中文
相关论文

相关论文: Probing the anisotropic local universe and beyond …

200 篇论文

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 test the isotropy of the local Universe using low redshift supernova data from various catalogs and the non-parametric method of smoothed residuals. Using a recently developed catalog which combines supernova data from various surveys,…

宇宙学与河外天体物理 · 物理学 2015-06-15 Stephen Appleby , Arman Shafieloo , Andrew Johnson

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 present a cosmological analysis of the Lick Observatory Supernova Search (LOSS) Type Ia supernova (SN Ia) photometry sample introduced by Ganeshalingam et al. (2010). These SNe provide an effective anchor point to estimate cosmological…

宇宙学与河外天体物理 · 物理学 2013-07-04 Mohan Ganeshalingam , Weidong Li , Alexei V. Filippenko

We investigate the validity of the Cosmological Principle by mapping the cosmological parameters $H_0$ and $q_0$ through the celestial sphere. In our analysis, performed in a low-redshift regime to follow a model-independent approach, we…

宇宙学与河外天体物理 · 物理学 2015-07-21 C. A. P. Bengaly , A. Bernui , J. S. Alcaniz

We re-examine the contentious question of constraints on anisotropic expansion from Type Ia supernovae (SNIa) in the light of a novel determination of peculiar velocities, which are crucial to test isotropy with supernovae out to distances…

宇宙学与河外天体物理 · 物理学 2022-06-08 W. Rahman , R. Trotta , S. S. Boruah , M. J. Hudson , D. A. van Dyk

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

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

We present the Democratic Samples of Supernovae (DSS), a compilation of 775 low-redshift Type Ia and II supernovae (SNe Ia & II), of which 137 SN Ia distances are derived via the newly developed snapshot distance method. Using the objects…

宇宙学与河外天体物理 · 物理学 2021-05-26 Benjamin E. Stahl , Thomas de Jaeger , Supranta S. Boruah , WeiKang Zheng , Alexei V. Filippenko , Michael J. Hudson

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

The standard cosmology strongly relies upon the Cosmological Principle, which consists on the hypotheses of large scale isotropy and homogeneity of the Universe. Testing these assumptions is, therefore, crucial to determining if there are…

宇宙学与河外天体物理 · 物理学 2018-04-27 U. Andrade , C. A. P. Bengaly , J. S. Alcaniz , B. Santos

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

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 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

In this paper, we study an anisotropic universe model with Bianchi-I metric using Joint Light-curve Analysis (JLA) sample of type Ia supernovae (SNe Ia). Because light-curve parameters of SNe Ia vary with different cosmological models and…

宇宙学与河外天体物理 · 物理学 2017-12-27 Y. Y. Wang , F. Y. Wang

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

Within the volume-limited subsample at $z<0.06$ of the Zwicky Transient Facility (ZTF) DR2 sample, we confirm a statistically significant excess of Type Ia supernovae (SNe Ia) at $z \simeq 0.02$-$0.04$, previously reported but not explained…

Type Ia supernovae (SNe Ia) were instrumental in establishing the acceleration of the universe's expansion. By virtue of their combination of distance reach, precision, and prevalence, they continue to provide key cosmological constraints,…

We re-analyze the detectability of large scale dark flow (or local bulk flow) with respect to the CMB background based upon the redshift-distance relation for Type Ia supernovae (SN Ia). We made two independent analyses: one based upon…

宇宙学与河外天体物理 · 物理学 2016-08-19 G. J. Mathews , B. Rose , P. Garnavich , D. Yamazaki , T. Kajino

The rate evolution of subluminous Type Ia Supernovae is presented using data from the Supernova Legacy Survey. This sub-sample represents the faint and rapidly-declining light-curves of the observed supernova Ia (SN Ia) population here…

‹ 上一页 1 2 3 10 下一页 ›