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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.

168,657 papers · 148 categories

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77154230307 · Jun 202019922001200920172026
48 results for big bang convergence

The paper proves conditions for curvature blow-up in quiescent big bang singularities.

problem Understanding the nature of big bang singularities in cosmological models.
method Analyzing initial data sets with positive mean curvature and proving curvature blow-up conditions.
result Proves the formation of quiescent big bang singularities under certain conditions.

Localized big bang singularities found without background solutions.

problem Proving localized big bang formation without proximity to background solutions.
method Introducing a new foliation by spacelike hypersurfaces and a time function to synchronize and stabilize the singularity.
result Maximally globally hyperbolic developments have local quiescent big bang singularities with curvature blow-up.

Einstein's equation, in its standard form, breaks down at the Big Bang singularity. A new version, equivalent to Einstein's whenever the latter is defined, but applicable in wider situations, is proposed. The new equation remains smooth at the Big Bang singularity of the Friedmann-Lemaitre-Robertson-Walker model. It is…

2012-03-08abs ↗pdf ↗

Develops geometric framework for analyzing big bang singularities without symmetry assumptions.

problem Analyzing big bang singularities without symmetry constraints.
method Geometric framework combined with Einstein's equations.
result Partial improvements of assumptions on expansion normalised Weingarten map and convergence of K\mathcal{K}.

The paper proves that certain FLRW spacetimes cannot be extended past the big bang.

problem The singularity structure of FLRW spacetimes without particle horizons at the C0C^0-level.
method Analyzing the singularity structure of FLRW spacetimes with constant spatial curvature.
result A geometric obstruction prevents continuous spacetime extensions for a wide range of scale factors in the case of K=1K=-1.

New obstruction prevents certain spacetimes with both big bang and big crunch.

problem Preventing spacetimes with both big bang and big crunch.
method Analyzing initial data sets subject to dominant energy condition and enlargeability obstruction.
result Pairs of spacetimes with both big bang and big crunch are not connected in certain cases.

We consider branes $N=I\times\so$, where $\so$ is an nn\ndash dimensional space form, not necessarily compact, in a Schwarzschild-AdS_{(n+2)} bulk $\mc N$. The branes have a big crunch singularity. If a brane is an ARW space, then, under certain conditions, there exists a smooth natural transition flow through the sin…

2004-04-13abs ↗pdf ↗

Proves initial data on big bang singularities for Einstein-nonlinear scalar field equations lead to unique solutions.

problem Initial data on big bang singularities for Einstein equations.
method Geometric formulation of initial data, proving existence and uniqueness of solutions.
result Initial data on the singularity for the Einstein-nonlinear scalar field equations in 4 spacetime dimensions lead to a unique development of the data.

Study proves stability of big bang singularity in complex system.

problem Stability of Kasner solutions in Einstein-Maxwell-scalar field-Vlasov system.
method Detailed mathematical structures and new delicate arguments.
result Nonlinear stability with Kasner exponents in full strong sub-critical regime.

The Weyl curvature hypothesis of Penrose attempts to explain the high homogeneity and isotropy, and the very low entropy of the early universe, by conjecturing the vanishing of the Weyl tensor at the Big-Bang singularity. In previous papers it has been proposed an equivalent form of Einstein's equation, which extends i…

2012-03-15abs ↗pdf ↗

We consider branes NN in a Schwarzschild-AdS(n+2)\text{AdS}_{(n+2)} bulk, where the stress energy tensor is dominated by the energy density of a scalar fields map $\f:N\ra \mc S$ with potential VV, where $\mc S$ is a semi-Riemannian moduli space. By transforming the field equation appropriately, we get an equivalent field …

2004-09-13abs ↗pdf ↗

We consider the so-called inverse FF-curvature flow (IFCF) x˙=F1ν\dot x = -F^{-1}ν in ARW spaces, i.e. in Lorentzian manifolds with a special future singularity. Here, FF denotes a curvature function of class (K)(K^*), which is homogenous of degree one, e.g. the nn-th root of the Gaussian curvature, and νν the past dire…

2011-06-23abs ↗pdf ↗

New null distance bounds confirm Big Bang singularity in cosmological models.

problem Understanding the geometry of spacetime near Big Bang singularities.
method Developed a new null distance metric for temporal functions and applied it to cosmological models.
result Null distance is bounded by a constant multiple of Riemannian distance on level sets with constant gradient norm.

