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(Abridged) The 7-year WMAP data and improved astrophysical data rigorously test the standard cosmological model and its extensions. By combining WMAP with the latest distance measurements from BAO and H0 measurement, we determine the…

Based on almost 20 years of data collected by the high-resolution spectrometer SPI on board the International Gamma-Ray Astrophysics Laboratory (INTEGRAL) we present constraints on a decaying dark matter particle undergoing a decay into two…

高能天体物理现象 · 物理学 2023-02-15 S. Fischer , D. Malyshev , L. Ducci , A. Santangelo

The interaction between Dark Matter and Dark Energy has been proposed as a mechanism to alleviate the coincidence problem. We analyze the effect of the interaction on the evolution of the gravitational field and propose two new observables…

宇宙学与河外天体物理 · 物理学 2015-06-16 Xiao-Dong Xu , Bin Wang , Pengjie Zhang , Fernando Atrio-Barandela

We present constraints on cosmological parameters based on a sample of Sunyaev-Zel'dovich-selected galaxy clusters detected in a millimeter-wave survey by the Atacama Cosmology Telescope. The cluster sample used in this analysis consists of…

Thermal Sunyaev-Zel'dovich effect is one of the recent probes of cosmology and large scale structures. We update constraints on cosmological parameters from galaxy clusters observed by the Planck satellite in a first attempt to combine…

宇宙学与河外天体物理 · 物理学 2018-06-06 Laura Salvati , Marian Douspis , Nabila Aghanim

The Sunyaev-Zel'dovich (SZ) effect is a spectral distortion of the cosmic microwave background as observed through the hot plasma in galaxy clusters. This distortion is a decrement in the CMB intensity for lambda > 1.3 mm, an increment at…

We consider a late closed universe of which scale factor is a power function of time using observational data from combined WMAP5+BAO+SNIa dataset and WMAP5 dataset. The WMAP5 data give power-law exponent, $\alpha = 1.01$ agreeing with the…

宇宙学与河外天体物理 · 物理学 2012-10-30 Burin Gumjudpai , Kiattisak Thepsuriya

Dark Matter is essential for structure formation in the late Universe so it must be stable on cosmological time scales. But how stable exactly? Only assuming decays into relativistic particles, we report an otherwise model independent bound…

宇宙学与河外天体物理 · 物理学 2015-01-19 Benjamin Audren , Julien Lesgourgues , Gianpiero Mangano , Pasquale Dario Serpico , Thomas Tram

The Sunyaev-Zel'dovich (SZ) effect associated with pressure fluctuations of the large scale structure gas distribution will be probed with current and upcoming wide-field small angular scale cosmic microwave background experiments. We study…

天体物理学 · 物理学 2008-11-26 Asantha Cooray

We consistently include the effect of massive neutrinos in the thermal Sunyaev Zeldovich (SZ) power spectrum and cluster counts analyses, highlighting subtle dependencies on the total neutrino mass and data combination. In particular, we…

宇宙学与河外天体物理 · 物理学 2020-12-15 Boris Bolliet , Thejs Brinckmann , Jens Chluba , Julien Lesgourgues

We consider a decaying scalar dark matter (DM) with mass $m_\chi$ in the range 10 GeV - 10 TeV and vary the branching ratios of all possible two-body SM final states (excluding and including $\nu\bar{\nu}$) in the range $0\%-100\%$ to…

高能物理 - 唯象学 · 物理学 2022-09-07 Koushik Dutta , Avirup Ghosh , Arpan Kar , Biswarup Mukhopadhyaya

The Dark Ages and the Cosmic Dawn are an untapped well of information about the particle physics properties of dark matter, which may become accessible with future radio telescopes able to probe the 21-cm signal from atomic hydrogen. In…

宇宙学与河外天体物理 · 物理学 2026-04-22 Markus R. Mosbech , Cristina Benso , Felix Kahlhoefer

The Sunyaev Zel'dovich effect (SZ effect) is a complete probe of ionized baryons, the majority of which are likely hiding in the intergalactic medium. We ran a $512^3$ $\Lambda$CDM simulation using a moving mesh hydro code to compute the…

天体物理学 · 物理学 2009-11-07 Pengjie Zhang , Ue-Li Pen , Benjamin Wang

From observations at low and high redshifts, it is well known that the bulk of dark matter (DM) has to be stable or at least very long-lived. However, the possibility that a small fraction of DM is unstable or that all DM decays with a…

宇宙学与河外天体物理 · 物理学 2023-04-19 Jozef Bucko , Sambit K. Giri , Aurel Schneider

We present angular power spectra of the cosmic microwave background radiation anisotropy due to fluctuations of the Sunyaev-Zel'dovich (SZ) effect through clusters of galaxies. A contribution from the correlation among clusters is…

天体物理学 · 物理学 2009-10-31 Eiichiro Komatsu , Tetsu Kitayama

The latest Planck results on the power spectrum of the Compton-$y$ parameter are the most accurate probe of the thermal Sunyaev Zeldovich (tSZ) effect caused by resolved and un-resolved clusters of galaxies. On large angular scales, the…

宇宙学与河外天体物理 · 物理学 2018-06-14 Boris Bolliet

Since its original formulation the Sunyaev-Zeldovich (SZ) effect has been recognized as a ``powerful laboratory'' for our comprehension of physical processes in cosmic structures and to derive crucial information on some general properties…

天体物理学 · 物理学 2009-06-23 Carlo Burigana

The Sunyaev-Zel'dovich effect provides a useful probe of cosmology and structure formation in the Universe. Recent years have seen rapid progress in both quality and quantity of its measurements. In this review, we overview cosmological and…

宇宙学与河外天体物理 · 物理学 2014-07-02 Tetsu Kitayama