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相关论文: From Little Bangs to the Big Bang

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In popular cold dark matter cosmological scenarios, stars may have first appeared in significant numbers around a redshift of 10 or so, as the gas within protogalactic halos with virial temperatures in excess of 20,000 K (corresponding to…

天体物理学 · 物理学 2007-05-23 Piero Madau

In this note, it is shown that nonvanishing spatial curvature produces primordial matter in the initially empty universe due to quantum gravity effects. This matter decays faster than radiation and is described by a stiff equation of state.…

广义相对论与量子宇宙学 · 物理学 2026-04-14 V. E. Kuzmichev , V. V. Kuzmichev

We calculate the present expansion of our Universe endowed with relict colored objects - quarks and gluons - that survived hadronization either as isolated islands of quark-gluon "nuggets", or spread uniformly in the Universe. In the first…

宇宙学与河外天体物理 · 物理学 2013-08-05 Maxim Brilenkov , Maxim Eingorn , Laszlo Jenkovszky , Alexander Zhuk

A rapid phase of accelerated expansion in the early universe, known as inflation, dilutes all matter except the vacuum induced quantum fluctuations. These are responsible for seeding the initial perturbations in the baryonic matter, the…

高能物理 - 唯象学 · 物理学 2011-06-28 Anupam Mazumdar

For two decades the hot big-bang model as been referred to as the standard cosmology -- and for good reason. For just as long cosmologists have known that there are fundamental questions that are not answered by the standard cosmology and…

天体物理学 · 物理学 2009-10-31 Michael S. Turner

Dark matter, proposed decades ago as a speculative component of the universe, is now known to be the vital ingredient in the cosmos, eight times more abundant than ordinary matter, one quarter of the total energy density and the component…

天体物理学 · 物理学 2009-09-15 Jeremiah P. Ostriker , Paul J. Steinhardt

The hot big-bang cosmology provides a reliable accounting of the Universe from about $10^{-2}\sec$ after the bang until the present, as well as a robust framework for speculating back to times as early as $10^{-43}\sec$. Cosmology faces a…

天体物理学 · 物理学 2014-10-13 Michael S. Turner

Mechanisms for the generation of the matter-antimatter asymmetry and dark matter strongly depend on the reheating temperature T_R, the maximal temperature reached in the early universe. Forthcoming results from the LHC, low energy…

高能物理 - 唯象学 · 物理学 2012-12-17 Wilfried Buchmuller

For two decades the hot big-bang model has been referred to as the standard cosmology -- and for good reason. For just as long cosmologists have known that there are fundamental questions that are not addressed by the standard cosmology and…

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

Over the past few decades, a consensus picture has emerged in which roughly a quarter of the universe consists of dark matter. I begin with a review of the observational evidence for the existence of dark matter: rotation curves of…

宇宙学与河外天体物理 · 物理学 2017-05-31 Katherine Freese

The standard theory of cosmic structure formation posits that the present-day rich structure of the Universe developed through gravitational amplification of tiny matter density fluctuations generated in its very early history. Recent…

宇宙学与河外天体物理 · 物理学 2009-06-25 Naoki Yoshida

As we follow our Universe to early times, we find that matter was crushed to high densities, somewhat similar to the behavior at a black hole singularity. String theory has made progress in explaining the internal structure of black holes,…

高能物理 - 理论 · 物理学 2008-12-18 Samir D. Mathur

Based on the results from numerous astrophysics experiments, it is currently believed that the majority of matter in the Universe is in some unknown form, known as dark matter. In the past it has been common to model dark matter as a…

高能物理 - 唯象学 · 物理学 2008-12-25 Chris Bird

An introductory account is given of the modern understanding of the physics of the early Universe. Particular emphasis is placed on the paradigm of cosmological inflation, which postulates a period of accelerated expansion during the…

天体物理学 · 物理学 2008-02-03 Andrew R Liddle

A model concerning particle theory and cosmology is proposed. Matter field, dark matter and dark energy are created by an energy flow from space to primordial matter fields at the phase transition in the early universe.

综合物理 · 物理学 2024-10-08 Masayasu Tsuge

The origin of dark matter in the universe may be scalar particles produced by amplification of quantum fluctuations during a period of dilaton-driven inflation. We show, for the first time, that a single species of particles, depending on…

高能物理 - 唯象学 · 物理学 2009-10-31 Ram Brustein , Merav Hadad

The physics of the 20th Century is governed by two pillars, Einstein's relativity principle and the quantum principle. At the beginning of the 21st Century, it becomes clear that there exist the smallest units of matter, such as electrons,…

宇宙学与河外天体物理 · 物理学 2017-01-16 W-Y. Pauchy Hwang , Sang Pyo Kim

Our universe appears to have been created not out of nothing but from a strange space-time dust. Quantum geometry (loop quantum gravity) makes it possible to avoid the ominous beginning of our universe with its physically unrealistic (i.e.…

科普物理 · 物理学 2007-05-23 Ruediger Vaas

Physical process version of the first law of black hole thermodynamics in Einstein- Maxwell dark matter gravity was derived. The dark matter sector is mimicked by the additional U(1)-gauge field coupled to the ordinary Maxwell one. By…

高能物理 - 理论 · 物理学 2019-02-01 Marek Rogatko , Aneta Wojnar

Was the primordial universe turbulent or non-turbulent soon after the Big Bang? How did the hydrodynamic state of the early universe affect the formation of structure from gravitational forces, and how did the formation of structure by…

天体物理学 · 物理学 2007-05-23 Carl H. Gibson