Milne-like spacetimes are a class of FLRW models which admit C0C^0 spacetime extensions through the big bang. The boundary of a Milne-like spacetime can be identified with a null cone in the extension. We find that the comoving observers all emanate from a single point in the extension. This suggests that something phy…

2017-06-05abs ↗pdf ↗

Einstein's equation is rewritten in an equivalent form, which remains valid at the singularities in some major cases. These cases include the Schwarzschild singularity, the Friedmann-Lemaître-Robertson-Walker Big Bang singularity, isotropic singularities, and a class of warped product singularities. This equation is co…

2012-03-09abs ↗pdf ↗

New proof of past stability for Kasner solutions in (3+1)(3+1)-dimensional Einstein vacuum spacetime.

problem Stability of Kasner singularities in (3+1)(3+1)-dimensional Einstein vacuum spacetime.
method Developed (2+1)(2+1) orthonormal-frame decomposition and symmetrization argument, applying Fuchsian techniques.
result Perturbed solutions are asymptotically pointwise Kasner, geodesically incomplete, and crushing at the Big Bang singularity.

A large collection of financial contracts offering guaranteed minimum benefits are often posed as control problems, in which at any point in the solution domain, a control is able to take any one of an uncountable number of values from the admissible set. Often, such contracts specify that the holder exert control at a…

2015-02-19abs ↗pdf ↗

This paper is a continuation of the work by the same authors on the Cartan group equipped with the sub-Finsler \ell_\infty norm. We start by giving a detailed presentation of the structure of bang-bang extremal trajectories. Then we prove upper bounds on the number of switchings on bang-bang minimizers. We prove that…

2018-10-12abs ↗pdf ↗

Under the optimal withdrawal strategy of a policyholder, the pricing of variable annuities with Guaranteed Minimum Withdrawal Benefit (GMWB) is an optimal stochastic control problem. The surrender feature available in marketed products allows termination of the contract before maturity, making it also an optimal stoppi…

2015-07-31abs ↗pdf ↗

Consider a smooth manifold MM with a smooth cometric gg^{\ast} which changes the bilineal type by transverse way, on a hypersurface DD^{\infty}. Suppose that the radical annihilator hyperplane is tangent to DD^{\infty}. We examine the geometry of the (gg^{\ast}-dual) covariant metric gg on MM- DD^{\infty}, prov…

2006-06-02abs ↗pdf ↗

The two-dimensional renormalization group acting as the Ricci flow ΛΛgμν=RμνΛ\frac{\partial}{\partialΛ} g_{μν} = R_{μν} produces a specific 1+3 dimensional space-time metric which describes an expanding universe that starts with a big bang at1/3a \sim t^{\scriptscriptstyle 1/\sqrt3} then decelerates until z=0.2z=0.2 then accelerate…

2019-09-03abs ↗pdf ↗

New findings show cosmological constant as initial condition for non-isotropic spacetimes.

problem Cosmological constant as initial condition in non-isotropic spacetimes.
method Generalized previous results to non-isotropic spacetimes.
result Quasi de Sitter expansion for early universe, potential for inflationary scenarios.

