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We investigate Big Bang nucleosynthesis (hereafter, BBN) in a cosmic environment characterized by a distribution of small-scale matter/antimatter domains. Production of antimatter domains in a baryo-asymmetric universe is predicted in some…

Astrophysics · Physics 2009-10-30 Jan B. Rehm , Karsten Jedamzik

High energy particles are produced by the annihilation of dark matter particles in our galaxy. These are presently searched for using balloon-borne antiproton and positron detectors and large area, deep underground neutrino telescopes. Dark…

High Energy Physics - Phenomenology · Physics 2016-09-01 F. Halzen , J. E Jacobsen

Big-bang nucleosynthesis (BBN) theory, together with the precise WMAP cosmic baryon density, makes tight predictions for the abundances of the lightest elements. Deuterium and 4He measurements agree well with expectations, but 7Li…

Cosmology and Nongalactic Astrophysics · Physics 2012-03-19 Brian D. Fields

It is postulated that the energy density of the (quantum) vacuum acts firstly as dark energy and secondly as a part of dark matter. Assisted by electric fields arising from a small charge mismatch in the cosmic plasma, it can condense on…

General Physics · Physics 2024-06-19 Theodorus Maria Nieuwenhuizen

Evidence of neutron stars with deconfined quark-matter cores suggest a new pathway for the evolution of black holes. New theories about the cores of neutron stars support the idea that quarkonium is likely to grow there as the neutron star…

High Energy Physics - Phenomenology · Physics 2025-03-04 Zachary R. Smith , Neil F. Comins

Macroscopic dark matter with dominating strong interactions, supposed to be composites, represents an alternative to the most popular WIMP particles. Predicted in various models as strangelets, nuclearites, nuggets, having different…

High Energy Physics - Phenomenology · Physics 2026-04-01 Ionel Lazanu , Konstantin Zioutas

We propose a new dark matter candidate, quirky dark matter, that is a scalar baryonic bound state of a new non-Abelian force that becomes strong below the electroweak scale. The bound state is made of chiral quirks: new fermions that…

High Energy Physics - Phenomenology · Physics 2010-05-25 Graham D. Kribs , Tuhin S. Roy , John Terning , Kathryn M. Zurek

We propose a novel scenario to explain the observed cosmological asymmetry between matter and antimatter, based on nonperturbative QCD physics. This scenario relies on a mechanism of separation of quarks and antiquarks in two coexisting…

High Energy Physics - Phenomenology · Physics 2009-11-10 David H. Oaknin , Ariel Zhitnitsky

Several lines of evidence suggest that some of the dark matter may be non-baryonic: the non-detection of various plausible baryonic candidates for dark matter inferred, e.g., from galaxy rotation curves and from cluster of galaxy velocity…

Astrophysics · Physics 2007-05-23 David N. Spergel

The products of primordial nucleosynthesis and the cosmic microwave background (CMB) photons are relics from the early evolution of the Universe whose observations probe the standard model of cosmology and provide windows on new physics…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 Gary Steigman

In grand unified theories with gauge groups larger than SU(5), the multiplets that contain the known quarks and leptons also contain fermions that are singlets under the Standard Model gauge group. Some of these could be the dark matter of…

High Energy Physics - Phenomenology · Physics 2013-05-30 S. M. Barr

We present a mechanism to generate the baryon asymmetry of the Universe which preserves the net baryon number created in the Big Bang. If dark matter particles carry baryon number $B_X$, and $\sigma^{\rm annih}_{\bar{X}} < \sigma^{\rm…

High Energy Physics - Phenomenology · Physics 2009-11-11 Glennys R. Farrar , Gabrijela Zaharijas

Dark matter can be captured by celestial objects and accumulate at their centers, forming a core of dark matter that can collapse to a small black hole, provided that the annihilation rate is small or zero. If the nascent black hole is big…

High Energy Physics - Phenomenology · Physics 2021-05-13 Javier F. Acevedo , Joseph Bramante , Alan Goodman , Joachim Kopp , Toby Opferkuch

The quark star is such an exotic star of our Universe. The limiting mass for quark stars essentially depends on rotational frequency apart from bag constant and other fundamental parameters. The analytical results obtained agree with the…

High Energy Physics - Phenomenology · Physics 2024-11-05 Ashadul Halder

The cosmic first order phase transition from quarks to hadrons, occurring a few microseconds after the Big Bang, would lead to the formation of quark nuggets which would be stable on a cosmological time scale, if the associated baryon…

Astrophysics · Physics 2011-02-11 Jan-e Alam , Sibaji Raha , Bikash Sinha

Our world is wonderful because of the normal but negligibly small baryonic part (i.e., atoms) although unknown dark matter and dark energy dominate the Universe. A stable atomic nucleus could be simply termed as ``strong matter'' since its…

High Energy Physics - Phenomenology · Physics 2022-11-08 Xiaoyu Lai , Chengjun Xia , Renxin Xu

If the preon structure of quarks, leptons and gauge bosons will be proved then in the Universe during relativistic phase transition the production of nonperturbative preon condensates has been occured collective excitations of which are…

High Energy Physics - Phenomenology · Physics 2009-09-25 V. Burdyuzha , O. Lalakulich , Yu. Ponomarev , G. Vereshkov

Based on a scenario of the inhomogeneous big-bang nucleosynthesis (IBBN), we investigate the detailed nucleosynthesis that includes the production of heavy elements beyond Li-7. From the observational constraints on light elements of He4…

Cosmology and Nongalactic Astrophysics · Physics 2013-07-08 Riou Nakamura , Masa-aki Hashimoto , Shin-ichiro Fujimoto , Nobuya Nishimura , Katsuhiko Sato

Big-Bang nucleosynthesis (BBN) represents one of the earliest phenomena that can lead to observational constraints on the early Universe properties. It is well-known that many important mechanisms and phase transitions occurred before BBN.…

High Energy Physics - Phenomenology · Physics 2018-12-03 A. Arbey , J. Ellis , F. Mahmoudi , G. Robbins

In the context of the relationship between physics of cosmological dark matter and symmetry of elementary particles a wide list of dark matter candidates is possible. New symmetries provide stability of different new particles and their…

High Energy Physics - Phenomenology · Physics 2017-04-26 M. Yu. Khlopov
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