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We propose a mirror model for ordinary and dark matter that assumes a new SU(3) gauge group of transformations, as a natural extension of the Standard Model (SM). A close study of big bang nucleosynthesis, baryon asymmetries, cosmic…

高能物理 - 唯象学 · 物理学 2017-03-22 O. Oliveira , C. A. Bertulani , M. S. Hussein , W. de Paula , T. Frederico

There exist a range of exciting scientific opportunities for Big Bang Nucleosynthesis (BBN) in the coming decade. BBN, a key particle astrophysics "tool" for decades, is poised to take on new capabilities to probe beyond standard model…

宇宙学与河外天体物理 · 物理学 2019-07-23 Evan B. Grohs , J. Richard Bond , Ryan J. Cooke , George M. Fuller , Joel Meyers , Mark W. Paris

Primordial nucleosynthesis is considered a success story of the standard big bang (SBB) cosmology. The cosmological and elementary particle physics parameters are believed to be severely constrained by the requirement of correct abundances…

天体物理学 · 物理学 2007-05-23 Daksh Lohiya , Shobhit Mahajan , A. Mukherjee , Annu Batra

The hypothesis that dark matter consists of superheavy particles with the mass close to the Grand Unification scale is investigated. These particles were created from vacuum by the gravitation of the expanding Universe and their decay led…

广义相对论与量子宇宙学 · 物理学 2008-11-26 A. A. Grib , Yu. V. Pavlov

The instability of dark matter may produce visible signals in the spectrum of cosmic gamma-rays. We consider this possibility in frameworks with additional spatial dimensions and supersymmetry. Examples of particles include…

天体物理学 · 物理学 2011-11-10 Jose A. R. Cembranos , Jonathan L. Feng , Louis E. Strigari

The Standard Model of Particle Physics has been verified to unprecedented precision in the last few decades. However there are still phenomena in nature which cannot be explained, and as such new theories will be required. Since terrestrial…

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

A brief review is given of some recent works where baryogenesis and dark matter have a common origin within the $U(1)$ extensions of the standard model and of the minimal supersymmetric standard model. The models considered generate the…

高能物理 - 唯象学 · 物理学 2017-05-31 Wan-Zhe Feng , Pran Nath

Cosmic microwave background (CMB) observations suggest the possibility of an extra dark radiation component, while the current evidence from big bang nucleosynthesis (BBN) is more ambiguous. Dark radiation from a decaying particle can…

宇宙学与河外天体物理 · 物理学 2015-06-03 Justin L. Menestrina , Robert J. Scherrer

The identity of dark matter is one of the greatest puzzles of our Universe. Its solution may be associated with supersymmetry which is a fundamental space-time symmetry that has not been verified experimentally so far. In many…

高能物理 - 唯象学 · 物理学 2007-08-28 Frank Daniel Steffen

We argue that neutrino mass and dark matter can arise from an approximate $B-L$ symmetry. This idea can be realized in a minimal setup of the flipped 3-3-1 model, which discriminates lepton families while keeping universal quark families…

高能物理 - 唯象学 · 物理学 2020-05-22 Duong Van Loi , Phung Van Dong , Dang Van Soa

We consider the big bang nucleosynthesis (BBN) in the Brane world scenario, where all matter fields are confined on our 3-brane and the radion of the Brane evolves cosmologically. In the Einstein frame fundamental fermion masses vary and…

天体物理学 · 物理学 2009-11-13 Baojiu Li , Ming-Chung Chu

We present a realistic, simple and natural model of strongly-interacting dark matter based on the neutrino-portal paradigm. The strong interactions at small velocities are generated by the exchange of dark photons, and produce the observed…

高能物理 - 唯象学 · 物理学 2021-01-20 J. M. Lamprea , E. Peinado , S. Smolenski , J. Wudka

We consider theories where dark matter is composed of a thermal relic of weak scale mass, whose couplings to the Standard Model (SM) are however too small to give rise to the observed abundance. Instead, the abundance is set by annihilation…

高能物理 - 唯象学 · 物理学 2016-01-18 Zackaria Chacko , Yanou Cui , Sungwoo Hong , Takemichi Okui

The process of neutron-mirror neutron oscillation, motivated by symmetric mirror dark matter models, is governed by two parameters: $n-n'$ mixing parameter $\delta$ and $n-n'$ mass splitting $\Delta$. For neutron mirror neutron oscillation…

高能物理 - 唯象学 · 物理学 2017-12-06 Rabindra N. Mohapatra , Shmuel Nussinov

The Standard Model of particle physics is governed by Poincar\'e symmetry, while all other symmetries, exact or approximate, are essentially dictated by theoretical consistency with the particle spectrum. On the other hand, many models of…

高能物理 - 唯象学 · 物理学 2020-04-28 Mark P. Hertzberg , McCullen Sandora

We review the Cosmology and Physics underlying Primordial Nucleosynthesis and survey current observational data in order to compare the predictions of Big Bang Nucleosynthesis with the inferred primordial abundances. From this comparison we…

天体物理学 · 物理学 2008-11-26 Keith A. Olive , Gary Steigman , Terry P. Walker

We study cosmological constraints on the asymmetric mediator scenario, a variant of the scotogenic model that addresses the origins of neutrino masses, dark matter (DM), and the baryon asymmetry. An SU(2)$_L$ doublet scalar $\eta$ mediates…

高能物理 - 唯象学 · 物理学 2025-12-17 Kento Asai , Seishi Enomoto , Takuya Hirose , Masato Yamanaka

We study direct detection of dark matter in supersymmetric (SUSY) model where most of SUSY particles have very high-scale masses beyond the weak scale. In the scenario, Wino-like or Higgsino-like neutralino is a good candidate for the dark…

高能物理 - 唯象学 · 物理学 2013-03-04 Junji Hisano , Koji Ishiwata , Natsumi Nagata

Primordial nucleosynthesis is considered a success story of the standard big bang (SBB) cosmology. The cosmological and elementary particle physics parameters are believed to be severely constrained by the requirement of correct abundances…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Daksh Lohiya , Annu Batra , Shobhit Mahajan , Amitabha Mukherjee

Following a brief introduction to early Universe cosmology, the current of status of big bang nucleosynthesis is reviewed and the concordance between theory and observation is examined in detail. The abundances of He4 and Li7 determine the…

天体物理学 · 物理学 2007-05-23 Keith A. Olive