant phase space formalism to make progress on this problem in general relativity, with a particular focus on subregions bounded by null hypersurfaces, such as event horizons or causal diamonds. Surprisingly, on null surfaces the gravitational field will turn out to have infinitely many symmetries, akin to the BMS symmetries at null infinity. In a completely general setting in which the subsystem can emit or absorb radiation, I will then derive an infinite set of charges and conservation laws on the null surface, and explain their significance for physics deep in the gravitational field. Finally, I will describe progress towards an understanding of black hole entropy through this formalism. 
Gravity Seminar Monday, November 15, 2021 1:00 PM Online, Room via Zoom Join Zoom Meeting: https://virginia.zoom.us/j/92573320085 Meeting ID: 925 7332 0085 Passcode: 208444

"Aspects of Rotating Black Holes in Dynamical ChernSimons Gravity"Leah Jenks , Brown University [Host: Kent Yagi]
ABSTRACT:
In this talk I will give an overview of recent and ongoing work regarding rotating black holes in dynamical ChernSimons (dCS) gravity. dCS gravity is a well motivated modified theory of gravity which has been extensively studied in gravitational and cosmological contexts. I will first discuss unique geometric structures, `the ChernSimons caps,' which slowly rotating black holes in dCS gravity were recently found to possess. Motivated by the dCS caps, I will then discuss superradiance in the context of slowly rotating dCS black holes and show that there are corrections to the usual solution for a Kerr black hole. Lastly, I will comment on the observable implications for these corrections and point towards avenues for future work. VIDEO:

Gravity Seminar Monday, November 8, 2021 1:00 PM Online, Room via Zoom Join Zoom Meeting: https://us02web.zoom.us/j/89487769062Meeting ID: 894 8776 9062 Passcode: 287799 
"Black hole hair: from nohair theorems to scalarization"Professor Thomas Sotiriou , The University of Nottingham [Host: Alexander Saffer]
ABSTRACT:
In general relativity black holes are fully characterised by their mass, spin, and electromagnetic charge. Nohair theorems indicate that scalar fields cannot affect black hole spacetimes. However, the devil is in the details and, in practice, nohair theorems allow us to identify a list of interesting exceptions in which scalar field leave their imprint on black holes. Such scenarios are of particular interest to gravitational wave searches for new fundamental physics. I will give an overview of how new fundamental scalars affect black hole spacetimes and of how this can be imprinted on gravitational wave observations. 
Gravity Seminar Monday, November 1, 2021 1:00 PM Online, Room via Zoom Join Zoom Meetinghttps://virginia.zoom.us/j/94853461679Meeting ID: 948 5346 1679 Passcode: 780696 
"Gravitational radiation from a binary black hole coalescence in EinsteinscalarGaussBonnet gravity"FelixLouis Julie , Johns Hopkins University [Host: Alexander Saffer]
ABSTRACT:
I will show how to derive analytic gravitational waveforms associated to the coalescence of a “hairy” black hole binary in EinsteinscalarGaussBonnet gravity (ESGB). I will present the ESGB postNewtonian (PN) Lagrangian and gravitational wave fluxes. The PN framework relies on reducing the black holes to point particles with scalarfielddependent masses. In light of the first law of thermodynamics of ESGB black holes, I will show that this procedure amounts to fixing their Wald entropies. As a consequence, inspiraling ESGB black holes can grow scalar “hair” until they turn into naked singularities. I will then extend the scope of the PN approximation to the strong field regime near merger by generalizing the EffectiveOneBody (EOB) formalism to ESGB gravity. 
Gravity Seminar Monday, October 18, 2021 1:00 PM Online, Room via Zoom Join Zoom Meetinghttps://virginia.zoom.us/j/98368369604Meeting ID: 983 6836 9604 Passcode: 130144 
"Resonances in black hole spacetimes"Dr. BÃ©atrice Bonga , Radboud University [Host: Alexander Grant]
ABSTRACT:
Resonances are ubiquitous in nature. In this talk, I will focus on resonances due to the interaction of two black holes orbiting a central massive black hole. Such tidal resonances will generically occur for EMRIs if nearby compact objects exist. By probing their influence on the phase of the EMRI waveform, we can in principle extract information about the environmental tidal field of the EMRI system, albeit at the cost of a more complicated EMRI waveform model. I will also describe mean motion resonances, which are a mechanism that can create the necessary conditions for tidal resonance to occur. 
Gravity Seminar Monday, October 4, 2021 1:00 PM Online, Room via Zoom Join Zoom Meetinghttps://virginia.zoom.us/j/92281876173Meeting ID: 922 8187 6173 Passcode: 606888 
"Highperformance Gravitational Wave Extraction in SpECTRE"Jordan Moxon , California Institute of Technology [Host: Alexander Grant]
ABSTRACT:
Numerical relativity stands as the primary method of generating precise waveform predictions for comparablemass compact binary coalescences used in gravitational wave data analysis pipelines. To produce those predictions, the spacetime in the vicinity of the binary system must be simulated to high precision, and then the waveform information must be extracted from the dynamical spacetime near the binary. Cauchy Characteristic Evolution (CCE) offers a wave extraction method capable of efficiently determining a complete, asymptotically wellbehaved metric at Scri+. For our implementation of CCE in SpECTRE, we have developed a number of mathematical refinements of the CCE system that improves spectral convergence and eases the computation of detailed dynamical spacetime information at Scri+. Our implementation in SpECTRE is far faster than previous CCE codes, is free from logarithmic pathologies, and computes full waveform information: news, strain, and all five Weyl scalars. I will discuss the numerical methods used to improve the performance of SpECTRE CCE, as well as several projects that have used the system to study gravitational wave memory and other subtle waveform effects that become available with full access to waveform data at Scri+. VIDEO:

