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The improving sensitivity of measurements of the kinetic Sunyaev-Zel'dovich (SZ) effect opens a new window into the thermodynamic properties of the baryons in halos. We propose a methodology to constrain these thermodynamic properties by…

宇宙学与河外天体物理 · 物理学 2017-12-13 Nicholas Battaglia , Simone Ferraro , Emmanuel Schaan , David Spergel

The cosmic velocity field is an unbiased probe of the total matter distribution but is challenging to measure directly at intermediate and high redshifts. The large-scale velocity field imprints a signal in the cosmic microwave background…

宇宙学与河外天体物理 · 物理学 2024-11-20 Alex Laguë , Mathew S. Madhavacheril , Kendrick M. Smith , Simone Ferraro , Emmanuel Schaan

The kinetic Sunyaev Zel'dovich (kSZ) effect, cosmic microwave background (CMB) anisotropies induced by scattering from free electrons in bulk motion, is a primary target of future CMB experiments. Measurements of the kSZ effect have the…

宇宙学与河外天体物理 · 物理学 2018-09-12 Juan I. Cayuso , Matthew C. Johnson , James B. Mertens

We develop an estimator to extract the mean radial velocity profile of cosmic voids via the kinematic Sunyaev-Zeldovich effect of pairs of galaxies surrounding them. The estimator is tested with simulated pure kSZ map and void catalogue…

宇宙学与河外天体物理 · 物理学 2020-02-06 Yi-Chao Li , Yin-Zhe Ma , Seshadri Nadathur

Recent reconstructions of the large-scale cosmological velocity field with kinetic Sunyaev Zeldovich (kSZ) tomography have returned an amplitude that is low with respect to the halo model prediction, captured by the kSZ velocity…

宇宙学与河外天体物理 · 物理学 2025-10-31 Avery J. Tishue , Charuhas Shiveshwarkar , Gilbert Holder

We study the kinematic Sunyaev-Zel'dovich (kSZ) effect in a Lem\^itre-Tolman-Bondi (LTB) universe model whose distance-redshift relation agrees with that of the concordance $\Lambda$CDM model at redshifts $z\lesssim2$. This LTB universe…

宇宙学与河外天体物理 · 物理学 2015-05-19 Chul-Moon Yoo , Ken-ichi Nakao , Misao Sasaki

The kinematic Sunyaev-Zel'dovich (kSZ) signal is a powerful probe of the cosmic baryon distribution. The kSZ signal is proportional to the integrated free electron momentum rather than the electron pressure (which sources the thermal SZ…

宇宙学与河外天体物理 · 物理学 2017-01-02 Simone Ferraro , J. Colin Hill , Nick Battaglia , Jia Liu , David N. Spergel

Measurements of secondary cosmic microwave background (CMB) anisotropies, such as the Sunyaev-Zel'dovich (SZ) effect, will enable new tests of neutrino and dark sector properties. The kinetic SZ (kSZ) effect is produced by cosmological…

宇宙学与河外天体物理 · 物理学 2023-03-07 Gerrit S. Farren , Daniel Grin , Andrew H. Jaffe , Renée Hložek , David J. E. Marsh

The kinetic Sunyaev Zel'dovich (kSZ) effect is a blackbody cosmic microwave background (CMB) temperature anisotropy induced by Thomson scattering off free electrons in bulk motion with respect to the CMB rest frame. The statistically…

宇宙学与河外天体物理 · 物理学 2026-05-11 Richard Bloch , Matthew C. Johnson

We present the mean pairwise momentum of clusters, as observed through the kinematic Sunvaev-Zel'dovich (kSZ) effect, as a novel probe of massive neutrinos. We find that kSZ measurements with current and upcoming surveys will provide…

宇宙学与河外天体物理 · 物理学 2015-09-09 Eva-Maria Mueller , Francesco de Bernardis , Rachel Bean , Michael D. Niemack

We propose a novel technique to separate the late-time, post-reionization component of the kinetic Sunyaev-Zeldovich (kSZ) effect from the contribution to it from a (poorly understood and probably patchy) reionization history. The kSZ…

宇宙学与河外天体物理 · 物理学 2017-02-01 D. Munshi , I. T. Iliev , K. L. Dixon , P. Coles

The gas density profile around galaxies, shaped by feedback and affecting the galaxy lensing signal, is imprinted on the cosmic microwave background (CMB) by the kinematic Sunyaev-Zel'dovich effect (kSZ). We precisely measure this effect…

We develop an optimization-based maximum likelihood approach to analyze the cross-correlation of the Cosmic Microwave Background (CMB) and large-scale structure induced by the kinetic Sunyaev-Zeldovich (kSZ) effect. Our main goal is to…

宇宙学与河外天体物理 · 物理学 2024-03-01 Yurii Kvasiuk , Moritz Münchmeyer

We develop and test a new statistical method to measure the kinematic Sunyaev-Zel'dovich (kSZ) effect. A sample of independently detected clusters is combined with the cosmic flow field predicted from a galaxy redshift survey in order to…

宇宙学与河外天体物理 · 物理学 2014-11-11 Ming Li , Raul E. Angulo , Simon D. M. White , Jens Jasche

The kinematic Sunyaev-Zel'dovich (kSZ) effect in the cosmic microwave background (CMB) is a powerful probe of gas physics and large-scale structure (LSS) in our universe. We consider the "projected-field" kSZ estimator, which involves…

宇宙学与河外天体物理 · 物理学 2026-05-21 Michael Jacob Rodriguez , Aleksandra Kusiak , Shivam Pandey , J. Colin Hill

The kinematic and thermal Sunyaev-Zel'dovich (kSZ and tSZ) effects probe the abundance and thermodynamics of ionized gas in galaxies and clusters. We present a new hybrid estimator to measure the kSZ effect by combining cosmic microwave…

In this review we present a comprehensive discussion of peculiar velocity field measured recently on very large scales with a novel method using X-ray galaxy clusters as tracers. The measurement is based on the kinematic component of the…

宇宙学与河外天体物理 · 物理学 2012-02-06 A. Kashlinsky , F. Atrio-Barandela , H. Ebeling

We present results on the thermal and kinetic Sunyaev-Zel'dovich (SZ) effects from a sequence of high resolution hydrodynamic simulations of structure formation, including cooling, feedback and metal injection. These simulations represent a…

天体物理学 · 物理学 2008-11-26 Martin White , Lars Hernquist , Volker Springel

Compton scattering of the cosmic microwave background (CMB) from hot ionized gas produces a range of effects, and the leading order effects are the kinetic and thermal Sunyaev Zel'dovich (kSZ and tSZ) effects. In the near future, CMB…

宇宙学与河外天体物理 · 物理学 2020-09-16 William R. Coulton , Atsuhisa Ota , Alexander van Engelen

We report the direct detection of the kinetic Sunyaev-Zel'dovich (kSZ) effect in galaxy clusters with a 3.5 sigma significance level. The measurement was performed by stacking the Planck map at 217 GHz at the positions of galaxy clusters…

宇宙学与河外天体物理 · 物理学 2021-01-26 Hideki Tanimura , Saleem Zaroubi , Nabila Aghanim