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相关论文: Branons as dark matter

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An extension of the Standard Model by three right-handed neutrinos with masses smaller than the electroweak scale (the $\nu$MSM) can explain simultaneously dark matter and baryon asymmetry of the Universe, being consistent with the data on…

天体物理学 · 物理学 2016-11-15 Mikhail Shaposhnikov

Braneworld models with variable brane tension $\lambda $ introduce a new degree of freedom that allows for evolving gravitational and cosmological constants, the latter being a natural candidate for dark energy. We consider a thermodynamic…

广义相对论与量子宇宙学 · 物理学 2011-03-28 K. C. Wong , K. S. Cheng , T. Harko

We calculate the present expansion of our Universe endowed with relict colored objects - quarks and gluons - that survived hadronization either as isolated islands of quark-gluon "nuggets", or spread uniformly in the Universe. In the first…

宇宙学与河外天体物理 · 物理学 2013-08-05 Maxim Brilenkov , Maxim Eingorn , Laszlo Jenkovszky , Alexander Zhuk

We point out a novel role for the Standard Model neutrino in dark matter phenomenology where the exchange of neutrinos generates a long-range potential between dark matter particles. The resulting dark matter self interaction could be…

高能物理 - 唯象学 · 物理学 2021-10-13 Nicholas Orlofsky , Yue Zhang

Dark matter and neutrinos provide the two most compelling pieces of evidence for new physics beyond the Standard Model of Particle Physics but they are often treated as two different sectors. The aim of this paper is to determine whether…

高能物理 - 唯象学 · 物理学 2018-05-09 Andres Olivares-Del Campo , Celine Boehm , Sergio Palomares-Ruiz , Silvia Pascoli

The assumption that our Universe is close to a late time fixed point of the equations of cosmology, leads to a modification of the latter to include energy exchange between the matter and the "dark energy". The brane-world scenario provides…

高能物理 - 唯象学 · 物理学 2007-05-23 Theodore N. Tomaras

A recent baryogenesis scenario [Phys. Rev. D 110, 023520 (2024)], rooted in a two-brane Universe model, proposed a solution to the matter-antimatter asymmetry through the dynamics of a new pseudo-scalar field. In the present paper, one…

高能物理 - 唯象学 · 物理学 2025-10-24 Michaël Sarrazin

We investigate if the fluctuations of the scalar field mediating quintessence -- the cosmon -- can play an important role in cosmology. Small fluctuations with short wavelength behave similar to a relativistic gas. In contrast, the…

高能物理 - 唯象学 · 物理学 2009-11-07 C. Wetterich

This paper presents a brief review of the evidence for dark matter in the Universe on the scales of galaxies. In the interests of critically and objectively testing the dark matter paradigm on these scales, this evidence is weighed against…

天体物理学 · 物理学 2016-11-03 M. R. Merrifield

We consider a class of theories in which neutrino masses depend significantly on environment, as a result of interactions with the dark sector. Such theories of mass varying neutrinos (MaVaNs) were recently introduced to explain the origin…

高能物理 - 唯象学 · 物理学 2009-11-10 David B. Kaplan , Ann E. Nelson , Neal Weiner

We consider the brane gas picture of the early universe. At later stages, when there are no winding modes and the background is free to expand, we show that a moving 3-brane, which we identify with our universe, can inflate even though it…

高能物理 - 唯象学 · 物理学 2009-11-07 M. F. Parry , D. A. Steer

The origin of dark matter in the universe may be weakly interacting scalar particles produced by amplification of quantum fluctuations during a period of dilaton-driven inflation. We present two interesting cases, the case of small…

高能物理 - 唯象学 · 物理学 2009-10-31 Ram Brustein , Merav Hadad

Dark matter, proposed decades ago as a speculative component of the universe, is now known to be the vital ingredient in the cosmos, eight times more abundant than ordinary matter, one quarter of the total energy density and the component…

天体物理学 · 物理学 2009-09-15 Jeremiah P. Ostriker , Paul J. Steinhardt

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

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

Dark matter (comprising a quarter of the Universe) is usually assumed to be due to one and only one weakly interacting particle which is neutral and absolutely stable. We consider the possibility that there are several coexisting…

高能物理 - 唯象学 · 物理学 2007-12-03 Qing-Hong Cao , Ernest Ma , Jose Wudka , C. -P. Yuan

We study the formation and properties of dark neutron stars in a scenario where dark matter is made up of (heavy) dark baryons in a sequestered copy of the MSSM. This scenario naturally explains the coincidence of baryonic and dark matter…

高能物理 - 唯象学 · 物理学 2025-11-05 Jacob A. Litterer , João G. Rosa

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…

高能物理 - 唯象学 · 物理学 2009-09-25 V. Burdyuzha , O. Lalakulich , Yu. Ponomarev , G. Vereshkov

Adopting Dirac's brane variation prescription, the energy-momentum tensor of a brane gets supplemented by a geometrical (embedding originated) dark component. While the masslessness of the graviton is preserved, and the Newton force law is…

广义相对论与量子宇宙学 · 物理学 2010-02-17 Ilya Gurwich , Aharon Davidson

We may call "alien particles" those particles belonging to the matter/field content of a $d$-dimensional brane other than the $3$-brane (or stack of branes) sweeping the space-time in which we live. They can appear in our space-time at the…

综合物理 · 物理学 2016-11-15 M. Gasperini