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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.

168,657 papers · 148 categories

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21416282 · Jun 202619922001200920172026
48 results for big bang singularities

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 ↗

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.

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.

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 $N=I\times\so$, 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 ↗

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.

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}.

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.

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 ↗

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.

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.

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.

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 ↗

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 ↗

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 ↗

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 ↗

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 ↗

Seminar held at JINR, Dubna, May 15, 2012. In General Relativity, spacetime singularities raise a number of problems, both mathematical and physical. One can identify a class of singularities - with smooth but degenerate metric - which, under a set of conditions, allow us to define proper geometric invariants, and to w…

2012-07-23abs ↗pdf ↗

The paper examines gravitational singularities in spacetimes and proves inextendibility.

problem Investigating gravitational singularities in spacetimes.
method Analyzing local holonomy and using it to prove inextendibility.
result Proves the Cloc0,1C^{0,1}_{\mathrm{loc}}-inextendibility of certain spacetimes.

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 ↗

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 ↗

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 ↗

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 ↗

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 ↗

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 ↗

Uniform volume estimate for Kähler metrics in big cohomology classes.

problem Estimating volume for singular Kähler metrics in big cohomology classes.
method Generalized mixed energy estimate for functions in complex Sobolev space to big cohomology classes.
result Uniform non-collapsing volume estimate for local Kähler metrics.

Let XX be a compact Kähler manifold and {θ}\{θ\} be a big cohomology class. We prove several results about the singularity type of full mass currents, answering a number of open questions in the field. First, we show that the Lelong numbers and multiplier ideal sheaves of θθ-plurisubharmonic functions with full mass a…

2016-06-05abs ↗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.

The Miyaoka-Yau inequality is proven for certain singular varieties with big canonical or anticanonical divisors.

problem Establishing the Miyaoka-Yau inequality for singular varieties with specific divisors.
method Defining the non-pluripolar product and establishing the Bogomolov-Gieseker type inequality for Higgs sheaves; investigating second Chern class inequalities.
result Proven the Miyaoka-Yau inequality for projective klt varieties with big canonical or anticanonical divisors.

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.

We show that normalized currents of integration along the common zeros of random mm-tuples of sections of powers of mm singular Hermitian big line bundles on a compact Kähler manifold distribute asymptotically to the wedge product of the curvature currents of the metrics. If the Hermitian metrics are Hölder with sing…

2015-06-04abs ↗pdf ↗

We use integrable systems techniques to study the singularities of timelike non-minimal constant mean curvature (CMC) surfaces in the Lorentz-Minkowski 3-space. The singularities arise at the boundary of the Birkhoff big cell of the loop group involved. We examine the behaviour of the surfaces at the big cell boundary,…

2011-10-20abs ↗pdf ↗

J. Nitsche proved that an isolated singularity of a conformal hyperbolic metric is either a conical singularity or a cusp one. We prove by developing map that there exists a complex coordinate zz centered at the singularity where the metric has the expression of either $\displaystyle{\frac{4α^2\vert z \vert^{2α-2}}{(1…

2017-11-03abs ↗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 ↗