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相关论文: Calculation of Dark Matter as a Feature of Space-T…

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In this paper we combine high resolution N-body simulations with a semi analytical model of galaxy formation to study the effects of a possible Warm Dark Matter (WDM) component on the observable properties of galaxies. We compare three WDM…

宇宙学与河外天体物理 · 物理学 2015-06-05 Xi Kang , Andrea V. Macciò , Aaron A. Dutton

Two forms are suggested for the energy-momentum source term associated with an aggregate of dark matter (with the properties described in Paper I). Both have large pressure-like components which dominate the density terms. Using one form a…

广义相对论与量子宇宙学 · 物理学 2020-01-20 H. L. Helfer

The observed excess of gravitational forces in galaxies and galactic clusters is usually referred as the existence of "dark matter particles" of unknown origin. An alternative explanation of the dark matter effect is presented here by…

宇宙学与河外天体物理 · 物理学 2011-10-04 Arkady Z. Dolginov

The cold dark matter paradigm has been posited as the standard explanation for the non-Keplerian behavior of galaxy rotation curves, where for galaxies satisfying the Tully-Fisher relation, the mass of the dark matter halo from a large…

广义相对论与量子宇宙学 · 物理学 2021-09-08 Godwill Mbiti Kanyolo , Titus Masese

We use a semianalytical approach and a CDM cosmological model to study the gravitational collapse and virialization, the structure, as well as the global and statistical properties of isolated dark matter galactic halos which emerge from…

天体物理学 · 物理学 2010-04-06 V. Avila-Reese , C. Firmani , X. Hernández

We continue the study of the tensor-four-scalars theory which is a modification of general relativity. We include normal matter by applying the displace, cut, and reflect method to our previous vacuum solutions with dark halo. The resulting…

广义相对论与量子宇宙学 · 物理学 2012-05-22 Günter Scharf

The distributions of normal matter and of dark matter in the Galaxy are coupled to each other as they both move in the common gravitational potential. In order to fully exploit this interplay and to derive the various properties of dark…

星系天体物理 · 物理学 2013-12-16 Benjamin Burch , Ramanath Cowsik

Rotation curves of spiral galaxies \emph{i}) fall off much less steeply than the Keplerian curves do, and \emph{ii}) have asymptotic speeds almost proportional to the fourth root of the mass of the galaxy, the Tully-Fisher relation. These…

广义相对论与量子宇宙学 · 物理学 2010-11-02 Y. Sobouti , A. Hasani Zonoozi , H. Haghi

We combine observed properties of galaxies as the core density and radius with the theoretical linear evolution of density fluctuations computed from first principles since the end of inflation till today. The halo radius r_0 is computed in…

宇宙学与河外天体物理 · 物理学 2015-05-18 H. J. de Vega , P. Salucci , N. G. Sanchez

We describe the motion of a particle in a central field in an expanding universe. Use is made of a double expansion in 1/c and 1/T, where c and T are the speed of light and the Hubble time. In the lowest approximation the fourth power of…

天体物理学 · 物理学 2007-05-23 Moshe Carmeli

Dark matter, believed to be present in many galaxies, is interpreted as a hydrodynamical system in interaction with the gravitational field and with nothing else. The gravitational field of our Galaxy can be inferred from observation of…

广义相对论与量子宇宙学 · 物理学 2012-04-11 Christian Fronsdal , Thomas J. Wilcox

We numerically explore on galaxy scales the Dipolar dark matter (DM) model based on the concept of gravitational polarization. This DM model has been proposed as a natural way to reproduce observed tight galactic scaling relations such as…

宇宙学与河外天体物理 · 物理学 2022-10-05 Clément Stahl , Benoit Famaey , Guillaume Thomas , Yohan Dubois , Rodrigo Ibata

[abridged] We explore the possibility that the dark matter (DM) component in galaxies may originate fractional gravity. In such a framework, the standard law of inertia continues to hold, but the gravitational potential associated to a…

星系天体物理 · 物理学 2023-06-07 Francesco Benetti , Andrea Lapi , Giovanni Gandolfi , Paolo Salucci , Luigi Danese

Observations show that for disk galaxies the fourth power of the circular velocity of stars around the core of the galaxy is proportional to the luminosity L. This is known as the Tully-Fisher law. Since L is proportional to the mass M of…

天体物理学 · 物理学 2007-05-23 Silvia Behar , Moshe Carmeli

Cosmological simulations of galaxy formation predict a universal form for the mass profile of dark matter (DM) halos from cluster to galaxy scales. Remarkably few interesting constraints exist, however, on DM halos in early-type galaxies.…

We investigate the viability of a simple dark matter (DM) model consisting of a single fermion in the context of galactic dynamics. We use a consistent approach that does not presume a particular DM density profile but instead requires that…

星系天体物理 · 物理学 2019-10-16 K. Pal , L. V. Sales , J. Wudka

Motivated by results implying that the constituents of dark matter (DM) might be collisional, we consider a cosmological (toy-) model, in which the DM itself possesses some sort of thermodynamic properties. In this case, not only can the…

广义相对论与量子宇宙学 · 物理学 2015-03-19 Kostas Kleidis , Nicholas K. Spyrou

It is shown that the cosmological constant links the roots both of General Relativity and Newtonian gravity via the general function satisfying Newton's theorem according to which the gravitating sphere acts as a point mass situated in its…

广义相对论与量子宇宙学 · 物理学 2019-01-10 V. G. Gurzadyan

Phenomena currently attributed to Dark Energy (DE) and Dark Matter (DM) are merely a result of the interplay between gravitational energy density, generated by the contraction of space by matter, and the energy density of the Cosmological…

天体物理学 · 物理学 2008-12-25 Shlomo Barak , Elia M Leibowitz

In this study, we investigate a scenario that dark matter (DM) has only gravitational interaction. In the framework of effective field theory of gravity, we find that DM is still stable at tree level even if there is no symmetry to protect…

高能物理 - 唯象学 · 物理学 2016-06-07 Yong Tang , Yue-Liang Wu
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