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arXiv research

A locally-built, LLM-digested index of recent arXiv papers in quant finance, geometry/topology, and statistical ML — keyword search served straight from SQLite on this machine.

168,742 papers · 148 categories

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48 results for positive energy-momentum

The paper proves positive energy-momentum theorems for charged AdS initial data sets.

problem Proving positive energy-momentum theorems for charged asymptotically AdS initial data sets.
method Introducing a charged energy-momentum functional and establishing positive theorems under a dominant energy condition.
result The charged energy-momentum functional is non-negative on a natural real cone.

When a spacetime takes Bondi radiating metric, and is vacuum and asymptotically flat at spatial infinity which ensures the positive mass theorem, we prove that the standard ADM energy-momentum is the past limit of the Bondi energy-momentum. We also derive a formula relating the ADM energy-momentum of any asymptotically…

2005-11-08abs ↗pdf ↗

Study of Bondi-Sachs formalism for massless scalar field with zero cosmological constant.

problem Analyzing the Bondi-Sachs formalism for Einstein's massless scalar field equations.
method Asymptotic expansions and peeling property for Bondi-Sachs metrics and scalar fields.
result Positivity of Bondi energy-momentum under specific conditions.

New proof shows equality in spacetime mass theorem.

problem Proving the equality case of spacetime positive mass theorem.
method Uses a new approach requiring only EPE \ge |P| for near initial data sets.
result Initial data sets with null ADM energy-momentum must embed into Minkowski space.

One has not any conventional energy-momentum conservation law in Lagrangian field theory, but relations involving different stress-energy-momentum tensors associated with different connections. It is not obvious how to choose the true energy-momentum tensor. This problem is solved in the framework of the multimomentum …

1995-03-22abs ↗pdf ↗

We affirm the rigidity conjecture of the spacetime positive mass theorem in dimensions less than eight. Namely, if an asymptotically flat initial data set satisfies the dominant energy condition and has E=PE=|P|, then E=P=0E=|P|=0, where (E,P)(E, P) is the ADM energy-momentum vector. The dimensional restriction can be removed…

2017-06-12abs ↗pdf ↗

We show that the causal-future-directed character of the energy-momentum vector of nn-dimensional asymptotically hyperbolic Riemannian manifolds with spherical conformal infinity, n3n\ge 3, can be traced back to that of asymptotically Euclidean general-relativistic initial data sets satisfying the dominant energy cond…

2019-01-16abs ↗pdf ↗

On SpincSpin^c manifolds, we study the Energy-Momentum tensor associated with a spinor field. First, we give a spinorial Gauss type formula for oriented hypersurfaces of a SpincSpin^c manifold. Using the notion of generalized cylinders, we derive the variationnal formula for the Dirac operator under metric deformation and po…

2010-11-01abs ↗pdf ↗

The paper examines geometric curvatures in generalized Riemannian spaces.

problem Understanding the physical meaning of scalar curvatures in generalized Riemannian spaces.
method Developed Madsen's formulae for pressures and energy-densities, analyzed with different concepts of generalized Riemannian spaces.
result Linearities of energy-momentum tensor, pressure, energy-density, and state-parameter are examined.

Derives energy-momentum tensor from Standard Model, examines energy conditions.

problem Validating energy conditions in the context of the Standard Model.
method Geometric variational problem on globally hyperbolic manifold, deriving energy-momentum tensor.
result Validates various energy conditions in general relativity.

Generalizes energy-momentum method for non-autonomous Hamiltonian systems.

problem Stability analysis of non-autonomous Hamiltonian systems with symmetries.
method Develops a new approach to relative equilibrium points and stability conditions for non-autonomous systems.
result Conditions ensuring stability of relative equilibrium points in non-autonomous Hamiltonian systems.

This work is devoted to the study of Einstein equations with a special shape of the energy-momentum tensor. Our results continue Stepanov's classification of Riemannian manifolds according to special properties of the energy-momentum tensor to Kähler manifolds. We show that in this case the number of classes reduces.

2010-03-23abs ↗pdf ↗

The paper examines properties of WW-curvature tensor in relativistic space-times.

problem Investigating the properties and implications of the WW-curvature tensor in relativistic space-times.
method Analyzing the semi-symmetry and divergence properties of the energy-momentum tensor in relation to the WW-curvature tensor.
result Space-times with specific properties of the WW-curvature tensor are classified as Einstein or Codazzi type.

Paper bounds mass of 3D Einstein data using spacetime harmonic functions.

problem Calculating the mass of 3D asymptotically flat initial data for the Einstein equations.
method Uses spacetime harmonic functions to give a lower bound for the ADM mass.
result New proof of spacetime positive mass theorem and rigidity statement.

