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相关论文: On Larger $H_0$ Values in the CMB Dipole Direction

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Gamma ray bursts (GRBs) have recently attracted much attention as a possible way to extend the Hubble diagram to very high redshift. To this aim, the luminosity (or isotropic emitted energy) of a GRB at redshift z must be evaluated from a…

宇宙学与河外天体物理 · 物理学 2010-01-11 V. F. Cardone , S. Capozziello , M. G. Dainotti

The Cosmological Principle, that the Universe is homogeneous and isotropic on sufficiently large scales, underpins the standard model of cosmology. However, a recent analysis of 1.36 million infrared-selected quasars has identified a…

宇宙学与河外天体物理 · 物理学 2023-08-08 Lawrence Dam , Geraint F. Lewis , Brendon J. Brewer

Inflationary cosmology predicts that the particle horizon should be generically much bigger than the present-day Hubble radius, $1/H_0$. This implies a special regime of super-Hubble scale energy density fluctuations imprinted on the cosmic…

天体物理学 · 物理学 2009-10-30 Arjun Berera , Li-Zhi Fang , Gary Hinshaw

This paper is a demonstration of how relativistic, broad-lined type Ic supernovae (SNe IcBL) can be used to constrain a value of the Hubble constant in the local universe ($H_{0}$). Included in our sample of SNe IcBL are the SNe associated…

宇宙学与河外天体物理 · 物理学 2016-01-22 Zach Cano , Pall Jakobsson , Oli Pall Geirsson

This paper presents a new model-independent constraint on the Hubble constant ($H_0$) by anchoring relative distances from Type Ia supernovae (SNe Ia) observations to absolute distance measurements from time-delay strong Gravitational…

宇宙学与河外天体物理 · 物理学 2025-03-13 L. R. Colaço

The difference from 4 to 6 $\sigma$ in the Hubble constant ($H_0$) between the values observed with the local (Cepheids and Supernovae Ia, SNe Ia) and the high-z probes (CMB obtained by the Planck data) still challenges the astrophysics and…

Tight constraints on cosmological parameters can be obtained with standard candles spanning a range of redshifts as large as possible. We propose to treat SN Ia and long Gamma-Ray Bursts (GRBs) as a single class of candles. Taking advantage…

天体物理学 · 物理学 2007-05-23 C. Firmani , V. Avila-Reese , G. Ghisellini , G. Ghirlanda

We are in motion against the cosmic backdrop. This motion is evidenced by the systematic temperature shift - or dipole anisotropy - observed in the Cosmic Microwave Background radiation (CMB). Because of the Doppler effect, the temperature…

天体物理学 · 物理学 2015-06-24 Chris Blake , Jasper Wall

In standard cosmology, the late Universe is assumed to be statistically homogeneous and isotropic. However, a recent study based on galaxy clusters by Migkas et al. (2021, arXiv:2103.13904) found an apparent spatial variation of…

宇宙学与河外天体物理 · 物理学 2024-12-02 A. Pandya , K. Migkas , T. H. Reiprich , A. Stanford , F. Pacaud , G. Schellenberger , L. Lovisari , M. E. Ramos-Ceja , N. T. Nguyen-Dang , S. Park

The Cosmological Principle, which states that the Universe is homogeneous and isotropic (when averaged on large scales), is the foundational assumption of Friedmann-Lemaitre-Robertson-Walker (FLRW) cosmologies such as the current standard…

宇宙学与河外天体物理 · 物理学 2025-12-15 Nathan Secrest , Sebastian von Hausegger , Mohamed Rameez , Roya Mohayaee , Subir Sarkar

The Hubble diagram (HD) is a plot that contains luminous distance modulus presented with respect to the redshift. The distance modulus--redshift relation of the most well-known ``standard candles'', the type Ia supernovae (SN), is a crucial…

宇宙学与河外天体物理 · 物理学 2023-11-07 Nikita Lovyagin , Rustam Gainutdinov , Stanislav Shirokov , Vladimir Gorokhov

Gravitational waves (GWs) from compact binary coalescences (CBCs) can constrain the cosmic expansion of the universe. In the absence of an associated electromagnetic counterpart, the spectral sirens method exploits the relation between the…

宇宙学与河外天体物理 · 物理学 2023-12-20 Grégoire Pierra , Simone Mastrogiovanni , Stéphane Perriès , Michela Mapelli

The Universe on scales $10-100~h^{-1}$ Mpc is dominated by a cosmic web of voids, filaments, sheets and knots of galaxy clusters. These structures participate differently in the global expansion of the Universe: from non-expanding clusters…

宇宙学与河外天体物理 · 物理学 2016-06-21 Krzysztof Bolejko , M. Ahsan Nazer , David L. Wiltshire

Recent cosmic microwave background (CMB) measurements over a large range of angular scales have become sensitive enough to provide interesting constraints on cosmological parameters within a restricted class of models. We use the CMB…

天体物理学 · 物理学 2008-02-03 Charles H. Lineweaver , Domingos Barbosa

The current knowledge in cosmology deals with open problems whose solutions are still under investigation. The main issue is the so-called Hubble constant ($H_0$) tension, namely, the $4-6 \sigma$ discrepancy between the local value of…

宇宙学与河外天体物理 · 物理学 2025-01-23 Maria Giovanna Dainotti , Biagio De Simone , Aditya Narendra , Agnieszka Pollo

We report estimates of the cosmological parameters $\Omega_m$ and $\Omega_{\Lambda}$ obtained using supernovae (SNe) associated with gamma-ray bursts (GRBs) at redshifts up to 0.606. Eight high-fidelity GRB-SNe with well-sampled light…

宇宙学与河外天体物理 · 物理学 2015-06-22 Xue Li , Jens Hjorth , Radosław Wojtak

We revisit the degeneracy between the Hubble constant, $H_0$, and matter density, $\Omega_m$, for current cosmic microwave background (CMB) observations within the standard $\Lambda CDM$ model. We show that Planck, Wilkinson Microwave…

宇宙学与河外天体物理 · 物理学 2021-01-26 Joshua A. Kable , Graeme E. Addison , Charles L. Bennett

We review a subset of the current tensions affecting the standard $\Lambda$CDM cosmological model, emphasizing the role of chronic systematics and significance inflation in shaping their interpretation. As a unifying framework, we consider…

宇宙学与河外天体物理 · 物理学 2026-02-02 Valerio Marra

We present a measurement of the Hubble constant ($H_{0}$) and other cosmological parameters from a joint analysis of six gravitationally lensed quasars with measured time delays. All lenses except the first are analyzed blindly with respect…

Recent observations by the Hubble Space Telescope of Cepheids in the Virgo cluster imply a Hubble Constant $H_0=80\pm17$\ km/sec/Mpc. We attempt to clarify some issues of interpretation of these results for determining the global…

天体物理学 · 物理学 2016-08-30 A. H. Jaffe