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相关论文: Dibaryons cannot be the dark matter

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A supercooled phase transition in a nearly conformal dark sector can provide a natural setting for darkogenesis via its out-of-equilibrium dynamics, where a particle-antiparticle number asymmetry in the dark sector can be reprocessed into…

高能物理 - 唯象学 · 物理学 2025-10-21 Sudhakantha Girmohanta , Yuichiro Nakai , Zhihao Zhang

I use Bousso's causal diamond measure to make a statistical prediction for the dark matter abundance, assuming an axion with a large decay constant f_a >> 10^{12} GeV. Using a crude approximation for observer formation, the prediction…

高能物理 - 理论 · 物理学 2015-05-13 Ben Freivogel

What is the upper limit of the mass of the neutralino dark matter whose thermal relic is consistent with the observation? If the neutralino dark matter and colored sparticles are extremely degenerated in mass, with a mass difference less…

高能物理 - 唯象学 · 物理学 2020-01-07 Hajime Fukuda , Feng Luo , Satoshi Shirai

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

Superluminal preons (superbradyons) with a critical speed in vacuum much larger than the speed of light would, if they exist, play a fundamental role as constituents of the physical vacuum and of the conventional particles considered in…

宇宙学与河外天体物理 · 物理学 2010-12-15 Luis Gonzalez-Mestres

Dwarf spheroidal galaxies provide well-known challenges to the standard cold and collisionless dark matter scenario: The too-big-to-fail problem, namely the mismatch between the observed mass enclosed within the half-light radius of dwarf…

星系天体物理 · 物理学 2018-08-29 Mauro Valli , Hai-Bo Yu

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

In this Letter, we propose a new possible connection between dark matter relic density and baryon asymmetry of the universe. The portal between standard model sector and dark matter not only controls the relic density and detections of dark…

高能物理 - 唯象学 · 物理学 2015-05-30 Talal Ahmed Chowdhury , Miha Nemevsek , Goran Senjanovic , Yue Zhang

We study the evolution of matter composition from nuclear to quark densities in the confining regime, by extending an ideal model of Quarkyonic matter, IdylliQ model, to multi-flavor systems including strangeness. The model provides a dual…

核理论 · 物理学 2026-03-24 Yuki Fujimoto , Toru Kojo , Larry McLerran

We investigate the existence of bound states of baryons in a kaon condensate using chiral mean field theory. The interactions are described by an effective SU(3)_L X SU(3)_R chiral lagrangian where terms of higher order in density, baryon…

高能物理 - 唯象学 · 物理学 2016-09-06 Bruce Ritzi , Graciela Gelmini

It is proposed that dark matter could consist of compressed collections of atoms (or metallic matter) encapsulated into, for example, 20 cm big pieces of a different phase. The idea is based on the assumption that there exists at least one…

天体物理学 · 物理学 2009-11-16 C. D. Froggatt , H. B. Nielsen

The similar densities of dark matter and baryons in the universe imply that they might arise from the same ultraviolet model. The B-Mesogenesis, which assumes dark matter is charged under the baryon number, attempts to simultaneously…

高能物理 - 唯象学 · 物理学 2024-08-20 Yong Zheng , Jian-Nan Ding , Dong-Hao Li , Lei-Yi Li , Cai-Dian Lü , Fu-Sheng Yu

The $SU(3)_c^{}\times SU(2)_L^{} \times U(1)_Y^{}$ standard model is extended by a $U(1)_{B-L}^{}$ gauge symmetry with four right-handed neutrinos. Because of their Yukawa couplings to a Higgs singlet for spontaneously breaking the…

高能物理 - 唯象学 · 物理学 2025-08-21 Pei-Hong Gu

We propose a scenario with a fermion dark matter, where the dark matter particle used to be the Dirac fermion, but it takes the form of the Majorana fermion at a late time. The relic number density of the dark matter is determined by the…

高能物理 - 唯象学 · 物理学 2015-06-05 Nobuchika Okada , Osamu Seto

We study the effect of a first-order phase transition in a confining $SU(N)$ dark sector with heavy dark quarks. The baryons of this sector are the dark matter candidate. During the confinement phase transition the heavy quarks are trapped…

高能物理 - 唯象学 · 物理学 2021-11-24 Pouya Asadi , Eric David Kramer , Eric Kuflik , Gregory W. Ridgway , Tracy R. Slatyer , Juri Smirnov

The general character of 4-quark (mesonic) and strange 6-quark (baryonic) quark systems is very briefly reviewed a la Jaffe, i.e. in the MIT bag, and so far still possibly viable candidates are indicated. Concentration is on S=-2 systems.…

核理论 · 物理学 2015-06-26 D. E. Kahana , S. H. Kahana

Dark matter is postulated to be a neutral Dirac fermion, charged under a dark $U(1)_D$ gauge symmetry. Scalar partners of the quarks and leptons are also charged under $U(1)_D$. The dark gauge boson $Z_D$ and the dark Higgs boson $h_D$…

高能物理 - 唯象学 · 物理学 2022-07-06 Ernest Ma

From a systematic analysis of the energy-dependence of four antibaryon-to-baryon ratios relative to the antikaon-to-kaon ratio, we propose an alternative approach determining the strange-quark chemical potential ($\mu_{\mathrm{s}}$). It is…

高能物理 - 唯象学 · 物理学 2017-08-03 Abdel Nasser Tawfik , Magda Abdel Wahab , Hayam Yassin , Eman R. Abo Elyazeed , Hadeer M. Nasr El Din

The evidence is that the mass of the universe is dominated by an exotic nonbaryonic form of matter largely draped around the galaxies. It approximates an initially low pressure gas of particles that interact only with gravity, but we know…

宇宙学与河外天体物理 · 物理学 2017-01-23 P. J. E. Peebles

If a bosonic partner of a right-handed neutrino dominates the early universe sufficiently before its decay, important ingredients in the present universe are related to physics of the right-handed neutrino sector. In particular, we find…

高能物理 - 唯象学 · 物理学 2009-11-10 M. Ibe , T. Yanagida
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