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The origin of the galaxies represents an important focus of current cosmological research, both observational and theoretical. Its resolution involves a comprehensive understanding of star formation, galaxy dynamics, the cosmology of the…

天体物理学 · 物理学 2009-11-10 Joseph Silk

Caustics are a generic feature of the nonlinear growth of structure in the dark matter distribution. If the dark matter were absolutely cold, its mass density would diverge at caustics, and the integrated annihilation probability would also…

天体物理学 · 物理学 2009-11-13 Simon D. M. White , Mark Vogelsberger

Motivated by inflation, the theory of big-bang nucleosynthesis and the quest for a deeper understanding of the fundamental forces and particles, a very successful paradigm for the development of structure in the Universe has evolved. It…

天体物理学 · 物理学 2009-10-28 Scott Dodelson , Evalyn Gates , Michael S. Turner

We study particle decay as the origin of dark radiation. After elaborating general properties and useful parametrisations we provide model-independent and easy-to-use constraints from nucleosynthesis, the cosmic microwave background and…

高能物理 - 唯象学 · 物理学 2014-02-14 Jasper Hasenkamp , Jörn Kersten

If the dark matter is produced in the early universe prior to Big Bang nucleosynthesis, a modified cosmological history can drastically affect the abundance of relic dark matter particles. Here, we assume that an additional species to…

高能物理 - 唯象学 · 物理学 2018-02-26 Francesco D'Eramo , Nicolas Fernandez , Stefano Profumo

We present a scenario for non-thermal production of dark matter from evaporation of primordial black holes. A period of very early matter domination leads to formation of black holes with a maximum mass of $\simeq 2 \times 10^8$ g, whose…

宇宙学与河外天体物理 · 物理学 2018-03-15 Rouzbeh Allahverdi , James B. Dent , Jacek Osinski

The first phase of stellar evolution in the history of the universe may be Dark Stars, powered by dark matter heating rather than by fusion. Weakly interacting massive particles, which are their own antiparticles, can annihilate and provide…

宇宙学与河外天体物理 · 物理学 2010-02-17 Paolo Gondolo , Katherine Freese , Douglas Spolyar , Anthony Aguirre , Peter Bodenheimer , Jeremy A. Sellwood , Naoki Yoshida

We demonstrate that if the universe is dominated by the massive cold dark matter, then besides the generally believed thermal distribution of the dark matter relics, there may exist some very energetic non-thermal relics of the dark matter…

高能物理 - 唯象学 · 物理学 2007-05-23 Xue-Qian Li , Zhijian Tao

The nonbaryonic dark matter of the Universe can consist of new stable charged leptons and quarks, if they are hidden in elusive "dark atoms" of composite dark matter. Such possibility can be compatible with the severe constraints on…

宇宙学与河外天体物理 · 物理学 2015-05-20 Maxim Yu. Khlopov

We propose that dark matter is not yet another new particle in nature, but that it is a remnant of quantum gravitational effects on known fields. We arrive at this possibility in an indirect and surprising manner: by considering retarded,…

高能物理 - 理论 · 物理学 2015-11-11 Mehdi Saravani , Siavash Aslanbeigi

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

We present a thorough analysis of the sequential freeze-in mechanism for dark matter production in the early universe. In this mechanism the dark matter relic density results from pair annihilation of mediator particles which are themselves…

高能物理 - 唯象学 · 物理学 2020-08-19 Genevieve Belanger , Cedric Delaunay , Alexander Pukhov , Bryan Zaldivar

Here, creation of the universe is obtained only from gravity sector. The dynamical universe begins with two basic ingredients (i) vacuum energy, also called dark energy (as vacuum energy is not observed) and (ii) background radiation. These…

高能物理 - 理论 · 物理学 2007-05-23 S. K. Srivastava

We consider the production of axion dark matter through the misalignment mechanism in the context of a nonstandard cosmological history involving early matter domination by a scalar field with a time-dependent decay rate. In cases where the…

高能物理 - 唯象学 · 物理学 2023-05-24 Paola Arias , Nicolás Bernal , Jacek K. Osiński , Leszek Roszkowski

High energy collisions of particles may have created tiny black holes in the early Universe, which might leave stable remnants instead of fully evaporating as a result of Hawking radiation. If the reheating temperature was sufficiently…

广义相对论与量子宇宙学 · 物理学 2019-04-03 Tomohiro Nakama , Jun'ichi Yokoyama

High energy neutrinos are produced by the annihilation of dark matter particles in our galaxy. These are presently searched for with large area, deep underground neutrino telescopes. Cold dark matter particles, trapped inside the sun, are…

高能物理 - 唯象学 · 物理学 2009-09-25 F. Halzen , J. E. Jacobsen

Dark matter can be produced in the early universe via the freeze-in or freeze-out mechanisms. Both scenarios were investigated in references, but the production of dark matters via the combination of these two mechanisms are not addressed.…

高能物理 - 唯象学 · 物理学 2018-05-15 Wei Chao

It is quite possible that the reheat temperature of the universe is extremely low close to the scale of Big Bang nucleosynthesis, i.e. $T_{R}\sim 1-10$ MeV. At such low reheat temperatures generating matter anti-matter asymmetry and…

高能物理 - 唯象学 · 物理学 2009-11-10 Kazunori Kohri , Anupam Mazumdar , Narendra Sahu

Dark matter constitutes the great majority of the matter content in the Universe, but its microscopic nature remains an intriguing mystery, with profound implications for particle physics, astrophysics and cosmology. Here we shed light on…

宇宙学与河外天体物理 · 物理学 2015-09-16 A. Lapi , L. Danese

Over the past three years we have determined the basic features of the Universe -- spatially flat; accelerating; comprised of 1/3 a new form of matter, 2/3 a new form of energy, with some ordinary matter and a dash of massive neutrinos; and…

天体物理学 · 物理学 2009-11-07 Michael S. Turner