Gravity Seminar Monday, April 26, 2021 1:00 PM Online, Room Zoom Join Zoom Meetinghttps://virginia.zoom.us/j/98166651049Meeting ID: 981 6665 1049 Passcode: 726235 
"Formation and dynamics of extreme mass ratio inspirals with environmental effects"Huan Yang , Perimeter Institute and University of Guelph [Host: Alexander Grant]
ABSTRACT:
In this talk I will discuss relevant environment effects (i.e., accretion disk, tidal gravitational field from close objects) that influence the formation and dynamics of extreme mass ratio inspirals (EMRIs), which are important sources for LISA. I will show that diskassisted EMRIs may be more commonly seen by LISA. They can be distinguished from EMRIs formed through cluster multibody scattering by eccentricity measurements. The disk force and tidal gravitational field from nearby objects may also leave observable imprints on the waveform of the EMRIs, which provide new opportunities in probing the stellar distributions and constraining the accretion physics at galactic centers.
VIDEO:

Gravity Seminar Monday, April 5, 2021 1:00 PM Online, Room via Zoom Join Zoom Meeting:https://virginia.zoom.us/j/98166651049Meeting ID: 981 6665 1049

"Adventures in Gravitationalwave Astronomy: testing for hair, memory, and eccentricity"Paul Lasky , Monash University [Host: Alexander Saffer]
ABSTRACT:
Since the first gravitationalwave detection of a binary black hole merger in 2015, the LIGO and Virgo detectors have observed gravitational waves from more than 50 merging systems. That number is expected to increase significantly over the coming years as these experiments become even more sensitive. The increased number of detections, and the improved sensitivity of these instruments, allows us to probe the ultrastrong regime of gravity, as well as the formation history of these systems. I will discuss ongoing efforts to test general relativity in the ultra strongfield regime, including tests of the nohair theorem and searches for gravitationalwave memory  a permanent deformation of spacetime following the passage of a gravitational wave. I will also discuss efforts to detect orbital eccentricity in these systems, which has led to potentially the first observation of a secondgeneration black hole merger. 
Gravity Seminar Monday, March 22, 2021 6:00 PM Online, Room via Zoom Join Zoom Meeting:https://virginia.zoom.us/j/97049511556Meeting ID: 970 4951 1556

