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相关论文: Dark Matter Superfluidity

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Modified gravity models often contain modes that couple to normal matter and propagate with slightly less than the speed of light. High-energy cosmic rays then lose energy due to Cherenkov radiation, which constrains such models. This is…

广义相对论与量子宇宙学 · 物理学 2022-09-14 Tobias Mistele

We propose a connection between global physics and local galactic dynamics via quantum gravity. The salient features of cold dark matter (CDM) and modified Newtonian dynamics (MOND) are combined into a unified scheme by introducing the…

广义相对论与量子宇宙学 · 物理学 2015-05-28 Chiu Man Ho , Djordje Minic , Y. Jack Ng

Neutron stars (NSs) provide a unique laboratory to probe dark matter (DM) through its gravitational imprint on stellar evolution. We use a two-fluid framework with non-annihilating, asymmetric DM, both fermionic and bosonic, that interacts…

Recently, a new form of dark matter has been suggested to naturally reproduce the empirically successful aspects of Milgrom's law in galaxies. The dark matter particle candidates are axion-like, with masses of order eV and strong…

宇宙学与河外天体物理 · 物理学 2018-09-19 Lasha Berezhiani , Benoit Famaey , Justin Khoury

Warm dark matter (WDM) is an intriguing model of structure formation from the point of view of both cosmology and particle physics. We consider a one-parameter family of WDM models. The linear power spectra for these models is calculated…

天体物理学 · 物理学 2010-11-30 Stephane Colombi , Scott Dodelson , Lawrence M. Widrow

Cold Dark Matter (CDM) has become the standard modern theory of cosmological structure formation. Its predictions appear to be in good agreement with data on large scales, and it naturally accounts for many properties of galaxies. But…

天体物理学 · 物理学 2009-11-07 Joel R. Primack

We derive the MOND cosmology which is uniquely corresponding to the original MOND at galaxy scales via entropic gravity method. It inherits the key merit of MOND, that is, it reduces the baryonic matter and non-baryonic dark matter into…

广义相对论与量子宇宙学 · 物理学 2012-07-12 Hongsheng Zhang , Xin-Zhou Li

We present detailed semi-analytical models for the formation of disk galaxies both in a Universe dominated by dark matter (DM), and in one for which the force law is given by modified Newtonian dynamics (MOND). We tune the models to fit the…

天体物理学 · 物理学 2009-10-31 Frank C. van den Bosch , Julianne J. Dalcanton

We consider a supersymmetric model of dark energy coupled to cold dark matter: the supersymmetron. In the absence of cold dark matter, the supersymmetron converges to a supersymmetric minimum with a vanishing cosmological constant. When…

高能物理 - 唯象学 · 物理学 2015-05-30 Philippe Brax , Anne-Christine Davis

Cold Dark Matter (CDM) has become the standard modern theory of cosmological structure formation. Its predictions appear to be in good agreement with data on large scales, and it naturally accounts for many properties of galaxies. But…

天体物理学 · 物理学 2007-05-23 Joel R. Primack

Unified dark matter models are appealing in that they describe the dark sector in terms of a single component. They however face problems when attempting to account for structure formation: in the linear regime, density fluctuations can…

宇宙学与河外天体物理 · 物理学 2015-09-16 Amr El-Zant

Currently, a large amount of data implies that the matter constituents of the cosmological dark sector might be collisional. An attractive feature of such a possibility is that, it can reconcile dark matter (DM) and dark energy (DE) in…

宇宙学与河外天体物理 · 物理学 2015-03-25 K. Kleidis , N. K. Spyrou

In the very last years, cosmological models where the properties of the dark components of the Universe - dark matter and dark energy - are accounted for by a single "dark fluid" have drawn increasing attention and interest. Amongst many…

宇宙学与河外天体物理 · 物理学 2012-04-02 Stefano Camera , Carmelita Carbone , Lauro Moscardini

We discuss a comparison of models for the formation of disk galaxies both in a Universe dominated by cold dark matter (CDM) and one in which the force law is given by modified Newtonian dynamics (MOND). Our main aim is to address the claim…

天体物理学 · 物理学 2007-05-23 Frank C. van den Bosch , Julianne J. Dalcanton

The old dream of integrating into one the study of micro and macrocosmos is now a reality. Cosmology, astrophysics, and particle physics intersect in a scenario (but still not a theory) of cosmic structure formation and evolution called…

天体物理学 · 物理学 2015-06-24 V. Avila-Reese

We develop a perturbative model to describe large-scale structure in cosmologies where dark matter consists of a mixture of cold (CDM) and warm (WDM) components. In such mixed dark matter (MDM) scenarios, even a subdominant warm component…

宇宙学与河外天体物理 · 物理学 2025-09-11 Şafak Çelik , Fabian Schmidt

Modern astronomical data on galaxy and cosmological scales have revealed powerfully the existence of certain dark sectors of fundamental physics, i.e., existence of particles and fields outside the standard models and inaccessible by…

天体物理学 · 物理学 2008-12-18 HongSheng Zhao

I describe the MOND paradigm, which posits a departure from standard physics below a certain acceleration scale. This acceleration as deduced from the dynamics in galaxies is found mysteriously to agree with the cosmic acceleration scales…

宇宙学与河外天体物理 · 物理学 2010-10-11 Mordehai Milgrom

There are many hot discussions in the literature about two competing paradigms in galactic and extra-galactic astronomy and cosmology, namely the Dark Matter and the Modified Newtonian Dynamics (MOND). It is very difficult to challenge MOND…

宇宙学与河外天体物理 · 物理学 2014-05-27 Alexey Golovnev , Natalia Masalaeva

We consider the history of the universe from a possible big bang or a bounce into a late period of a unified interacting dark energy - dark matter model. The model is based on the Two Measures Theories (T.M.T.) which introduces a metric…

广义相对论与量子宇宙学 · 物理学 2018-07-30 David Benisty , Eduardo I. Guendelman