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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.

168,695 papers · 148 categories

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20416181 · Jun 202019922001200920172026
48 results for ADM energy

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 ↗

New relation found between ADM mass and generalized Komar energy for dynamical spacetimes.

problem Finding equality between ADM mass and Komar energy in dynamical spacetimes.
method Constructing a generalized Komar energy from the normal evolution vector and proving equality under specific conditions.
result Equality between ADM mass and generalized Komar energy for dynamical asymptotically-flat spacetimes.

We consider an asymptotically flat Lorentzian manifold of dimension (1,3). An inequality is derived which bounds the Riemannian curvature tensor in terms of the ADM energy in the general case with second fundamental form. The inequality quantifies in which sense the Lorentzian manifold becomes flat in the limit when th…

2003-06-10abs ↗pdf ↗

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.

Constructs initial data for multiple black holes with specified ADM parameters.

problem Forming multiple black holes with specific ADM parameters.
method Smooth, asymptotically flat vacuum initial data with prescribed ADM energy, momentum, and angular momentum.
result Maximal development of data results in spacetimes containing multiple black holes.

We modify previous quasi-local mass definition. The new definition provides expressions of the quasi-local energy, the quasi-local linear momentum and the quasi-local mass. And they are equal to the ADM expressions at spatial infinity. Moreover, the new quasi-local energy has the positivity property.

2009-05-17abs ↗pdf ↗

Proves Green function rigidity for specific operators and obtains new ADM mass formula.

problem Proving Green function rigidity for specific operators and obtaining new ADM mass formula.
method Positive mass theorem and positive energy theorem for Paneitz operator.
result Obtained new formula for the ADM mass of asymptotically flat hypersurfaces.

Paper glues characteristic data to Kerr spacetime, proving spacelike gluing.

problem Solving characteristic gluing problem for Einstein vacuum equations.
method Detailed characteristic gluing of strongly asymptotically flat data to Kerr spacetime.
result Alternative proof of spacelike gluing construction for strongly asymptotically flat spacelike initial data.

We establish a Penrose-Like Inequality for general (not necessarily time symmetric) initial data sets of the Einstein equations which satisfy the dominant energy condition. More precisely, it is shown that the ADM energy is bounded below by an expression which is proportional to the square root of the area of the outer…

2009-10-27abs ↗pdf ↗

The paper extends spin geometry to weighted manifolds and defines a new mass for Ricci flow.

problem Generalizing spin geometry to weighted manifolds and defining a new mass.
method Investigates spectral properties of the weighted Dirac operator and defines a new mass.
result Defines a new mass for weighted asymptotically Euclidean manifolds and shows its monotonicity under Ricci flow.

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 ↗

A universal geometric inequality for bodies relating energy, size, angular momentum, and charge is naturally implied by Bekenstein's entropy bounds. We establish versions of this inequality for axisymmetric bodies satisfying appropriate energy conditions, thus lending credence to the most general form of Bekenstein's b…

2018-02-13abs ↗pdf ↗

Proves a higher-order positive energy theorem for stationary solutions in fourth-order gravity.

problem Proving a positive energy theorem for fourth-order gravitational theories.
method Analyzes geometric analysis intersections and links to QQ-curvature.
result Establishes a positive energy theorem for stationary solutions in fourth-order gravity, similar to the classical ADM theorem.

We study the limit of quasilocal mass defined in [4] and [5] for a family of spacelike 2-surfaces in spacetime. In particular, we show the limit coincides with the ADM mass at spatial infinity. The limit for coordinate spheres of a boosted slice of the Schwarzchild solution is computed explicitly and shown to give the …

2009-06-01abs ↗pdf ↗

Given a spacelike 2-surface ΣΣ in a spacetime NN and a constant future timelike unit vector T0T_0 in R3,1\R^{3,1}, we derive upper and lower estimates of Wang-Yau quasilocal energy E(Σ,X,T0)E(Σ, X, T_0) for a given isometric embedding XX of ΣΣ into a flat 3-slice in R3,1\R^{3,1}. The quantity E(Σ,X,T0) E(Σ, X, T_0) itself depends …

2009-09-04abs ↗pdf ↗

We establish a Penrose-like inequality for general (not necessarily time-symmetric) initial data sets of the Einstein-Maxwell equations, which satisfy the dominant energy condition. More precisely, it is shown that the ADM energy is bounded below by an expression which is proportional to the sum of the square root of t…

2013-08-16abs ↗pdf ↗

Paper solves Einstein vacuum equations gluing problem with applications.

problem Solving characteristic gluing problem for Einstein vacuum equations.
method Codimension-10 gluing construction, relating charges to ADM energy, and localized version.
result Asymptotically flat data can be glued to Kerr spacetime with 10 charges.