"Recent developments in the postMinkowskian approach to the spinning black hole binary problem"Justin Vines , Max Planck Institute for Gravitational Physics (Albert Einstein Institute) [Host: Alexander Grant]
ABSTRACT:
The detection and analysis of gravitational wave signals from coalescing binary systems crucially relies on analytic perturbative approaches to the twobody problem in general relativity (as well as on numerical approaches). While the postNewtonian (weakfield and slowmotion) approximation is most directly relevant to observations by LIGO et al., recent developments have revived interest in the more inclusive postMinkowskian (weakfield but arbitraryspeed) approximation  particularly in relation to highly advanced techniques developed by particle physicists for computing relativistic quantum scattering amplitudes and associated classical observables. This interplay between highenergy quantum physics and gravitationalwave science has led to several new results and useful insights, particularly regarding relationships between complimentary approximation schemes; this importantly also includes the "selfforce" or "posttestbody" approach, treating small mass ratios but arbitrary field strengths and speeds. We will review some of these developments, focusing on the postMinkowskian treatment of the spinning black hole binary problem. VIDEO:

Gravity Seminar Monday, March 8, 2021 1:00 PM Online, Room Zoom Join Zoom Meeting:https://virginia.zoom.us/j/98166651049Meeting ID: 981 6665 1049

"Testing the Schwarzschild/Kerr black hole hypothesis with gravitational and electromagnetic waves"Alejandro CardenasAvendano , University of Illinois UrbanaChampaign [Host: Alexander Saffer]
ABSTRACT:
Over the past years, electromagnetic and gravitational observations have been used to understand the nature of black holes and the material around them. Our ability to learn about the underlying physics, however, depends heavily on our understanding of the gravity theory that describes the geometry around these compact objects, and for the electromagnetic observations, also on the complex astrophysics that produces the observed radiation. In this talk, I will discuss our current ability to constrain and detect deviations from general relativity using (i) the electromagnetic radiation emitted by an accretion disk around a black hole, and (ii) the gravitational waves produced when comparablemass black holes collide, and when a small compact object falls into a supermassive one in an extreme massratio inspiral. I will also compare the constraining capabilities of these two types of observations to show how current gravitational wave observations have already placed constraints on possible modifications to general relativity, that are more stringent than what can be achieved with current and nearfuture electromagnetic observations. VIDEO:

Gravity Seminar Monday, February 22, 2021 1:00 PM Online, Room Zoom Join Zoom Meeting:https://virginia.zoom.us/j/98692700509Meeting ID: 986 9270 0509

"The classical evolution of binary black hole systems in scalartensor theories"Justin Ripley , University of Cambridge [Host: Alexander Saffer]
ABSTRACT:
In this talk I will discuss recent work on numerically solving for the binary black hole dynamics of black holes in Einstein scalar GaussBonnet (ESGB) gravity. This modified gravity theory can be motivated by effective field theory reasoning, and admits scalarized black hole solutions. These two facts make it a promising theory to constrain using binary black hole, gravitational wave observations. I will discuss how recent advances in mathematical relativityin particular, the development of the "modified harmonic formulation"have opened up the possibility of constructing fully nonlinear solutions to the equations of motion of ESGB gravity (in addition to a class of scalartensor modified theories known as "Horndeski" theories). I will discuss numerical simulations of single and binary black hole systems in these theories, and the gravitational and scalar radiation they emit. 
Gravity Seminar Monday, February 8, 2021 1:00 PM Online, Room Zoom Join Zoom Meeting:https://virginia.zoom.us/j/99269571512Meeting ID: 992 6957 1512

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