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相关论文: Branons as dark matter

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Generic extensions of the Standard Model that respect baryon and lepton numbers have accidentally stable particles. Typical examples are the lightest exotic neutral fermion, or "neutralino", and fields with non-trivial lepton and baryon…

高能物理 - 唯象学 · 物理学 2014-07-16 Luca Vecchi

We analyze the dark matter problem in the context of brane cosmology. We investigate the impact of the non-conventional brane cosmology on the relic abundance of non-relativistic stable particles in high and low reheating scenarios. We show…

高能物理 - 唯象学 · 物理学 2009-11-11 E. Abou El Dahab , S. Khalil

In a brane (domain wall) scenario with an infinite extra dimension and localized gravity, bulk fermions and scalars often have bound states with zero 4-dimensional mass. In this way massless matter residing on the brane may be obtained. We…

高能物理 - 理论 · 物理学 2009-07-09 S. L. Dubovsky , V. A. Rubakov , P. G. Tinyakov

The so called `cosmic coincidence' problem seems to suggest a coupling between dark energy and dark matter. A possibility could be given by dark matter particles with masses depending exponentially on the scalar field associated to dark…

高能物理 - 唯象学 · 物理学 2007-05-23 Massimo Pietroni

We summarize the main features of several dark matter candidates in extra-dimensional theories. In particular, we review Kaluza-Klein (KK) gravitons in universal extra dimensions and branons in brane-world models. KK gravitons are superWIMP…

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

Neutron Stars (NSs) are compact stellar objects that are stable solutions in General Relativity. Their internal structure is usually described using an equation of state that involves the presence of ordinary matter and its interactions.…

高能天体物理现象 · 物理学 2020-12-18 M. Ángeles Pérez-García , J. Silk

We propose a cosmological scenario based on the assumption that the Standard Model possesses a large number of copies. It is demonstrated that baryons in the hidden copies of the standard model can naturally account for the dark matter. The…

高能物理 - 理论 · 物理学 2009-08-11 Gia Dvali , Ignacy Sawicki , Alexander Vikman

The majority of the matter in the universe is still unidentified and under investigation by both direct and indirect means. Many experiments searching for the recoil of dark-matter particles off target nuclei in underground laboratories…

高能物理 - 唯象学 · 物理学 2015-10-28 Michael Klasen , Martin Pohl , Günter Sigl

According to the braneworld idea, ordinary matter is confined on a 3-dimensional space (brane) that is embedded in a higher-dimensional space-time where gravity propagates. In this work, after reviewing the limits coming from general…

广义相对论与量子宇宙学 · 物理学 2016-05-18 R. Gonzalez Felipe , D. Manreza Paret , A. Perez Martinez

We discuss observational constrains coming from supernovae Ia imposed on the behaviour of the Randall-Sundrum models. In the case of dust matter on the brane, the difference between the best-fit Perlmutter model with a $\Lambda$-term and…

天体物理学 · 物理学 2009-11-10 Wlodzimierz Godlowski , Marek Szydlowski

The fraction of matter that is in the form of baryons or dark matter could have spatial fluctuations in the form of baryon-dark matter isocurvature fluctuations. We use big bang nucleosynthesis calculations compared with observed light…

宇宙学与河外天体物理 · 物理学 2015-05-13 Gilbert P. Holder , Kenneth M. Nollett , Alexander van Engelen

The braneworld description of our universe entails a large extra dimension and a fundamental scale of gravity that might be lower by several orders of magnitude compared to the Planck scale. An interesting consequence of the braneworld…

天体物理学 · 物理学 2009-11-10 A. S. Majumdar , N. Mukherjee

We discuss observational constrains coming from supernovae Ia \cite{Perlmutter99} imposed on the behaviour of the Randall-Sundrum models. In the case of dust matter on the brane, the difference between the best-fit general relativistic…

天体物理学 · 物理学 2015-06-24 Mariusz P. Dabrowski , Wlodzimierz Godlowski , Marek Szydlowski

Progress in observational cosmology over the past five years has established that the Universe is dominated dynamically by dark matter and dark energy. Both these new and apparently independent forms of matter-energy have properties that…

天体物理学 · 物理学 2009-11-10 J. M. Overduin , P. S. Wesson

In a model where a multiverse wavefunction explores a multitude of vacua with different symmetries and parameters, properties of universes closely related to ours can be understood by examining the consequences of small departures of…

天体物理学 · 物理学 2007-05-23 Craig J. Hogan

Neutron stars contain a significant number of stable muons due to the large chemical potential and degenerate electrons. This makes them the unique vessel to capture muonphilic dark matter, which does not interact with other astrophysical…

高能物理 - 唯象学 · 物理学 2019-09-04 Raghuveer Garani , Julian Heeck

A number of observed phenomena in high energy physics and cosmology lack their resolution within the Standard Model of particle physics. These puzzles include neutrino oscillations, baryon asymmetry of the universe and existence of dark…

高能物理 - 唯象学 · 物理学 2008-12-18 Mikhail Shaposhnikov

Astronomical and cosmological observations of the past 80 years build solid evidence that atomic matter makes up only a small fraction of the matter in the universe. The dominant fraction does not interact with electromagnetic radiation,…

宇宙学与河外天体物理 · 物理学 2015-05-27 Wolfgang Rau

In the context of the standard model of particle physics, there is a definite upper limit to the density of stable compact stars. However, if a more fundamental level of elementary particles exists, in the form of preons, stability may be…

天体物理学 · 物理学 2007-05-23 J. Hansson , F. Sandin