In General Relativity the metric can be recovered from the structure of the lightcones and a measure giving the volume element. Since the causal structure seems to be simpler than the Lorentzian manifold structure, this suggests that it is more fundamental. But there are cases when seemingly healthy causal structure an…

2015-04-27abs ↗pdf ↗

Gravitational wave memory increases faster than Brownian motion in early universe and astrophysical sources.

problem Detecting gravitational wave memory from early universe and astrophysical sources.
method Investigated gravitational wave sources in early universe and astrophysical settings, showing memory increases faster than Brownian motion.
result Gravitational wave memory increases following a power law, faster than the t\sqrt{t} scaling law of Brownian motion.

In this article the degenerate warped products of singular semi-Riemannian manifolds are studied. They were used recently by the author to handle singularities occurring in General Relativity, in black holes and at the big-bang. One main result presented here is that a degenerate warped product of semi-regular semi-Rie…

2011-05-17abs ↗pdf ↗

Let (Bt)0tT(B_t)_{0\leq t\leq T} be either a Bernoulli random walk or a Brownian motion with drift, and let Mt:=max{Bs:0st}M_t:=\max\{B_s: 0\leq s\leq t\}, 0tT0\leq t\leq T. This paper solves the general optimal prediction problem \sup_{0\leqτ\leq T}\sE[f(M_T-B_τ)], where the supremum is over all stopping times ττ adapted to the natural…

2009-10-03abs ↗pdf ↗

This work presents the foundations of Singular Semi-Riemannian Geometry and Singular General Relativity, based on the author's research. An extension of differential geometry and of Einstein's equation to singularities is reported. Singularities of the form studied here allow a smooth extension of the Einstein field eq…

2013-01-10abs ↗pdf ↗

In this paper we study a sub-Finsler geometric problem on the free-nilpotent group of rank 2 and step 3. Such a group is also called Cartan group and has a natural structure of Carnot group, which we metrize considering the \ell_\infty norm on its first layer. We adopt the point of view of time-optimal control theory…

2018-10-09abs ↗pdf ↗

The existence, established over the past number of years and supporting earlier work of Ori [14], of physically relevant black hole spacetimes that admit C0C^0 metric extensions beyond the future Cauchy horizon, while being C2C^2-inextendible, has focused attention on fundamental issues concerning the strong cosmic cen…

2016-10-10abs ↗pdf ↗

Given a time function ττ on a spacetime MM, we define a `null distance function', d^τ\hat{d}_τ, built from and closely related to the causal structure of MM. In basic models with timelike τ\nabla τ, we show that 1) d^τ\hat{d}_τ is a definite distance function, which induces the manifold topology, 2) the causal struct…

2015-08-03abs ↗pdf ↗

New method improves likelihood-free parameter estimation in complex models.

problem Estimating parameters in simulation-based models with unknown likelihood.
method Nested multi-time-scale stochastic approximation (NMTS) method.
result Eliminates bias and accelerates convergence in likelihood-free inference.

MiMuon optimizer improves generalization for large models by reducing generalization error.

problem Improving generalization of Muon optimizer for large models.
method Enhanced Muon optimizer using orthogonalization of gradient, proving lower generalization error.
result MiMuon optimizer has a lower generalization error of O(1N)O\big(\frac{1}{N}\big) compared to Muon's O(1NκT)O\big(\frac{1}{Nκ^{T}}\big).

We propose the online machine learning for big data analysis with heterogeneity. We performed an experiment to compare the accuracy of each iteration between batch one and online one. It is possible to converge quickly with the same accuracy as the batch one.

2019-06-15abs ↗pdf ↗

Study improves covariance estimation for SGD under Markovian data, matching best rates.

problem Improving covariance estimation for SGD in Markovian data settings.
method Online overlapping batch-means covariance estimator for SGD under Markovian sampling.
result Established convergence rates for covariance estimation under Markovian sampling.

We consider spacetimes consisting of a manifold with Lorentzian metric and a weight function or scalar field. These spacetimes admit a Bakry-Émery-Ricci tensor which is a natural generalization of the Ricci tensor. We impose an energy condition on the Bakry-Émery-Ricci tensor and obtain singularity theorems of a cosmol…

2013-12-12abs ↗pdf ↗