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相关论文: Probing bulk flow with nearby SNe Ia data

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The question of the transition to global isotropy from our anisotropic local Universe is studied using the Union 2 catalogue of Type Ia supernovae (SNe Ia). We construct a "residual" statistic sensitive to systematic shifts in their…

宇宙学与河外天体物理 · 物理学 2015-03-17 Jacques Colin , Roya Mohayaee , Subir Sarkar , Arman Shafieloo

The use of methods that investigate the value of the Hubble constant H$_0$ in different patches (60 $ or 90$^ size) across the sky to probe the statistical isotropy of the Universe using large SNe Ia databases has led to contradictory…

宇宙学与河外天体物理 · 物理学 2026-05-19 Antonio Quintana-Estellés , Pilar Ruiz-Lapuente

Observations reveal a `bulk flow' in the local Universe which is faster and extends to much larger scales than is expected around a typical observer in the standard $\Lambda$CDM cosmology. This is expected to result in a scale-dependent…

宇宙学与河外天体物理 · 物理学 2019-11-27 Jacques Colin , Roya Mohayaee , Mohamed Rameez , Subir Sarkar

We present a method to test the isotropy of the magnitude-redshift relation of Type Ia Supernovae (SNe Ia) and single out the most discrepant direction (in terms of the signal-to-noise ratio) with respect to the all-sky data. Our technique…

宇宙学与河外天体物理 · 物理学 2015-08-31 Behnam Javanmardi , Cristiano Porciani , Pavel Kroupa , Jan Pflamm-Altenburg

In this paper, we study the anisotropic expansion of the universe using type Ia supernovae Union 2.1 sample and 116 long gamma-ray bursts. The luminosity distance is expanded with model-independent cosmographic parameters as a function of…

宇宙学与河外天体物理 · 物理学 2015-06-22 J. S. Wang , F. Y. Wang

Studies of the peculiar velocity bulk flow based on different tools and datasets have been consistent so far in their estimation of the direction of the flow, which also happens to lie in close proximity to several features identified in…

宇宙学与河外天体物理 · 物理学 2015-06-12 Ben Rathaus , Ely D. Kovetz , Nissan Itzhaki

We test the isotropy of the expansion of the Universe by estimating the hemispherical anisotropy of supernova type Ia (SN Ia) Hubble diagrams at low redshifts (z<0.2). We compare the best fit Hubble diagrams in pairs of hemispheres and…

宇宙学与河外天体物理 · 物理学 2022-11-25 Benedict Bahr-Kalus , Dominik J. Schwarz , Marina Seikel , Alexander Wiegand

We study large-scale coherent motion in our universe using the existing Type IA supernovae data. If the recently observed bulk flow is real, then some imprint must be left on supernovae motion. We run a series of Monte Carlo Markov Chain…

宇宙学与河外天体物理 · 物理学 2015-05-27 De-Chang Dai , William H. Kinney , Dejan Stojkovic

In this paper, we study the anisotropy of cosmic acceleration the using Pantheon sample, which includes 1048 spectroscopically confirmed Type Ia supernovae (SNe Ia) covering the redshift range $0.01 < z < 2.3$. In hemisphere comparison…

宇宙学与河外天体物理 · 物理学 2018-07-05 Z. Q. Sun , F. Y. Wang

We present the first study of the isotropy of the distribution of morphological types of galaxies in the Local Universe out to around 200 Mpc using more than 60,000 galaxies from the HyperLeda database. We divide the sky into two opposite…

星系天体物理 · 物理学 2017-01-18 Behnam Javanmardi , Pavel Kroupa

Context. Our Local Group of galaxies appears to be moving relative to the cosmic microwave background with the source of the peculiar motion still uncertain. While in the past this has been studied mostly using galaxies as distance…

We analyze two volume limited galaxy samples from the SDSS photometric and spectroscopic data to test the isotropy in the local Universe. We use information entropy to quantify the global anisotropy in the galaxy distribution at different…

宇宙学与河外天体物理 · 物理学 2018-12-12 Suman Sarkar , Biswajit Pandey , Rishi Khatri

Recent studies have indicated that an anisotropic cosmic expansion may exist. In this paper, we use three datasets of type Ia supernovae (SNe Ia) to probe the isotropy of cosmic acceleration. For the Union2.1 dataset, the direction and…

宇宙学与河外天体物理 · 物理学 2019-10-23 Z. Q. Sun , F. Y. Wang

We test the isotropy of the Hubble diagram. At small redshifts, this is possible without assumptions on the cosmic inventory and provides a fundamental test of the cosmological principle. At higher redshift we check for the self-consistency…

天体物理学 · 物理学 2011-07-28 Dominik J. Schwarz , Bastian Weinhorst

We employ the hemisphere comparison (HC) method and the dipole fitting (DF) method to investigate the cosmic anisotropy in the recently released Pantheon sample of type Ia supernovae (SNe Ia) and five combinations among Pantheon. For the HC…

宇宙学与河外天体物理 · 物理学 2019-05-21 Dong Zhao , Yong Zhou , Zhe Chang

Astronomical observations showed that there may exist a bulk flow with peculiar velocities in the universe, which contradicts with the (\Lambda)CDM model. The bulk flow reveals that the observational universe is anisotropic at large scales.…

宇宙学与河外天体物理 · 物理学 2013-06-07 Zhe Chang , Ming-Hua Li , Sai Wang

We study the bulk flow of the local universe using Type Ia supernova data by considering a class of cosmological model which is spatially flat,(FRW) space-times and contains cold dark matter and $Q$ component (QCDM models) of the fluid as a…

宇宙学与河外天体物理 · 物理学 2022-05-31 A. Salehi , M. Yarahmadi , S. Fathi

We analyze the magnitude-redshift data of type Ia supernovae included in the Union and Union2 compilations in the framework of an anisotropic Bianchi type I cosmological model and in the presence of a dark energy fluid with anisotropic…

宇宙学与河外天体物理 · 物理学 2011-05-12 L. Campanelli , P. Cea , G. L. Fogli , A. Marrone

Peculiar velocities are one of the only probes of very large-scale mass density fluctuations in the nearby Universe. We present new "minimal variance" bulk flow measurements based upon the "First Amendment" compilation of 245 Type Ia…

宇宙学与河外天体物理 · 物理学 2015-06-03 Stephen J. Turnbull , Michael J. Hudson , Hume A. Feldman , Malcolm Hicken , Robert P. Kirshner , Richard Watkins

A combined sample of 79 high and low redshift supernovae Ia (SNe) is used to set constraints on the degree of anisotropy in the Universe out to $z\simeq1$. First we derive the global most probable values of matter density $\Omega_M $, the…

天体物理学 · 物理学 2015-06-24 Tsafrir S. Kolatt , Ofer Lahav
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