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We investigate the effect of supersonic relative velocities between baryons and dark matter, recently shown to arise generically at high redshift, on baryonic acoustic oscillation (BAO) measurements at low redshift. The amplitude of the…

宇宙学与河外天体物理 · 物理学 2015-05-28 Jaiyul Yoo , Neal Dalal , Uros Seljak

The baryon acoustic oscillations (BAO) prior to recombination should be imprinted onto the 21cm emission background from the epoch of reionization through the underlying density perturbations. Using an analytical approach for both matter…

天体物理学 · 物理学 2009-11-13 Xiao-Chun Mao , Xiang-Ping Wu

The baryon-acoustic oscillation (BAO) feature in the Lyman-$\alpha$ forest is one of the key probes of the cosmic expansion rate at redshifts z~2.5, well before dark energy is believed to have become dynamically significant. A key advantage…

宇宙学与河外天体物理 · 物理学 2017-12-27 Christopher M. Hirata

In this review we summarize the effect of relative supersonic velocities between gas and dark matter created right after recombination on astrophysics and cosmology. The relative velocities formally introduce a second order effect on the…

宇宙学与河外天体物理 · 物理学 2014-07-22 Anastasia Fialkov

We examine the impact of baryon-dark matter relative velocities on intergalactic small-scale structure and the 21 cm signal during reionization. Streaming velocities reduced clumping in the intergalactic medium (IGM) on mass scales of $\sim…

宇宙学与河外天体物理 · 物理学 2020-08-18 Christopher Cain , Anson D'Aloisio , Vid Iršič , Matthew McQuinn , Hy Trac

We investigate the suppression of the baryon density fluctuations compared to the dark matter in the linear regime. Previous calculations predict that the suppression occurs up to a characteristic mass scale of ~ 1,000,000 solar masses,…

天体物理学 · 物理学 2008-11-26 Smadar Naoz , Rennan Barkana

Studies of the formation of the first stars have established that they formed in small halos of $\sim 10^5 - 10^6 M_{\odot}$ via molecular hydrogen cooling. Since a low level of ultraviolet radiation from stars suffices to dissociate…

宇宙学与河外天体物理 · 物理学 2016-04-06 Aviad Cohen , Anastasia Fialkov , Rennan Barkana

The relative velocity between baryons and dark matter in the early Universe can suppress the formation of small-scale baryonic structure and leave an imprint on the baryon acoustic oscillation (BAO) scale at low redshifts after…

宇宙学与河外天体物理 · 物理学 2022-03-30 Heyang Long , Jahmour J. Givans , Christopher M. Hirata

Recently the initial supersonic relative velocity between the dark matter and baryons was shown to have an important effect on galaxy formation at high redshift. We study the impact of this relative motion on the distribution of the…

宇宙学与河外天体物理 · 物理学 2015-05-30 Anastasia Fialkov , Rennan Barkana , Dmitriy Tseliakhovich , Christopher M. Hirata

Future dark energy experiments will require better and more accurate theoretical predictions for the baryonic acoustic oscillations (BAO) signature in the spectrum of cosmological perturbations. Here, we use large N-body simulations of the…

We study the effect of the supersonic relative velocity between dark matter and baryons on large-scale galaxy clustering and derive the constraint on the relative velocity bias parameter from the Baryonic Oscillation Spectroscopic Survey…

宇宙学与河外天体物理 · 物理学 2015-06-16 Jaiyul Yoo , Uros Seljak

Recently, Tseliakhovich and Hirata (2010) showed that during the cosmic Dark Ages the baryons were typically moving supersonically with respect to the dark matter with a spatially variable Mach number. Such supersonic motion may source…

宇宙学与河外天体物理 · 物理学 2015-06-04 Matthew McQuinn , Ryan M. O'Leary

It has recently been suggested that the power spectrum of redshifted 21cm fluctuations could be used to measure the scale of baryonic acoustic oscillations (BAOs) during the reionisation era. The resulting measurements are potentially as…

天体物理学 · 物理学 2014-11-18 Kirsty J. Rhook , Paul M. Geil , J. Stuart B. Wyithe

The expansion of the universe appears to be accelerating, and the mysterious anti-gravity agent of this acceleration has been called ``dark energy''. To measure the dynamics of dark energy, Baryon Acoustic Oscillations (BAO) can be used.…

天体物理学 · 物理学 2008-11-26 Tzu-Ching Chang , Ue-Li Pen , Jeffrey B. Peterson , Patrick McDonald

An acoustic oscillation of the primeval photon-baryon fluid around the decoupling time imprints a characteristic scale in the galaxy distribution today, known as the baryon acoustic oscillation (BAO) scale. Several on-going and/or future…

Baryon acoustic oscillation (BAO) is a powerful probe on the expansion of the universe, shedding light on elusive dark energy and gravity at cosmological scales. BAO measurements through biased tracers of the underlying matter density…

天体物理学 · 物理学 2008-02-19 Pengjie Zhang

We measure the halo power spectrum in redshift space from cosmological N-body simulations, and test the analytical models of redshift distortions particularly focusing on the scales of baryon acoustic oscillations (BAOs). Remarkably, the…

宇宙学与河外天体物理 · 物理学 2011-09-08 Takahiro Nishimichi , Atsushi Taruya

New statistical method is proposed to coherently combine Baryon Acoustic Oscillation statistics (BAO) and peculiar velocity measurements exploiting decomposed density-density and velocity-velocity spectra in real space from the observed…

宇宙学与河外天体物理 · 物理学 2011-06-07 Yong-Seon Song

The large-scale clustering of galaxies encodes both geometric and dynamical information about the Universe. The Baryon Acoustic Oscillations (BAO) phenomenon provides a standard ruler that constrains the cosmic expansion history, while…

宇宙学与河外天体物理 · 物理学 2026-05-04 C. Franco , H. M. Courtois , A. Bernui

At the time of recombination, baryons and photons decoupled and the sound speed in the baryonic fluid dropped from relativistic to the thermal velocities of the hydrogen atoms. This is less than the relative velocities of baryons and dark…

宇宙学与河外天体物理 · 物理学 2015-03-17 Dmitriy Tseliakhovich , Christopher Hirata
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