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相关论文: Limits on evolution of the fine-structure constant…

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As is well known, measurements of the Sunyaev-Zeldovich effect can be combined with observations of the X-ray surface brightness of galaxy clusters to estimate the angular diameter distance to these structures. In this paper, we show that…

宇宙学与河外天体物理 · 物理学 2021-11-01 R. F. L. Holanda , V. C. Busti , L. R. Colaço , J. S. Alcaniz , S. J. Landau

We propose a new method to probe a possible time evolution of the fine structure constant $\alpha$ from X-ray and Sunyaev-Zeldovich measurements of the gas mass fraction ($f_{gas}$) in galaxy clusters. Taking into account a direct relation…

宇宙学与河外天体物理 · 物理学 2021-11-01 R. F. L. Holanda , S. J. Landau , J. S. Alcaniz , I. E. Sanchez G. , V. C. Busti

In order to probe a possible time variation of the fine-structure constant ($\alpha$), we propose a new method based on Strong Gravitational Lensing and Type Ia Supernovae observations. By considering a class of dilaton runaway models,…

宇宙学与河外天体物理 · 物理学 2021-10-04 L. R. Colaço , R. F. L. Holanda , R. Silva

We study the detailed evolution of the fine-structure constant $\alpha$ in the string-inspired runaway dilaton class of models of Damour, Piazza and Veneziano. We provide constraints on this scenario using the most recent $\alpha$…

宇宙学与河外天体物理 · 物理学 2015-03-18 C. J. A. P. Martins , P. E. Vielzeuf , M. Martinelli , E. Calabrese , S. Pandolfi

Galaxy clusters have been used as a cosmic laboratory to verify a possible time variation of fundamental constants. Particularly, it has been shown that the ratio $Y_{SZ}D_{A}^{2}/C_{XZS}Y_X $, which is expected to be constant with…

宇宙学与河外天体物理 · 物理学 2021-11-01 L. R. Colaço , R. F. L. Holanda , R. Silva , J. S. Alcaniz

A new method based on large-scale structure observations is proposed to probe a possible time variation of the fine-structure constant ($\alpha$). Our analyses are based on time-delay of Strong Gravitational Lensing and Type Ia Supernovae…

宇宙学与河外天体物理 · 物理学 2021-09-09 L. R. Colaço , J. E. Gonzalez , R. F. L. Holanda

We search for a variation of the electromagnetic fine structure constant ($\alpha \equiv e^2/\hbar c$) using a sample of 58 SZ selected clusters in the redshift range ($0.2<z<1.5$) detected by the South Pole Telescope, along with X-ray…

宇宙学与河外天体物理 · 物理学 2021-02-12 Kamal Bora , Shantanu Desai

We explore a possible time variation of the fine structure constant ($\alpha \equiv e^2/\hbar c$) using the Sunyaev-Zel'dovich effect measurements of galaxy clusters along with their X-ray observations. Specifically, the ratio of the…

宇宙学与河外天体物理 · 物理学 2021-11-24 Zhi-E Liu , Wen-Fei Liu , Tong-Jie Zhang , Zhong-Xu Zhai , Kamal Bora

We have constrained the spatial variation of the fine structure constant using multi-frequency measurements of the thermal Sunyaev-Zeldovich effect of 618 X-ray selected clusters. Although our results are not competitive with the ones from…

宇宙学与河外天体物理 · 物理学 2016-12-22 I. de Martino , C. J. A. P. Martins , H. Ebeling , D. Kocevski

We propose a new method to probe for variations in the fine structure constant alpha using clusters of galaxies, opening up a window on a new redshift range for such constraints. Hot clusters shine in the X-ray mainly due to bremsstrahlung,…

宇宙学与河外天体物理 · 物理学 2015-06-12 Silvia Galli

We propose a new method to use the kinematic Sunyaev-Zeldovich for measuring the baryon fraction in cluster of galaxies. In this proposal we need a configuration in which a supernova Type Ia resides in a brightest cluster galaxy of…

宇宙学与河外天体物理 · 物理学 2019-02-12 Shant Baghram

The possible time variation of the fundamental constants of nature has been an active subject of research since the large-number hypothesis was proposed by Dirac. In this paper, we propose a new method to investigate a possible time…

宇宙学与河外天体物理 · 物理学 2022-08-29 L. R. Colaço , S. J. Landau , J. E. Gonzalez , J. Spinelly , G. L. F. Santos

The large-number hypothesis conjectures that fundamental constants may vary. Accordingly, the spacetime variation of fundamental constants has been an active subject of research for decades. Recently, using data obtained with large…

宇宙学与河外天体物理 · 物理学 2015-04-23 Lucila Kraiselburd , Susana J. Landau , Carolina Negrelli , Enrique García-Berro

Aims. We constrain a hypothetical variation in the fundamental physical constants over the course of cosmic time. Methods. We use unique observations of the CO(7-6) rotational line and the [CI] 3P_2 - 3P_1 fine-structure line towards a…

宇宙学与河外天体物理 · 物理学 2013-06-12 S. A. Levshakov , F. Combes , F. Boone , I. I. Agafonova , D. Reimers , M. G. Kozlov

We propose an improved methodology to constrain spatial variations of the fine structure constant using clusters of galaxies. We use the {\it Planck} 2013 data to measure the thermal Sunyaev-Zeldovich effect at the location of 618 X-ray…

宇宙学与河外天体物理 · 物理学 2016-11-02 I. de Martino , C. J. A. P. Martins , H. Ebeling , D. Kocevski

Testing possible variations in fundamental constants of nature is a crucial endeavor in observational cosmology. This paper investigates potential cosmological variations in the fine structure constant ($\alpha$) through a non-parametric…

宇宙学与河外天体物理 · 物理学 2024-10-30 Marcelo Ferreira , Rodrigo F. L. Holanda , Javier E. Gonzalez , L. R. Colaço , Rafael C. Nunes

Star-forming galaxies at high redshifts are the ideal targets to probe the hypothetical variation of the fine-structure constant alpha over cosmological time scales. We propose a modification of the alkali doublets method which allows us to…

宇宙学与河外天体物理 · 物理学 2017-05-10 S. A. Levshakov , M. G. Kozlov

Since Dirac stated his Large Number Hypothesis the space-time variation of fundamental constants has been an active subject of research. Here we analyze the possible spatial variation of two fundamental constants: the fine structure…

宇宙学与河外天体物理 · 物理学 2018-12-10 Carolina Negrelli , Lucila Kraiselburd , Susana J. Landau , Enrique García-Berro

We present constraints on cosmological parameters based on a sample of Sunyaev-Zel'dovich-selected galaxy clusters detected in a millimeter-wave survey by the Atacama Cosmology Telescope. The cluster sample used in this analysis consists of…

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