During the Spring 2019 Semester, a weekly seminar will be held on General Relativity. The seminar will take place at on Thursdays at 3:00pm in Science Center 411.
The schedule will be updated below.
Date | Speaker | Title/abstract |
9/7/2018 | Christos Mantoulidis (MIT) | Title: Capacity and quasi-local mass
Abstract. This talk is based on work with P. Miao and L.-F. Tam. We derive new inequalities between the boundary capacity of an asymptotically flat 3-manifold with nonnegative scalar curvature and boundary quantities that relate to quasi-local mass; one relates to Brown-York mass and the other is new. Among other things, our work yields new variational characterizations of Riemannian Schwarzschild manifolds and new comparison results for surfaces in them. |
9/12/2018 | Aghil Alaee (CMSA) | Title: Mass-angular momentum inequality for black holes
Abstract: In this talk, I will review the results of mass-angular momentum inequality for four-dimensional axisymmetric black holes. Then I will establish versions of this inequality for five-dimensional black holes and in particular black ring, which is the most intriguing asymptotically flat solution of vacuum Einstein equations. Moreover, I will show these inequalities are sharp if and only if the initial data sets are isometric to the canonical slices of known extreme stationary solutions. These results are joint work with Marcus Khuri and Hari Kunduri. |
9/19/2018 | Pei-Ken Hung (MIT) | Title: The linear stability of the Schwarzschild spacetime in the harmonic gauge: odd part
Abstract: We study the odd solution of the linearlized Einstein equation on the Schwarzschild background and in the harmonic gauge. With the aid of Regge-Wheeler quantities, we are able to estimate the odd part of Lichnerowicz d’Alembertian equation. In particular, we prove the solution decays at rate $\tau^{-1+\delta}$ to a linearlized Kerr solution. |
9/26/2018 | Jordan Keller (BHI) | Title: Quasi-local Angular Momentum and Center-of-Mass at Future Null Infinity
Abstract: We calculate the limits of the quasi-local angular momentum and center-of-mass defined by Chen-Wang-Yau [3] for a family of spacelike two-spheres approaching future null infinity in an asymptotically flat spacetime admitting a Bondi-Sachs expansion. Our result complements earlier work of Chen-Wang-Yau [2], where the authors calculate the quasi-local energy and linear momentum at null infinity. Finiteness of the quasi-local center-of-mass requires that the spacetime be in the so-called center-of-mass frame, which amounts to a mild assumption on the mass aspect function corresponding to vanishing of the quasi-local linear momentum calculated in [2]. With this condition and the assumption that the mass aspect function is non-trivial, we obtain explicit expressions for the quasi-local angular momentum and center-of-mass at future null infinity in terms of the observables appearing in the Bondi-Sachs expansion of the spacetime metric. This is joint work with Ye-Kai Wang and Shing-Tung Yau. |
10/3/2018 | Christos Mantoulidis (MIT) | Title: The Bartnik mass of apparent horizons
Abstract: We will discuss a spectral characterization of apparent horizons in three-dimensional time-symmetric initial data sets. Then, for a dense class of nondegenerate apparent horizons, we will construct sharp asymptotically flat extensions to conclude that their Bartnik mass equals their Hawking mass. This is joint work with R. Schoen. |
10/10/2018 | Salem Al Mosleh (CMSA) | Title: Thin elastic shells and isometric embedding of surfaces in three-dimensional Euclidean space
Abstract: We will first discuss the reduction of theories describing elastic bodies in three-dimensions to effective descriptions defined on embedded surfaces. Then, we describe the isometric deformations of surfaces and the key role of played by asymptotic curves, curves with zero normal curvature, in determining the local mechanical behavior of thin shells. This was joint work with C. Santangelo. |
10/17/2018 | Sébastien Picard (Harvard) | Title: The Anomaly flow over Riemann surfaces
Abstract: The Anomaly flow is a geometric flow on Calabi-Yau threefolds which is motivated by string theory. We will study the flow on certain fibrations where it reduces to a scalar evolution equation on a Riemann surface. This is joint work with T. Fei and Z. Huang. |
10/31/2018 | Alex Lupsasca (Harvard) | Title: Polarization Whorls from M87 at the Event Horizon Telescope
Abstract: The Event Horizon Telescope (EHT) is expected to soon produce polarimetric images of the supermassive black hole at the center of the neighboring galaxy M87. This black hole is believed to be very rapidly spinning, within 2% of extremality. General relativity predicts that such a high-spin black hole has an emergent conformal symmetry near its event horizon. In this talk, I will briefly review this symmetry and use it to derive an analytic prediction for the polarized near-horizon emissions to be seen at the EHT. The resulting pattern is very distinctive and consists of whorls aligned with the spin. |
11/7/2018 | Jordan Keller
(BHI) |
Title: Linear Stability of Higher Dimensional Schwarzschild Black Holes
Abstract: The Schwarzschild-Tangherlini black holes are higher-dimensional generalizations of the Schwarzschild spacetimes, comprising a static, spherically symmetric family of black hole solutions to higher-dimensional vacuum gravity. The physical relevance of such solutions is intimately related to their stability under gravitational perturbations. This talk will address results on the linear stability of the Schwarzschild-Tangherlini black holes, part of ongoing joint work with Pei-Ken Hung and Mu-Tao Wang. |
