Marcus Khuri

ORCID: 0000-0002-5718-2015
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Research Areas
  • Black Holes and Theoretical Physics
  • Cosmology and Gravitation Theories
  • Geometric Analysis and Curvature Flows
  • Advanced Differential Geometry Research
  • Geometry and complex manifolds
  • Nonlinear Partial Differential Equations
  • Relativity and Gravitational Theory
  • Advanced Mathematical Modeling in Engineering
  • Mathematics and Applications
  • Noncommutative and Quantum Gravity Theories
  • Numerical methods in inverse problems
  • Differential Equations and Boundary Problems
  • Advanced Mathematical Physics Problems
  • Point processes and geometric inequalities
  • Pulsars and Gravitational Waves Research
  • Astrophysical Phenomena and Observations
  • Geometric and Algebraic Topology
  • Advanced Mathematical Theories and Applications
  • advanced mathematical theories
  • Particle physics theoretical and experimental studies
  • Nonlinear Waves and Solitons
  • Advanced Mathematical Theories
  • Algebraic and Geometric Analysis
  • Algebraic Geometry and Number Theory
  • Polynomial and algebraic computation

Stony Brook University
2016-2025

Harvard University
2021

Memorial University of Newfoundland
2021

Clark University
2021

Mathematical Sciences Research Institute
2021

Gakushuin University
2017

Ariel University
2017

Freie Universität Berlin
2016

Max Planck Institute for Gravitational Physics
2016

State University of New York
2014

In this paper, we prove compactness for the full set of solutions to Yamabe Problem if $n\leq 24$. After proving sharp pointwise estimates at a blowup point, Weyl Vanishing The- orem in those dimensions, and reduce question showing positivity quadratic form. We also show that form has negative eigenvalues 25$.

10.4310/jdg/1228400630 article EN Journal of Differential Geometry 2009-01-01

We give a lower bound for the Lorentz length of ADM energy-momentum vector (ADM mass) 3‑dimensional asymptotically flat initial data sets Einstein equations. The is given in terms linear growth 'spacetime harmonic functions' addition to density matter fields, and valid regardless whether dominant energy condition holds or possess boundary. A corollary this result new proof spacetime positive mass theorem complete those with weakly trapped surface boundary, includes rigidity statement which...

10.4310/jdg/1669998184 article EN Journal of Differential Geometry 2022-10-01

In this paper, we show how to reduce the Penrose conjecture known Riemannian inequality case whenever certain geometrically motivated systems of equations can be solved.Whether or not these special have general existence theories is therefore an important open problem.The key tool in our method derivation a new identity which call generalized Schoen-Yau identity, independent interest.Using Jang equation, use propose canonical embeddings Cauchy data into corresponding static spacetimes.In...

10.4310/ajm.2011.v15.n4.a5 article EN Asian Journal of Mathematics 2011-01-01

In [4] and [5], Bray Khuri outlined an approach to prove the Penrose inequality for general initial data sets of Einstein equations.In this paper we extend so that it may be applied a charged version inequality.Moreover, assuming is time symmetric, rigidity statement in case equality inequality, result which seems absent from literature.A new quasi-local mass, tailored also introduced, used proof.

10.1088/0264-9381/29/24/245019 article EN Classical and Quantum Gravity 2012-12-03

We present a proof of the Riemannian Penrose inequality with charge in context asymptotically flat initial data sets for Einstein–Maxwell equations, having possibly multiple black holes no charged matter outside horizon, and satisfying relevant dominant energy condition. The is based on generalization Hubert Bray's conformal flow metrics adapted to this setting.

10.4310/jdg/1500084023 article EN Journal of Differential Geometry 2017-06-01

This is the second in a series of two papers to establish conjectured mass-angular momentum inequality for multiple black holes, modulo extreme hole 'no hair theorem'. More precisely it shown that either there counterexample uniqueness, form regular axisymmetric stationary vacuum spacetime with an asymptotically flat end and degenerate horizons which 'ADM minimizing', or following statement holds. Complete, simply connected, maximal initial data sets Einstein equations ends are cylindrical,...

10.48550/arxiv.2501.15093 preprint EN arXiv (Cornell University) 2025-01-25

A classic result of Shi and Tam states that a 2-sphere positive Gauss mean curvature bounding compact 3-manifold with nonnegative scalar must have total not greater than the isometric embedding into Euclidean 3-space, equality only for domains in this reference manifold. We generalize to 2-tori <inline-formula content-type="math/mathml"> <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" alttext="negative 1"> <mml:semantics> <mml:mrow> <mml:mo>−</mml:mo> <mml:mn>1</mml:mn> </mml:mrow>...

10.1090/proc/17223 article EN Proceedings of the American Mathematical Society 2025-03-05

We introduce a generalized version of the Jang equation, designedfor general case Penrose Inequality in setting ofan asymptotically flat space-like hypersurface spacetimesatisfying dominant energy condition. The appropriateexistence and regularity results are established specialcase spherically symmetric Cauchy data, applied to givea new proof for these data sets.When appropriately coupled with an inverse mean curvature flow,analogous existence associatedsystem equations nonspherical would...

