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相关论文: Crypto-baryonic Dark Matter

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We propose that dark matter consists of collections of atoms encapsulated inside pieces of an alternative vacuum, in which the Higgs field vacuum expectation value is appreciably smaller than in the usual vacuum. The alternative vacuum is…

天体物理学 · 物理学 2007-05-23 C. D. Froggatt , H. B. Nielsen

A component of the dark matter could consist of two darkly charged particles with a large mass ratio and a massless force carrier. This `atomic' dark sector could behave much like the baryonic sector, cooling and fragmenting down to…

星系天体物理 · 物理学 2018-07-04 Akshay Ghalsasi , Matthew McQuinn

A comet-like, but magnitudes smaller, extremely low albedo interstellar meteoroid population of fragile aggregates with solar type composition, measured in space and terrestrially, is most probably the universal dark matter. Although…

天体物理学 · 物理学 2007-05-23 Robert K. Soberman , Maurice Dubin

We suggest that dark matter is made up of massive quark objects that have survived from the Big Bang, representing the ground state of ``baryonic'' matter. Hence, there was no overall phase transition of the original quark matter, but only…

天体物理学 · 物理学 2007-05-23 S. Fredriksson , D. Enstrom , J. Hansson , S. Ekelin , A. Nicolaidis

The nonbaryonic dark matter of the Universe is assumed to consist of new stable particles. A specific case is possible, when new stable particles bear ordinary electric charge and bind in heavy "atoms" by ordinary Coulomb interaction. Such…

宇宙学与河外天体物理 · 物理学 2015-03-17 Maxim Yu. Khlopov , Andrey G. Mayorov , Evgeny Yu. Soldatov

Dark Matter might be an accidentally stable baryon of a new confining gauge interaction. We extend previous studies exploring the possibility that the DM is made of dark quarks heavier than the dark confinement scale. The resulting…

高能物理 - 唯象学 · 物理学 2017-11-21 Andrea Mitridate , Michele Redi , Juri Smirnov , Alessandro Strumia

In the simple Higgs-portal dark matter model with a conserved dark matter number, we show that there exists a non-topological soliton state of dark matter. This state has smaller energy per dark matter number than a free particle state and…

高能物理 - 唯象学 · 物理学 2019-10-02 Eduardo Pontón , Yang Bai , Bithika Jain

Baryonic matter in the core of a massive and evolved star is compressed significantly to form a supra-nuclear object, and compressed baryonic matter (CBM) is then produced after supernova. The state of cold matter at a few nuclear density…

高能天体物理现象 · 物理学 2013-07-23 Yanjun Guo , Renxin Xu

We continue our work on a proposal for what dark matter could be, namely that the dark matter consists of essentially macroscopic objects built from ordinary matter. The only element of new physics is that there should exist several types…

高能物理 - 唯象学 · 物理学 2023-05-23 Holger Bech Nielsen , Colin D. Froggatt

The recently observed Deuterium abundance in a low- metallicity high-redshift hydrogen cloud, which is about ten times larger than that observed in the near interstellar medium, is that expected from the Standard Big Bang Nucleosynthesis…

天体物理学 · 物理学 2009-10-28 Arnon Dar

We propose that dark matter is dominantly comprised of atomic bound states. We build a simple model and map the parameter space that results in the early universe formation of hydrogen-like dark atoms. We find that atomic dark matter has…

高能物理 - 唯象学 · 物理学 2015-05-14 David E. Kaplan , Gordan Z. Krnjaic , Keith R. Rehermann , Christopher M. Wells

We propose a new strategy to search for a particular type of dark matter via nuclear capture. If the dark matter particle carries baryon number, as motivated by a class of theoretical explanations of the matter-antimatter asymmetry of the…

高能物理 - 唯象学 · 物理学 2020-10-27 Bartosz Fornal , Benjamin Grinstein , Yue Zhao

Assuming existence of (very) heavy fourth generation of quarks and antiquarks we argue that antibaryon composed of the three heavy antiquarks can be light, stable and invisible, hence a good candidate for the Dark matter particle. Such…

高能物理 - 唯象学 · 物理学 2013-03-26 D. Gorbunov , P. Pakhlov

We study the possibility that dark matter is a baryon of a new strongly interacting gauge theory, which was introduced in the low energy theory of Cosmological SUSY Breaking (CSB). This particle can fit the observed dark matter density if…

高能物理 - 唯象学 · 物理学 2009-11-11 T. Banks , J. D. Mason , D. O'Neil

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

An initial state for the observable universe consisting of a finite region with a large vacuum energy will break-up due to near horizon quantum critical fluctuations. This will lead to a Friedmann-like early universe consisting of an…

宇宙学与河外天体物理 · 物理学 2010-05-04 George Chapline

"Dark quark nuggets", a lump of dark quark matter, can be produced in the early universe for a wide range of confining gauge theories and serve as a macroscopic dark matter candidate. The two necessary conditions, a nonzero dark baryon…

高能物理 - 唯象学 · 物理学 2019-11-26 Yang Bai , Andrew J. Long , Sida Lu

The state of cold bulk matter at around nuclear density depends on the fundamental strong interaction between quarks at low-energy scale, so-called non-perturbative quantum chromo-dynamics. Such kind of matter is conjectured to be condensed…

高能天体物理现象 · 物理学 2015-07-28 Renxin Xu

The quantum model of the homogeneous, isotropic, and spatially closed universe predicts an existence of two types of collective quantum states in the universe. The states of one type characterize a gravitational field, the others describe a…

天体物理学 · 物理学 2007-05-23 V. E. Kuzmichev , V. V. Kuzmichev

Dark Matter is one of the most intriguing riddles of modern astrophysics. The Standard Cosmological Model implies that only 4.5% of the mass-energy of the Universe is baryonic matter and the remaining 95% is unknown. Of this remainder, 22%…

天体物理仪器与方法 · 物理学 2010-11-19 Andrzej M. Szelc
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