11/14/2018 | Niky Kamran
(McGill) |
Title: Lorentzian Einstein metrics with prescribed conformal infinity
Abstract: We prove a local well-posedness theorem for the $(n+1)$-dimensional Einstein equations in Lorentzian signature, with initial data whose asymptotic geometry at infinity is similar to that anti-de Sitter (AdS) space and compatible boundary data prescribed at the time-like conformal boundary of space-time. This extends the fundamental result of Friedrich on the existence of anti-de Sitter space-times in 3+1 dimensions to arbitrary space-time dimensions, by a different approach that allows for generic smoothness and polyhomogeneity assumptions on the initial data. This is joint work with Alberto Enciso (ICMAT, Madrid). |
12/05/2018
*room G02* |
Pengzi Miao (University of Miami) | Title: Localization of the Penrose inequality and variation of quasi-local mass
Abstract: In the study of manifolds with nonnegative scalar curvature, a fundamental result is the Riemannian Positive mass theorem. If the manifold has horizon boundary, one has the Riemannian Penrose inequality. Given a compact region with boundary in these manifolds, one wants to understand how much mass or energy is localized in such a region. This question is usually referred to as the quasi-local mass problem. In this talk, we discuss an inequality on a compact manifold with nonnegative scalar curvature, which can be thought as a body surrounding horizons. Our discussion of the rigidity case of this inequality reveals an intriguing relation between two of the most important notions of quasi-local mass, the Bartnik mass and the Wang-Yau mass. The talk is based on joint work with Siyuan Lu. |
1/31/2019
SC 232 3-4pm |
Shahar Hadar (Harvard University) | Title: Late-time behavior of near-extremal black holes from symmetry
Abstract: Linear perturbations of extremal black holes exhibit the Aretakis instability, in which higher derivatives of the fields grow polynomially with time along the event horizon. Near-extremal black holes display similar behavior for some time, and eventually decay exponentially through quasinormal modes. In the talk I will show that the above behaviors are dictated by the conformal symmetry of the near-horizon region of such black holes. I will then discuss the significance of backreaction in the problem, and show how it can be simply accounted for within the near-horizon picture. |
2/7/2019
SC 411 3-4pm |
Pei-Ken Hung (MIT) | Title: The linear stability of the Schwarzschild spacetime in the harmonic gauge: even part
Abstract: We study the even solution of the linearlized Einstein equation on the Schwarzschild background and in the harmonic gauge. With the aid of the Zerilli equation, we estimate the even part of Lichnerowicz d’Alembertian equation. In particular, we show that up to a one dimensional stationary mode, the solution decays to a linearlized Kerr solution. This is ongoing joint work with S. Brendle. |
2/14/2019
SC 411 3-4pm |
Charles Marteau (Ecole Polytechnique) | Title: Null hypersurfaces and ultra-relativistic physics in gravity
Abstract: I will explain how the induced geometry on a null hypersurface gives rise to a particular type of structure called Carrollian geometry. The latter emerges when taking the ultra-relativistic limit of the usual pseudo-Riemannian metric. This property has strong consequences on the gravitational dynamics satisfied by the extrinsic geometry of the null hypersurface and on its symmetry group. We will see how the first one can be interpreted as ultra-relativistic conservation laws while the second corresponds to the isometries of the induced Carrollian geometry. These are very general statements for any null hypersurface but I will focus all along on a physically interesting case: the null infinity of an asymptotically flat spacetime. |
2/21/2019 | Hsin-Yu Chen (Black Hole Initiative) | Title: Measuring the Hubble Constant with Gravitational Waves
Abstract: The first detection of binary neutron star merger by Advanced LIGO-Virgo and the discovery of the optical counterpart allowed for the first independent measurement of Hubble constant with gravitational waves. In this talk, I will summarize latest cosmological measurements with gravitational waves, and discuss the future aspects of them. I will then talk about the potential challenges and how we improve the measurements. |
3/7/2019 | Laura Donnay (Harvard) | Title: Carrollian physics at the black-hole horizon
Abstract: In this talk, I will show that the near-horizon geometry of a black hole can be described as a Carrollian geometry emerging from an ultra-relativistic limit. The laws governing the dynamic of a black hole horizon, the null Raychaudhuri and Damour equations, are shown to be Carrollian conservation laws obtained by taking the ultra-relativistic limit of the conservation of an energy-momentum tensor. Vector fields preserving the Carrollian geometry of the horizon, dubbed Carrollian Killings, include BMS-like supertranslations and superrotations, and have non-trivial associated conserved charges. If time allows, I will discuss their relation with the infinite-dimensional horizon charges of the covariant phase space formalism. |
3/14/2019
3:30pm |
