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相关论文: Cosmology with Negative Absolute Temperatures

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The laws of thermodynamics in the expanding universe are formulated within the quasi-metric framework. Since the quasi-metric cosmic expansion does not directly influence momenta of material particles, so that the expansion directly cools…

广义相对论与量子宇宙学 · 物理学 2025-01-14 Dag Østvang

The presence of dark energy in the Universe is inferred directly and indirectly from a large body of observational evidence. The simplest and most theoretically appealing possibility is the vacuum energy density (cosmological constant).…

天体物理学 · 物理学 2008-11-26 J. S. Alcaniz

We investigate the cosmological behavior in a universe governed by time asymmetric extensions of general relativity, which is a novel modified gravity based on the addition of new, time-asymmetric, terms on the Hamiltonian framework, in a…

广义相对论与量子宇宙学 · 物理学 2015-11-11 Genly Leon , Emmanuel N. Saridakis

While, to ensure successful cosmology, dark matter (DM) must kinematically decouple from the standard model plasma very early in the history of the Universe, it can remain coupled to a bath of "dark radiation" until a relatively late epoch.…

宇宙学与河外天体物理 · 物理学 2013-06-05 Francis-Yan Cyr-Racine , Kris Sigurdson

How would negative energy density affect a classic Friedmann cosmology? Although never measured and possibly unphysical, certain realizations of quantum field theories leaves the door open for such a possibility. In this paper we analyze…

宇宙学与河外天体物理 · 物理学 2015-06-11 Robert J. Nemiroff , Ravi Joshi , Bijunath R. Patla

Stars form when cold cosmic nebulae spontaneously develop hot spots that steadily intensify until they reach fusion temperatures. Without this process, the universe would be dark and dead. Yet the spontaneous concentration of heat is…

量子气体 · 物理学 2013-01-25 M. P. Strzys , J. R. Anglin

We investigate various dark energy models by taking into account the thermal effects induced from Hawking radiation on the apparent horizon of the Universe, for example near a finite-time future singularity. If the dark energy density…

广义相对论与量子宇宙学 · 物理学 2021-02-17 Artyom V. Astashenok , Sergei D. Odintsov , Vasilis K. Oikonomou

Quantum fields can notoriously violate the null energy condition (NEC). In a cosmological context, NEC violation can lead to, e.g., dark energy at late times with an equation-of-state parameter smaller than $-1$ and nonsingular bounces at…

广义相对论与量子宇宙学 · 物理学 2025-07-01 Elly Moghtaderi , Brayden R. Hull , Jerome Quintin , Ghazal Geshnizjani

For more seventy years physicists have appreciated that Nature's vacuum is far from empty. The discovery of the Lamb shift in Hydrogen provided dramatic verification of the reality of the quantum vacuum. The advent of gauge theories has led…

天体物理学 · 物理学 2007-05-23 Michael S. Turner

The concept of negative absolute temperature, introduced by Ramsey based on the study of a nuclear spin system by Purcell and Pound in 1951, has been subject to continued debate. According to a recent analysis by Struchtrup, the apparent…

经典物理 · 物理学 2019-10-07 Quanmin Guo

To explain the accelerating universe driven by dark energy, a so-called "entropy-corrected new agegraphic dark energy" (ECNADE), was recently proposed with the help of quantum corrections to the entropy-area relation in the framework of…

广义相对论与量子宇宙学 · 物理学 2011-04-21 Kayoomars Karami , Ahmad Sheykhi , Mubasher Jamil , F. Felegary , M. M. Soltanzadeh

A huge amount of good quality data converges towards the picture of a spatially flat universe undergoing the today observed phase of accelerated expansion. This new observational trend is commonly addressed as Precision Cosmology. Despite…

广义相对论与量子宇宙学 · 物理学 2008-12-02 S. Capozziello

In this paper we consider the effects of adding curvature in extended cosmologies involving a free-to-vary neutrino sector and different parametrizations of Dark Energy (DE). We make use of the Planck 2018 cosmic microwave background…

宇宙学与河外天体物理 · 物理学 2023-03-29 Weiqiang Yang , William Giarè , Supriya Pan , Eleonora Di Valentino , Alessandro Melchiorri , Joseph Silk

It has been claimed that the observed magnitude of the vacuum energy density is consistent with the distribution predicted in anthropic models, in which an ensemble of universes is assumed. This calculation is revisited, without making the…

天体物理学 · 物理学 2009-06-23 J. A. Peacock

In the contemporary Cosmology, dark energy is modeled as a perfect fluid, having a very simple equation of state: pressure is proportional to dark energy density. As an alternative, I propose a more complex equation of state, with pressure…

综合物理 · 物理学 2009-11-04 Dragan Slavkov Hajdukovic

The accelerating expansion of the universe is the most surprising cosmological discovery in many decades. In this short review, we briefly summarize theories for the origin of cosmic acceleration and the observational methods being used to…

宇宙学与河外天体物理 · 物理学 2014-01-03 Michael J. Mortonson , David H. Weinberg , Martin White

In this work, we study some thermodynamical aspects associated with torsion in a flat FLRW spacetime cosmic evolution. By implementing two Ansatze for the torsion term, we find that the model admits a phantom regime or a quintessence…

广义相对论与量子宇宙学 · 物理学 2020-06-26 Miguel Cruz , Fernando Izaurieta , Samuel Lepe

We have investigated the thermodynamical properties of the Universe with dark energy. Adopting the usual assumption in deriving the constant co-moving entropy density that the physical volume and the temperature are independent, we observed…

广义相对论与量子宇宙学 · 物理学 2010-10-27 Yungui Gong , Bin Wang , Anzhong Wang

This is an essay sketching the line of thinking which has led the present author to propose the constituent or atomic model of gravitation more than a decade ago. It turns out that viewing the problem of gravitation as a quantum many body…

天体物理学 · 物理学 2009-10-19 Pawel O. Mazur

In this paper a new theory of Dark Matter is proposed. Experimental analysis of several Galaxies show how the non-gravitational contribution to galactic Velocity Rotation Curves can be interpreted as that due to the Cosmological Constant…

天体物理学 · 物理学 2007-05-23 G. V. Kraniotis , S. B. Whitehouse