We present a proof of the Riemannian Penrose inequality with charge rm+m2q2r\leq m + \sqrt{m^2-q^2}, where A=4πr2A=4πr^2 is the area of the outermost apparent horizon with possibly multiple connected components, mm is the total ADM mass, and qq the total charge of a strongly asymptotically flat initial data set for the Einste…

2013-08-17abs ↗pdf ↗

The rigidity statement of the positive mass theorem asserts that an asymptotically flat initial data set for the Einstein equations with zero ADM mass, and satisfying the dominant energy condition, must arise from an embedding into Minkowski space. In this paper we address the question of what happens when the mass is …

2019-06-26abs ↗pdf ↗

Constructs foliations of critical surfaces for Hawking energy in asymptotically flat initial data sets.

problem Positivity and rigidity of Hawking quasi-local energy in asymptotically flat spacetimes.
method Lyapunov-Schmidt reduction within a Willmore-foliation framework.
result Existence and uniqueness of foliations by Hawking surfaces, positivity and large-sphere limit of Hawking energy.

In this paper, we investigate the behavior of ADM mass and Einstein-Hilbert functional under the Yamabe flow. Through studying the Yamabe flow by weighted spaces, we show that ADM mass and Einstein-Hilbert functional are well-defined and monotone non-increasing under the Yamabe flow on nn-dimensional, n3n\geq 3, asymp…

2011-09-12abs ↗pdf ↗

Study shows a mass quantity for C0C^0 metrics that agrees with ADM mass.

problem Understanding ADM mass for C0C^0 metrics and its behavior under Ricci-DeTurck flow.
method Developed a C0C^0 mass quantity and analyzed its behavior under Ricci-DeTurck flow.
result The C0C^0 mass at infinity is independent of coordinate charts and has controlled distortion under Ricci-DeTurck flow.

We give some lower estimates of the ADM mass of an asymptotically flat (AF) Riemannian manifold without assuming that the scalar curvature of the manifold is nonnegative. Some sufficient conditions for an AF manifold to have nonnegative ADM mass are obtained. We also give some lower estimates of the Brown-York mass of …

2004-06-28abs ↗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 ↗

Predicts financial asset dependencies using spatiotemporal patterns.

problem Complex dependency structures in financial assets for risk mitigation.
method Proposes Asset Dependency Matrix (ADM) and Asset Dependency Neural Network (ADNN) with ConvLSTM for spatiotemporal asset dependency prediction.
result ADNN outperforms baselines in predicting asset dependencies and their applications.

We bound the locations of outermost minimal surfaces in geometrostatic manifolds whose ADM mass is small relative to the separation between the black holes and prove the Intrinsic Flat Stability of the Positive Mass Theorem in this setting.

2017-07-10abs ↗pdf ↗

For asymptotically flat initial data of Einstein's equations satisfying an energy condition, we show that the Penrose inequality holds between the ADM mass and the area of an outermost apparent horizon, if the data are restricted suitably. We prove this by generalizing Geroch's proof of monotonicity of the Hawking mass…

2002-01-08abs ↗pdf ↗

It is conjectured that the full (spacetime) Bartnik mass of a surface ΣΣ is realised as the ADM mass of some stationary asymptotically flat manifold with boundary data prescribed by ΣΣ. Assuming this holds true for a 1-parameter family of surfaces ΣtΣ_t evolving in an initial data set {with the dominant energy condit…

2019-02-06abs ↗pdf ↗

We prove a version the Penrose inequality for black hole space-times which are perturbations of the Schwarzschild exterior in a slab around a null hypersurface N0\underline{\mathcal{N}}_0. N0\underline{\mathcal{N}}_0 terminates at past null infinity I\mathcal{I}^- and S0:=N0\mathcal{S}_0:=\partial\underline{\mathcal{N}}_0

2015-06-21abs ↗pdf ↗

We provide integral formulae for the ADM mass of asymptotically flat hypersurfaces in Riemannian manifolds with a certain warped product structure in a neighborhood of infinity, thus extending Lam's recent results on Euclidean graphs to this broader context. As applications we exhibit, in any dimension, new classes of …

2011-08-27abs ↗pdf ↗

Online optimization has emerged as powerful tool in large scale optimization. In this paper, we introduce efficient online algorithms based on the alternating directions method (ADM). We introduce a new proof technique for ADM in the batch setting, which yields the O(1/T) convergence rate of ADM and forms the basis of …

2012-06-27abs ↗pdf ↗