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相关论文: Speed of Gravity and Gravitational Horizon

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If gravitons are super-strong interacting particles and the low-temperature graviton background exists, the basic cosmological conjecture about the Dopplerian nature of redshifts may be false. In this case, a full magnitude of cosmological…

高能物理 - 理论 · 物理学 2007-05-23 Michael A. Ivanov

We point out that the physics at the extreme IR---cosmology---might provide tests of the physics of the extreme UV---the Weak Gravity Conjecture. The current discrepancies in the determination of $H_0$ may hint at a modification of…

高能物理 - 理论 · 物理学 2019-11-11 Nemanja Kaloper

It has recently been suggested that the acceleration of the Universe can be explained as the backreaction effect of superhorizon perturbations using second order perturbation theory. If this mechanism is correct, it should also apply to a…

高能物理 - 理论 · 物理学 2009-11-11 Eanna E. Flanagan

The gravitational force harbours a fundamental instability against collapse. In standard General Relativity without Quantum Mechanics, this implies the existence of black holes as natural, stable solutions of Einstein's equations. If one…

广义相对论与量子宇宙学 · 物理学 2017-08-23 Gerard 't Hooft

If a civilization embarks on high-speed intergalactic expansion, growing to a cosmological scale over time, communication between remote galaxies in the civilization will incur an extreme time delay, due to the distance involved. Indeed, if…

科普物理 · 物理学 2022-08-17 S. Jay Olson

The universe's current acceleration is a pretty recent phenomenon in cosmological time scales. This means that the modes that have left our horizon since the beginning of the contemporary acceleration phase, have not really reached the…

高能物理 - 理论 · 物理学 2023-08-23 A. Ashoorioon , A. Yousefi-Sostani

The Hubble law is extended to massive particles based on the de Broglie wavelength. Due to the expansion of the universe the wavelength of an unbound particle would increase according to its cosmological redshift. Based on the navigation…

广义相对论与量子宇宙学 · 物理学 2009-11-11 Firmin J. Oliveira

Recent observational evidences of accelerating phase of the universe strongly demand that the dominating matter in the universe is in the form of dark energy. In this work, we study the evolution of the apparent and event horizons for…

广义相对论与量子宇宙学 · 物理学 2015-05-28 Ritabrata Biswas , Nairwita Mazumder , Subenoy Chakraborty

From Doppler tracking data and data on circular motion of astronomical objects we obtain a metric of the Pioneer Anomaly. The metric resolves the issue of manifest absence of anomaly acceleration in orbits of the outer planets and…

广义相对论与量子宇宙学 · 物理学 2009-08-14 I. A. Siutsou , L. M. Tomilchik

The introduction of coordinates representing the points of view of various observers results in the possibility of horizons when acceleration and gravitation are included. A horizon is a surface of possible light beams in a region of space…

广义相对论与量子宇宙学 · 物理学 2007-06-26 James Lindesay

I show that gravitational scattering of dark-matter objects of 10^4 solar masses and speeds of 10 km/s, provides the cross-section per unit mass required in self-interacting dark matter models that alleviate the small-scale structure…

宇宙学与河外天体物理 · 物理学 2022-04-27 Abraham Loeb

The information loss paradox is widely regarded as one of the biggest open problems in theoretical physics. Several classical and quantum features must be present to enable its formulation. First, an event horizon is needed to justify the…

广义相对论与量子宇宙学 · 物理学 2024-08-20 Robert B. Mann , Sebastian Murk , Daniel R. Terno

The mysterious `dark energy' needed to explain the current observations, poses a serious confrontation between fundamental physics and cosmology. The present crisis may be an outcome of the (so far untested) prediction of the general theory…

广义相对论与量子宇宙学 · 物理学 2020-05-19 Ram Gopal Vishwakarma

At sufficiently large radii dark energy modifies the behavior of (a) bound orbits around a galaxy and (b) virialized gas in a cluster of galaxies. Dark energy also provides a natural cutoff to a cluster's dark matter halo. In (a) there…

宇宙学与河外天体物理 · 物理学 2024-07-03 Kristen Lackeos , Richard Lieu

The particles of a dark matter due to gravitational interaction deviate from straight trajectories in the vicinity of a massive body. This causes their density to become inhomogeneous. The developed density contrast causes a gravitation…

宇宙学与河外天体物理 · 物理学 2013-01-29 S. L. Parnovsky

General Relativistic Entropic Acceleration (GREA) theory provides a covariant formalism for out-of-equilibrium phenomena in GR, extending the Einstein equations with an entropic force that behaves like bulk viscosity with a negative…

宇宙学与河外天体物理 · 物理学 2024-05-28 Juan Garcia-Bellido

Massive gravity with second and fourth derivatives is shown to give both attractive and repulsive gravities. In contrast to the attractive gravity correlated with the energy-momentum tensor, the repulsive gravity is related to a fixed mass…

天体物理学 · 物理学 2007-05-23 Xiang-Song Chen

The discovery of cosmic acceleration has stimulated theorists to consider dark energy or modifications to Einstein's General Relativity as possible explanations. The last decade has seen advances in theories that go beyond smooth dark…

For the past forty years the search for dark matter has been one of the primary foci of astrophysics, although there has yet to be any direct evidence for its existence (Porter et al. 2011). Indirect evidence for the existence of dark…

宇宙学与河外天体物理 · 物理学 2015-06-11 F. Elliott Koch , Angus H. Wright

If general relativity is the correct theory of physics on large scales, then there is a differential equation that relates the Hubble expansion function, inferred from measurements of angular diameter distance and luminosity distance, to…

天体物理学 · 物理学 2011-02-01 Mustapha Ishak , Amol Upadhye , David N. Spergel