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We explain the effect of dark matter (flat rotation curve) using modified gravitational dynamics. We investigate in this context a low energy limit of generalized general relativity with a nonlinear Lagrangian ${\cal L}\propto R^n$, where…

天体物理学 · 物理学 2008-11-26 Andrzej Borowiec , Wlodzimierz Godlowski , Marek Szydlowski

The field equations in $f(R)$ gravity derived from the Palatini variational principle and formulated in the Einstein conformal frame yield a cosmological term which varies with time. Moreover, they break the conservation of the…

广义相对论与量子宇宙学 · 物理学 2007-05-23 Nikodem J. Poplawski

f(R)-theories of gravity are reviewed in the framework of the matter-antimatter asymmetry in the Universe. The asymmetry is generated by the gravitational coupling of heavy (Majorana) neutrinos with the Ricci scalar curvature. In order that…

高能物理 - 唯象学 · 物理学 2015-06-23 G. Lambiase , S. Mohanty , L. Pizza

If dark matter self-annihilates then it may produce an observable signal when its density is high. The details depend on the intrinsic properties of dark matter and how it clusters in space. For example, the density profile of some dark…

高能天体物理现象 · 物理学 2015-06-03 Benjamin C. Bromley

The linearized Einstein theory in the approximately flat time-space is modified accounting for a massive graviton as a dark matter in the universe. On the basis of magnetic-type Maxwell- Proca -Vlasov equations, the interactions of the…

等离子体物理 · 物理学 2013-06-05 Xiao-qing Li

We investigate a two-component model for gravitational lenses, i.e., the fermion-fermion star as a dark matter self-gravitating system made from two kinds of fermions with different masses. We calculate the deflection angles varying from…

广义相对论与量子宇宙学 · 物理学 2009-10-31 Ke-Jian Jin , Yuan-Zhong Zhang , Zong-Hong Zhu

The Thomas-Fermi model at finite temperature is extended to describe a system of self-gravitating weakly interacting massive fermions in a general-relativistic framework. By cooling a nondegenerate gas of weakly interacting massive fermions…

高能物理 - 唯象学 · 物理学 2011-09-13 Neven Bilic , Raoul D. Viollier

Explanations of the late-time cosmic acceleration within the framework of general relativity are plagued by difficulties. General relativistic models are mostly based on a dark energy field with fine-tuned, unnatural properties. There is a…

天体物理学 · 物理学 2010-04-22 Ruth Durrer , Roy Maartens

We consider a simple class of models in which the dark matter, X, is coupled to a new gauge boson, phi, with a relatively low mass (m_phi \sim 100 MeV-3 GeV). Neither the dark matter nor the new gauge boson have tree-level couplings to the…

高能物理 - 唯象学 · 物理学 2013-05-30 Dan Hooper , Neal Weiner , Wei Xue

It is proposed that an ultra-light fermionic species, dubbed cosmic magnino has condensed into a ferromagnetic state in the Universe. The extended structure of domain walls associated with this ferromagnetism accounts for the observed Dark…

宇宙学与河外天体物理 · 物理学 2011-02-15 Urjit A. Yajnik

We discuss the possibility that suitable modifications of gravity could account for some amount of the radiation we observe today, in addition to the possibility of explaining the present speed up of the universe. We start introducing and…

广义相对论与量子宇宙学 · 物理学 2015-12-02 Joao Morais , Mariam Bouhmadi-Lopez , Salvatore Capozziello

In the first part of this note, we observe that a non-Riemannian piece in the affine connection (a "dark connection") leads to an algebraically determined, conserved, symmetric 2-tensor in the Einstein field equations that is a natural dark…

宇宙学与河外天体物理 · 物理学 2018-09-24 Ranit Das , Chethan Krishnan

Dark matter, one of the fundamental components of the universe, has remained mysterious in modern cosmology and particle physics, and hence, this field is of utmost importance at present moment. One of the foundational questions in this…

广义相对论与量子宇宙学 · 物理学 2025-02-04 Jaume de Haro , Supriya Pan

The dynamics of a self-gravitating cold Fermi gas is described using the analogy with an interacting self-gravitating Bose condensate having the same Thomas-Fermi limit. The dissipationless formation of a heavy neutrino star through…

天体物理学 · 物理学 2009-11-06 Neven Bilic , Robert J. Lindebaum , Gary B. Tupper , Raoul D. Viollier

This chapter aims to present an introduction to current research on the nature of the cosmological dark matter and the origin of galaxies and large scale structure within the standard theoretical framework: gravitational collapse of…

天体物理学 · 物理学 2008-02-03 Joel R. Primack

Dynamical mass discrepancies in galaxies have two possible explanations: the existence of large amounts of dark matter or the breakdown of Newtonian gravity. True dark matter halos of galaxies could differ in several respects from apparent…

天体物理学 · 物理学 2007-05-23 J. A. Sellwood , A. Kosowsky

Modified gravity, known as $f(R)$ gravity, has presently been applied to Cosmology as a realistic alternative to dark energy. For this kind of gravity the expansion of the Universe may accelerate while containing only baryonic and cold dark…

宇宙学与河外天体物理 · 物理学 2012-05-01 N. Pires , J. Santos , J. S. Alcaniz

We review various modified gravities considered as gravitational alternative for dark energy. Specifically, we consider the versions of $f(R)$, $f(G)$ or $f(R,G)$ gravity, model with non-linear gravitational coupling or string-inspired…

高能物理 - 理论 · 物理学 2009-09-17 S. Nojiri , S. D. Odintsov

Motivated by the fact that, so far, the whole body of evidence for dark matter is of gravitational origin, we study the decays of dark matter into Standard Model particles mediated by gravity portals, i.e., through nonminimal gravitational…

高能物理 - 唯象学 · 物理学 2017-03-14 Oscar Catà , Alejandro Ibarra , Sebastian Ingenhütt

We argue that the effect of cold dark matter in the cosmological setup can be explained by the coupling between the baryonic matter particles in terms of the long-range force having a graviton mass $m_g$ via the Yukawa gravitational…

广义相对论与量子宇宙学 · 物理学 2024-08-22 Kimet Jusufi , Genly Leon , Alfredo D. Millano