New method for studying tt-dependent Hamilton equations on cosymplectic manifolds.

problem Existence and stability of solutions of tt-dependent Hamilton equations.
method Develops a cosymplectic energy-momentum method for Hamilton equations with more types of symmetries.
result Provides a more general framework for studying tt-dependent Hamilton equations.

In \cite{ly, ly2}, Liu and the second author propose a definition of the quasi-local mass and prove its positivity. This is demonstrated through an inequality which in turn can be interpreted as a total mean curvature comparison theorem for isometric embeddings of a surface of positive Gaussian curvature. The Riemannia…

2006-02-15abs ↗pdf ↗

We show that it is natural to consider the energy-momentum tensor associated with a spinor field as the second fundamental form of an isommetric immersion. In particular we give a generalization of the warped product construction over a Riemannian manifold leading to this interpretation. Special sections of the spinor …

2003-02-18abs ↗pdf ↗

Mathematical framework for field theories on Finsler spacetimes.

problem Developing a consistent calculus for field theories on Finsler spacetimes.
method Constructing configuration bundles and applying coordinate-free calculus of variations.
result Averaged energy-momentum conservation law for Finsler field theories.

Novel method for solving ODEs on k-polysymplectic manifolds.

problem Solving ordinary differential equations on k-polysymplectic manifolds.
method k-polysymplectic energy-momentum method.
result Novel stability analysis techniques applied to Hamiltonian systems.

We show that there are isometrically nonequivalent Robertson-Walker metrics which have the same set of geodesics. While one of these metrics satisfies the Einstein equations of pure dust without a cosmological constant, all the other describe pure dust with additional energy momentum tensor of cosmological constant typ…

2010-03-07abs ↗pdf ↗

In Lorentzian manifolds of any dimension the concept of causal tensors is introduced. Causal tensors have positivity properties analogous to the so-called ``dominant energy condition''. Further, it is shown how to build, from ANY given tensor AA, a new tensor quadratic in AA and ``positive'', in the sense that it is …

2002-02-20abs ↗pdf ↗

As discussed in the paper, in a matter-filled spacetime, perhaps with positive cosmological constant, a stable marginally outer trapped 2-sphere must satisfy a certain area inquality. Namely, its area must be bounded above by 4π/c4π/c, where c>0c > 0 is a lower bound on a natural energy momentum term. In this note we cons…

2015-03-18abs ↗pdf ↗

On a compact surface endowed with any $\Spinc$ structure, we give a formula involving the Energy-Momentum tensor in terms of geometric quantities. A new proof of a Bär-type inequality for the eigenvalues of the Dirac operator is given. The round sphere S2\mathbb{S}^2 with its canonical $\Spinc$ structure satisfies the …

2012-04-02abs ↗pdf ↗

In a matter-filled spacetime, perhaps with positive cosmological constant, a stable marginally outer trapped 2-sphere must satisfy a certain area inequality. Namely, as discussed in the paper, its area must be bounded above by 4π/c4π/c, where c>0c > 0 is a lower bound on a natural energy-momentum term. We then consider th…

2015-05-29abs ↗pdf ↗

The paper explores symmetries and conserved charges on pre-symplectic manifolds.

problem Analyzing conserved charges on solutions of Hamiltonian field theories.
method Using pre-symplectic structures and Gotay's coisotropic embedding theorem, the paper deals with gauge theories and examples like Electrodynamics and Klein-Gordon theory.
result Emergence of the energy-momentum tensor algebra of conserved currents.

In this article, we consider the limit of quasi-local conserved quantities [31,9] at the infinity of an asymptotically hyperbolic initial data set in general relativity. These give notions of total energy-momentum, angular momentum, and center of mass. Our assumption on the asymptotics is less stringent than any previo…

2014-09-05abs ↗pdf ↗

We prove the spacetime positive mass theorem in dimensions less than eight. This theorem states that for any asymptotically flat initial data set satisfying the dominant energy condition, the ADM energy-momentum vector (E,P)(E,P) of the initial data satisfies the inequality EPE \ge |P|. Previously, this theorem was proven…

2011-10-10abs ↗pdf ↗

We study the divergence theorem on pseudo-Finsler spaces and obtain a completely Finslerian version for spaces having a vanishing mean Cartan torsion. This result helps to clarify the problem of energy-momentum conservation in Finsler gravity theories.

2015-08-25abs ↗pdf ↗

Smooth deformations of a Minkowski type metric in a four-dimensional space-time manifold are considered. Deformations of the basic spin-tensorial fields associated with this metric are calculated and their application to calculating the energy-momentum tensor of a massive spin 1/2 particle is shown.

2007-09-10abs ↗pdf ↗