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相关论文: The Fine Structure Constant and Habitable Planets

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Ultraviolet radiation is a double-edged sword to life. If it is too strong, the terrestrial biological systems will be damaged. And if it is too weak, the synthesis of many biochemical compounds can not go along. We try to obtain the…

太阳与恒星天体物理 · 物理学 2010-03-08 Jianpo Guo , Fenghui Zhang , Xianfei Zhang , Zhanwen Han

The habitable zone is the main tool that mission architectures utilize to select potentially habitable planets for follow up spectroscopic observation. Given its importance, the precise size and location of the habitable zone remains a hot…

地球与行星天体物理 · 物理学 2020-04-02 Ramses M. Ramirez

Bekenstein's model of a scalar field, \phi, that affects the electromagnetic permeability (usually identified with ``changing \alpha'') predicts tiny variations of the effective fine structure constant up to very high red-shifts,…

高能物理 - 唯象学 · 物理学 2009-09-15 Keith A. Olive , Maxim Pospelov

The fine-structure constant, $\alpha$, controls the strength of the electromagnetic interaction. There are extensions of the standard model in which $\alpha$ is dynamical on cosmological length and time-scales. The physics of the cosmic…

宇宙学与河外天体物理 · 物理学 2019-02-27 Tristan L. Smith , Daniel Grin , David Robinson , Davy Qi

We calculate the properties and investigate the stability of stars that burn via strong (and electromagnetic) interactions, and compare their properties with those that, as in our Universe, include a rate-limiting weak interaction. It has…

太阳与恒星天体物理 · 物理学 2016-01-13 Luke A. Barnes

Planetary rotation rate is a key parameter in determining atmospheric circulation and hence the spatial pattern of clouds. Since clouds can exert a dominant control on planetary radiation balance, rotation rate could be critical for…

地球与行星天体物理 · 物理学 2014-04-29 Jun Yang , Gwenael Boue , Daniel C. Fabrycky , Dorian S. Abbot

Higher-dimensional theories have the remarkable feature of predicting a time (and hence redshift) dependence of the `fundamental' four dimensional constants on cosmological timescales. In this paper we update the bounds on a possible…

A phenomenological model is proposed to explain the recent observed cosmological variation of the fine structure constant as an effect of the quantum vacuum, assuming a flat universe with cosmological constant $\Lambda$ in the cases…

天体物理学 · 物理学 2010-12-17 Antonio F. Rañada

The current observational and experimental bounds on the time variation of the constants of nature (the fine structure constant $\alpha$, the gravitational constant $G$ and the proton-electron mass ratio $\mu=m_p/m_e$) are reviewed.

广义相对论与量子宇宙学 · 物理学 2012-01-03 Takeshi Chiba

Cosmological variation of the fine structure constant $\alpha$ due to the evolution of a spatially homogeneous ultra-light scalar field ($m \sim H_0$) during the matter and $\Lambda$ dominated eras is analyzed. Agreement of $\Delta…

天体物理学 · 物理学 2009-11-07 Carl L. Gardner

Whether binaries can harbor potentially habitable planets depends on several factors including the physical properties and the orbital characteristics of the binary system. While the former determines the location of the habitable zone…

地球与行星天体物理 · 物理学 2015-05-14 Nader Haghighipour , Rudolf Dvorak , Elke Pilat-Lohinger

The relative effects of variation of the fine structure constant alpha=e^2/hc and dimensionless strong interaction parameter m_q/Lambda_{QCD} are enhanced 5-6 orders of magnitude in very narrow ultraviolet transition between the ground and…

原子物理 · 物理学 2011-11-23 V. V. Flambaum

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

Recent updated results of quasar spectra suggested a 3.9$\sigma$ significance of spatial variation of the fine-structure constant. Theoretically, it is important to examine whether the fine-structure constant, as a fundamental constant in…

广义相对论与量子宇宙学 · 物理学 2020-11-17 Zhe Chang , Qing-Hua Zhu

Astrophysical tests of the stability of dimensionless fundamental couplings, such as the fine-structure constant $\alpha$, are an area of much increased recent activity, following some indications of possible spacetime variations at the few…

宇宙学与河外天体物理 · 物理学 2014-07-16 P. M. M. Leal , C. J. A. P. Martins , L. B. Ventura

We analyse the constraints obtained from new atomic clock data on the possible time variation of the fine structure `constant' and the electron-proton mass ratio and show how they are strengthened when the seasonal variation of Sun's…

宇宙学与河外天体物理 · 物理学 2010-02-25 Douglas J. Shaw , John D. Barrow

Any time variation in the fine-structure constant alters the ionization history of the universe and therefore changes the pattern of cosmic microwave background fluctuations. We calculate the changes in the spectrum of these fluctuations as…

天体物理学 · 物理学 2009-10-31 Manoj Kaplinghat , Robert J. Scherrer , Michael S. Turner

In the report submitted here, an elementary formula is presented that allows calculation of the fine structure constant, derived on the basis of the unified theory of the electromagnetic and gravitational field elaborated by the author.…

综合物理 · 物理学 2007-05-23 Jaroslav Pavel

The ability of a planet to maintain surface water, key to life as we know it, depends on solar and planetary energy. As a star ages, it delivers more energy to a planet. As a planet ages it produces less internal heat, which leads to…

地球与行星天体物理 · 物理学 2021-06-29 Johnny Seales , Adrian Lenardic

We propose the concept of a "Galactic Habitable Zone" (GHZ). Analogous to the Circumstellar Habitable Zone (CHZ), the GHZ is that region in the Milky Way where an Earth-like planet can retain liquid water on its surface and provide a…

天体物理学 · 物理学 2008-11-26 Guillermo Gonzalez , Donald Brownlee , Peter Ward