10.3934/dcds.2010.27.741 article EN Discrete and Continuous Dynamical Systems 2010-01-01

The most general formulation of Penrose's inequality yields a lower bound for ADM mass in terms the area, charge, and angular momentum black holes. This is turn equivalent to an upper area remaining quantities. In this note, we establish single hole setting axisymmetric maximal initial data sets Einstein-Maxwell equations, when non-electromagnetic matter fields are not charged satisfy dominant energy condition. It shown that saturated if only arise from extreme Kerr-Newman spacetime. Further...

10.1103/physrevd.88.024048 article EN Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology 2013-07-26

We develop a framework for understanding the existence of asymptotically flat solutions to static vacuum Einstein equations on with geometric boundary conditions ∂M ≃ S2. A partial result is obtained, giving resolution conjecture Bartnik such extensions. The and uniqueness extensions closely related Bartnik's definition quasi-local mass.

10.1088/0264-9381/30/12/125005 article EN Classical and Quantum Gravity 2013-05-14

Abstract The generalized Jang equation was introduced in an attempt to prove the Penrose inequality setting of general initial data for Einstein equations. In this paper we give extensive study equation, proving existence, regularity, and blow-up results. particular, precise asymptotics behavior are given, it is shown that solutions not unique. Keywords: Blow-up solutionsGeneralized equationPenrose inequalityMathematics Subject Classification: 35Q7535J7083C9958J32 Acknowledgments first...

10.1080/03605302.2013.837919 article EN Communications in Partial Differential Equations 2013-09-20

In this paper, we show how a natural coupling of the Dirac equation with generalized Jang leads to proof rigidity statement in positive mass theorem charge, without maximal slicing condition, provided solution coupled system exists.

10.1063/1.4820469 article EN Journal of Mathematical Physics 2013-09-01

Abstract We study the problem of conformal deformation Riemannian structure to constant scalar curvature with zero mean on boundary. prove compactness for full set solutions when boundary is umbilic and dimension <m:math xmlns:m="http://www.w3.org/1998/Math/MathML"> <m:mrow> <m:mi>n</m:mi> <m:mo>≤</m:mo> <m:mn>24</m:mn> </m:mrow> </m:math> ${n\leq 24}$ . The Weyl Vanishing Theorem also established under these hypotheses, we provide counter-examples <m:mo>≥</m:mo> <m:mn>25</m:mn> ${n\geq 25}$...

10.1515/crelle-2014-0083 article EN Journal für die reine und angewandte Mathematik (Crelles Journal) 2014-10-28

10.1007/s00526-016-0969-8 article EN Calculus of Variations and Partial Differential Equations 2016-03-07

Abstract Generalized torical band inequalities give precise upper bounds for the width of compact manifolds with boundary in terms positive pointwise lower scalar curvature, assuming certain topological conditions. We extend several incarnations these results which curvature are replaced spectral bounds. More precisely, we prove principal eigenvalue operator $-\Delta +cR$, where $R$ denotes and $c&amp;gt;0$ is a constant. Three separate strategies employed to obtain distinct holding...

10.1093/imrn/rnad129 article EN International Mathematics Research Notices 2023-06-26

We give general sufficient conditions for the existence of trapped surfaces due to concentration matter in spherically symmetric initial data sets satisfying dominant energy condition. These results are novel that they apply and meaningful arbitrary spacelike slices, is, do not require any auxiliary assumptions such as maximality, time symmetry, or special extrinsic foliations, most importantly can easily be generalized nonspherical case once an theory a modified version Jang equation is...

10.1103/physrevd.80.124025 article EN Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D, Particles, fields, gravitation, and cosmology 2009-12-17

We study the old problem of isometrically embedding a twodimensional Riemannian manifold into Euclidean three-space.It is shown that if Gaussian curvature vanishes to finite order and its zero set consists two Lipschitz curves intersecting transversely at point, then local sufficiently smooth isometric embeddings exist.

10.4310/cag.2010.v18.n4.a2 article EN Communications in Analysis and Geometry 2010-01-01

10.1007/s10714-013-1588-8 article EN General Relativity and Gravitation 2013-08-29

We study the problem of asymptotically flat bi-axially symmetric stationary solutions vacuum Einstein equations in 5-dimensional spacetime. In this setting, cross section any connected component event horizon is a prime 3-manifold positive Yamabe type, namely 3-sphere S3, ring S1×S2, or lens space L(p, q). The reduce to an axially harmonic map with prescribed singularities from R3 into SL(3,R)/SO(3). paper, we solve for all possible topologies, and particular first candidates smooth...

10.1080/03605302.2018.1517791 article EN Communications in Partial Differential Equations 2018-08-03
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