Peter Hintz (MIT) | Title: Stability of Minkowski space and polyhomogeneity of the metric
Abstract: I will explain a new proof of the non-linear stability of the Minkowski spacetime as a solution of the Einstein vacuum equation. The proof relies on an iteration scheme at each step of which one solves a linear wave-type equation globally. The analysis takes place on a compactification of R^4 to a manifold with corners whose boundary hypersurfaces correspond to spacelike, null, and timelike infinity. I will describe how the asymptotic behavior of the metric can be deduced from the structure of simple model operators at these boundaries. Joint work with András Vasy. |
3/28/2019 | TBA | TBA |
4/4/2019
CMSA G02 |
Marcus Khuri (Stony Brook) | Title: Stationary Vacuum Black Holes in Higher Dimensions
Abstract: A result of Galloway and Schoen asserts that horizon cross-sections must be of positive Yamabe invariant. In this talk we discuss results on a converse problem. That is, which manifolds of positive Yamabe invariant arise as horizon cross-sections in a stationary vacuum spacetime. |
4/11/2019 | Amir Babak Aazami (Clarks) | Title: Kähler metrics via Lorentzian geometry in dimension 4
Abstract: Given a Lorentzian -manifold with two distinguished vector fields satisfying properties determined by their shear, twist and various Lie bracket relations, a family of Kähler metrics is constructed on . Under certain conditions and share various properties, such as a Killing vector field or a vector field with geodesic flow. The Ricci and scalar curvatures of are computed in some cases in terms of data associated to ; in certain cases the Kähler manifold will be complete and Einstein. Many classical spacetimes fit into this construction: warped products, for instance de Sitter spacetime, as well as gravitational plane waves and metrics of Petrov type , such as Kerr and NUT metrics. This work is joint with Gideon Maschler. |
4/19/2019
CMSA G02 Friday @ 9:30am |
Lydia Bieri (University of Michigan) | Title: Logarithmic or Not Logarithmic
Abstract: In General Relativity, we describe isolated gravitating systems by asymptotically flat solutions of the Einstein equations. For various classes of initial data corresponding classes of solutions have been constructed in the nonlinear stability proofs when slightly moving away from Minkowski spacetime. Many of the null asymptotic results still hold when one replaces the small initial data by large initial data. Therefore, these solutions have become an interesting and important source to understand gravitational waves and memory as observed at null infinity. Lately, discussions have flared up whether logarithmic terms are present at highest order in crucial components of the Riemannian curvature and shear of the spacetime and whether such terms would give a tail effect for ordinary memory. There is a large literature (older and newer) on terms of this sort. In this talk, I will address some of my recent work that proves that for asymptotically flat solutions of the Einstein equations the crucial curvature and shear components do not have logarithmic terms at highest order, but logarithmic terms naturally show up at lower order. From thisit follows that there is no divergent memory caused by logarithmic terms. However, in my earlier work, considering spacetimes with very slow decay, the ordinary memory diverges (though not logarithmically but faster) and null memory is always finite. Last but not least, these logarithmic terms do show up at leading order of certain other curvature and geometric components for specific decay of the initial data. These mathematical results are in accordance with a physical argument that I will present as well. |
4/24/2019
10:30am CMSA G02 |
Armando Cabrera Pacheco (Universität Tübingen) | Title: Asymptotically flat extensions with charge
Abstract: Inspired by the Mantoulidis and Schoen construction, we obtain time-symmetric black hole initial data sets for the Einstein–Maxwell equations satisfying the dominant energy condition, such that their horizon boundary geometry is prescribed, and their total masses and total charges are controlled. We also formulate a notion of boundary Bartnik mass in this context and compute its value for minimal Bartnik data. This talk is based on a joint work with A. Alaee and C. Cederbaum. |
4/25/2019
10:30am CMSA G02 |
Pengyu Le (University of Michigan) | Title: Perturbations of Null Hypersurfaces and Null Penrose Inequality
Abstract: The Penrose inequality in general relativity is a conjectured inequality between the area of the horizon and the mass of a black-hole spacetime. The null Penrose inequality is the case where it concerns the area of the horizon and the Bondi mass at null infinity on a null hypersurface. An effective method to prove Penrose-type inequalities is to exploit the monotonicity of the Hawking mass along certain foliations. The constant mass aspect function foliation is such a desired foliation, but the behavior of the foliation at past null infinity is an obstacle for the proof. An idea to overcome this difficulty is to vary the null hypersurface to achieve the desired behavior of the foliation at null infinity, leading to a spacetime version of the Penrose inequality. To formalise this idea, one need to study perturbations of null hypersurfaces. I will talk about my work on the study of perturbations of null hypersurfaces and its application to the null Penrose inequality. |