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The fluctuations in the dark matter-baryon relative velocity field are imprinted as acoustic oscillations in the 21-cm power spectrum during cosmic dawn (CD). These velocity acoustic oscillations (VAOs) keep the imprints of the comoving…

宇宙学与河外天体物理 · 物理学 2023-02-08 Debanjan Sarkar , Ely D. Kovetz

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

We calculate the angular correlation function of galaxies in the Two Micron All Sky Survey. We minimize the possible contamination by stars, dust, seeing and sky brightness by studying their cross correlation with galaxy density, and…

天体物理学 · 物理学 2009-11-07 Ariyeh H. Maller , Daniel H. McIntosh , Neal Katz , Martin D. Weinberg

Baryon acoustic oscillations (BAO) are a powerful probe of the expansion history of the universe, which can tell us about the nature of dark energy. In order to accurately characterize the dark energy equation of state using BAO, we must…

宇宙学与河外天体物理 · 物理学 2015-06-23 Nuala McCullagh , Alexander S. Szalay

The baryon acoustic oscillation (BAO) experiment requires a sufficiently dense sampling of large-scale structure tracers with spectroscopic redshift, which is observationally expensive especially at high redshifts $z\simgt 1$. Here we…

宇宙学与河外天体物理 · 物理学 2015-06-15 Atsushi J. Nishizawa , Masamune Oguri , Masahiro Takada

Baryon Acoustic Oscillations (BAO) provide a robust standard ruler for observational cosmology, enabling precise constraints on the expansion history of the Universe. We present a weakly model-dependent measurement of the BAO angular scale…

宇宙学与河外天体物理 · 物理学 2025-06-11 U. Ribeiro , F. Avila , C. R. Bom , C. Franco , A. Cortesi , C. Mendes de Oliveira , A. Kanaan , T. Ribeiro , W. Schoenell , E. Telles , A. Bernui

This thesis presents the analysis of the clustering of galaxies in the 6dF Galaxy Survey (6dFGS). At large separation scales the baryon acoustic oscillation (BAO) signal is detected which allows to make an absolute distance measurement at…

宇宙学与河外天体物理 · 物理学 2013-03-15 Florian Beutler

The oscillation spectrum of pressure waves in stars can be determined by monitoring their luminosity. For rapidly rotating stars, the corresponding ray dynamics is mixed, with chaotic and regular zones in phase space. Our numerical…

太阳与恒星天体物理 · 物理学 2019-04-22 Benjamin Evano , Bertrand Georgeot , François Lignières

We construct cosmic void catalogues with the DIVE void finder upon SDSS BOSS DR12 and eBOSS DR16 galaxy samples with BAO reconstruction applied, and perform a joint BAO analysis using different types of galaxies and the corresponding voids.…

In this letter we describe a new method to use Baryon Acoustic Oscillations (BAO) to derive a constraint on the possible variation of the speed of light. The method relies on the fact that there is a simple relation between the angular…

宇宙学与河外天体物理 · 物理学 2015-03-18 Vincenzo Salzano , Mariusz P. Dabrowski , Ruth Lazkoz

Motivated by the recent proposal that one can obtain quasi-periodic oscillations (QPOs) by photon echoes manifesting as non-trivial features in the autocorrelation function (ACF), we study the ACFs of the light curves of three accreting…

高能天体物理现象 · 物理学 2015-05-19 K. Fukumura , C. R. Shrader , J. W. Dong , D. Kazanas

The Baryon Acoustic Oscillation (BAO) feature in the two-point correlation function (TPCF) of discrete tracers such as galaxies is an accurate standard ruler. The covariance matrix of the TPCF plays an important role in determining how the…

宇宙学与河外天体物理 · 物理学 2024-10-24 Jaemyoung Jason Lee , Farnik Nikakhtar , Aseem Paranjape , Ravi K. Sheth

Photometric data can be analyzed using the three-dimensional correlation function $\xi_{\rm p}$ to extract cosmological information via e.g., measurement of the Baryon Acoustic Oscillations (BAO). Previous studies modeled $\xi_{\rm p} $…

宇宙学与河外天体物理 · 物理学 2022-02-16 Kwan Chuen Chan , Ismael Ferrero , Santiago Avila , Ashley J. Ross , Martin Crocce , Enrique Gaztanaga

Gravitational non-linear evolution induces a shift in the position of the baryon acoustic oscillations (BAO) peak together with a damping and broadening of its shape that bias and degrades the accuracy with which the position of the peak…

宇宙学与河外天体物理 · 物理学 2017-09-12 Andrej Obuljen , Francisco Villaescusa-Navarro , Emanuele Castorina , Matteo Viel

In this work we examine the baryon acoustic oscillations (BAO) in 2D angular and redshift space $\{\theta, \Delta z\}$, with $\Delta z$ denoting the redshift difference between two given angular shells. We thus work in the context of…

宇宙学与河外天体物理 · 物理学 2025-12-22 Paula S. Ferreira , Carlos Hernández-Monteagudo , Ribamar R. R. Reis

In the present study, the axisymmetric natural oscillations of a liquid drop supported by a flat surface is investigated by direct numerical simulation. The liquid-gas interface is captured using a geometric volume-of-fluid (VOF) method. A…

流体动力学 · 物理学 2023-11-16 Jordan Sakakeeny , Yue Ling

We present measurements of the Baryon Acoustic Oscillation (BAO) scale in redshift-space using the clustering of quasars. We consider a sample of 147,000 quasars from the extended Baryon Oscillation Spectroscopic Survey (eBOSS) distributed…

We use hydrodynamic cosmological simulations in a (600 Mpc)^3 volume to study the observability of baryon acoustic oscillations (BAO) in the intergalactic medium as probed by Lyman alpha forest (LAF) absorption. The large scale separation…

宇宙学与河外天体物理 · 物理学 2015-05-13 Michael L. Norman , Pascal Paschos , Robert Harkness

We calculated spatial correlation functions of galaxies, $\xi(r)$, structure functions, $g(r)=1 +\xi(r)$, gradient functions, $\gamma(r)= d \log g(r)/ d \log r$, and fractal dimension functions, $D(r)= 3+\gamma(r)$, using dark matter…

宇宙学与河外天体物理 · 物理学 2020-08-12 J. Einasto , G. Hütsi , T. Kuutma , M. Einasto