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Spherical collapse predicts that a single value of the turnaround density (average matter density within the scale on which a structure detaches from the Hubble flow) characterizes all cosmic structures at the same redshift. It has been…

宇宙学与河外天体物理 · 物理学 2020-07-01 Vasiliki Pavlidou , Giorgos Korkidis , Theodore Tomaras , Dimitrios Tanoglidis

Constraints on dark matter from the first CMS and ATLAS SUSY searches are investigated. It is shown that within the minimal supergravity model, the early search for supersymmetry at the LHC has depleted a large portion of the signature…

高能物理 - 唯象学 · 物理学 2011-07-19 Sujeet Akula , Daniel Feldman , Zuowei Liu , Pran Nath , Gregory Peim

We derive constraints on cosmological parameters using the power spectrum of galaxy clustering measured from the final two-degree field galaxy redshift survey (2dFGRS) and a compilation of measurements of the temperature power spectrum and…

In this paper, we discuss a model-independent way to obtain the present dark matter density parameter ($\Omega_{\rm{c,0}}$) by combining gas mass fraction measurements in galaxy clusters ($f_{gas}$), type Ia supernovae (SNe Ia) observations…

宇宙学与河外天体物理 · 物理学 2019-12-04 R. F. L. Holanda , R. S. Gonçalves , J. E. Gonzales , J. S. Alcaniz

The cold dark matter fermions with mass MeV scale, pair produced inside the supernova SN1987A core, can freely stream away from the supernovae and hence contributes to its energy loss rate. Similar type of DM fermions(having similar kind of…

高能物理 - 唯象学 · 物理学 2018-10-25 Atanu Guha , Prasanta Kumar Das

The latest experimental results from the LHC and dark matter (DM) searches suggest that the parameter space allowed in supersymmetric theories is subject to strong reductions. These bounds are especially constraining for scenarios entailing…

高能物理 - 唯象学 · 物理学 2017-05-04 M. Peiro , S. Robles

The nature of dark matter (DM) remains unknown despite very precise knowledge of its abundance in the universe. An alternative to new elementary particles postulates DM as made of macroscopic compact halo objects (MACHO) such as black holes…

宇宙学与河外天体物理 · 物理学 2018-10-10 Miguel Zumalacarregui , Uros Seljak

We use observational data on the large scale structure (LSS) of the Universe measured over a wide range of scales from sub-galactic up to horizon scale and on the cosmic microwave background anisotropies to determine cosmological parameters…

天体物理学 · 物理学 2011-07-19 R. Durrer , B. Novosyadlyj

A cosmological model with total density close to critical (and flat geometry), dominated by dark matter and dark energy of unknown nature, and consistent with the basic predictions of the inflationary scenario is a very good fit to a…

天体物理学 · 物理学 2007-05-23 A. Balbi

The neutralino sector of the semi-constrained next-to-minimal supersymmetric standard model is explored under recent experimental constraints, with special attention to dark matter (DM) limits. The effects of the upper and lower bounds of…

高能物理 - 唯象学 · 物理学 2021-02-02 Elham Aldufeery , Maien Binjonaid

In unparticle dark matter (unmatter) models the equation of state of the unmatter is given by $p=\rho/(2d_U+1)$, where $d_U$ is the scaling factor. Unmatter with such equations of state would have a significant impact on the expansion…

天体物理学 · 物理学 2008-12-18 Yan Gong , Xuelei Chen

Supersymmetry offers a cold dark matter candidate, provided that lepton number is {\em not violated by an odd number of units}. On the other hand, lepton number violation by even (two) units gives us an attractive mechanism of neutrino mass…

高能物理 - 唯象学 · 物理学 2008-11-26 Biswarup Mukhopadhyaya , Soumitra SenGupta , Raghavendra Srikanth

The magnitude-redshift relation is one of the tools for a direct observational approach to cosmology. The discovery of high redshift Type Ia supernovae (SNIa) and their use as ``standard candles'' has resurrected interest in this approach.…

天体物理学 · 物理学 2008-11-26 Marie-Noëlle Célérier

The relic abundance of thermal dark matter particles is generally assumed to be inversely proportional to their annihilation rate, which is therefore constrained by the present matter density, <sigma v> ~ 10^{-26} Omega_{dm}^{-1} cm^3…

宇宙学与河外天体物理 · 物理学 2010-01-07 Leonid Chuzhoy

In the framework of an nonuniversal $U(1)'$ extension of the standard model, we propose an scalar candidate for cold dark matter which exhibits interactions with ordinary matter through Higgs and gauge bosons. Using limits from low energy…

高能物理 - 唯象学 · 物理学 2014-11-07 R. Martinez , J. Nisperuza , F. Ochoa , J. P. Rubio

We compare the first results on searches for supersymmetry with the Large Hadron Collider (LHC) to the current and near-term performance of experiments sensitive to neutralino dark matter. We limit our study to the particular slices of…

高能物理 - 唯象学 · 物理学 2011-08-08 Stefano Profumo

We consider a minimal extension of the Standard Model (SM), which leads to unification of the SM coupling constants, breaks electroweak symmetry dynamically by a new strongly coupled sector and leads to novel dark matter candidates. In this…

高能物理 - 唯象学 · 物理学 2015-06-16 Kimmo Kainulainen , Kimmo Tuominen , Jussi Virkajärvi

The recent WMAP data provide a rather restricted range of the Cold Dark Matter (CDM) density $ \Omega_{CDM} h^2 $ of unprecedented accuracy. We combine these new data along with data from BNL E821 experiment measuring $ {(g_{\mu}-2)}$, $…

高能物理 - 唯象学 · 物理学 2008-11-26 A. B. Lahanas , D. V. Nanopoulos

The sensitivity of the lightest supersymmetric particle relic density calculation to the variation of the cosmological expansion rate before nucleosynthesis is discussed. We show that such a modification, even extremely modest and with no…

高能物理 - 唯象学 · 物理学 2010-05-12 A. Arbey , F. Mahmoudi

In recent work, it has been argued that multi-TeV masses for scalar superpartners are not unnatural. Indeed, they appear to have significant phenomenological virtues. Here we explore the implications of such `focus point' supersymmetry for…

高能物理 - 唯象学 · 物理学 2009-09-25 Jonathan L. Feng , Konstantin T. Matchev , Frank Wilczek