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相关论文: The Fine Structure Constant and Habitable Planets

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Observational constraints guide one forcefully to examine models in which the matter density is substantially less than critical density. Particularly noteworthy are those which are consistent with inflation. For these models, microwave…

天体物理学 · 物理学 2007-05-23 J. P. Ostriker , Paul J. Steinhardt

We search for transient variations of the fine structure constant using data from a European network of fiber-linked optical atomic clocks. By searching for coherent variations in the recorded clock frequency comparisons across the network,…

Standard definitions of habitability assume that life requires the presence of planetary gravity wells to stabilize liquid water and regulate surface temperature. Here the consequences of relaxing this assumption are evaluated. Temperature,…

地球与行星天体物理 · 物理学 2024-12-06 R. Wordsworth , C. Cockell

The goal of this paper is to explore the potential multistability of the climate of a planet around the habitable zone. A thorough investigation of the thermodynamics of the climate system is performed for very diverse conditions of energy…

大气与海洋物理 · 物理学 2015-06-05 Robert Boschi , Valerio Lucarini , Salvatore Pascale

In the past 15 years, astronomers have revealed that a significant fraction of the stars should harbor planets and that it is likely that terrestrial planets are abundant in our galaxy. Among these planets, how many are habitable, i.e.…

地球与行星天体物理 · 物理学 2013-05-09 Francois Forget

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

The early Universe inflation is well known as a promising theory to explain the origin of large scale structure of the Universe, a causal theory for the origin of primordial density fluctuations which may explain the observed density…

天体物理学 · 物理学 2007-05-23 Xin-he Meng

A stellar evolution computer model has been used to determine changes in the luminosity L and effective temperature T(e) of single stars during their time on the main sequence. The range of stellar masses investigated was from 0.5 to 1.5…

天体物理学 · 物理学 2009-11-10 David R. Underwood , Barrie W. Jones , P. Nick Sleep

The formation of the cosmic microwave background radiation (CMBR) provides a very powerful probe of the early universe at the epoch of recombination. Specifically, it is possible to constrain the variation of fundamental physical constants…

天体物理学 · 物理学 2009-10-31 Steen Hannestad

Many observed giant planets lie on eccentric orbits. Such orbits could be the result of strong scatterings with other giant planets. The same dynamical instability that produces these scatterings may also cause habitable planets in interior…

地球与行星天体物理 · 物理学 2016-09-21 Daniel Carrera , Melvyn B. Davies , Anders Johansen

In this paper, we investigate whether hypothetical Earth-like planets have high probability of remaining on stable orbits inside the habitable zones around the stars A and B of {\alpha} Centauri, for lengths of time compatible with the…

地球与行星天体物理 · 物理学 2015-06-22 Eduardo Andrade-Ines , Tatiana A. Michtchenko

Some properties of the world are fixed by physics derived from mathematical symmetries, while others are selected from an ensemble of possibilities. Several successes and failures of ``anthropic'' reasoning in this context are reviewed in…

天体物理学 · 物理学 2008-11-26 Craig J. Hogan

Our understanding of the processes that are relevant to the formation and maintenance of habitable planetary systems is advancing at a rapid pace, both from observation and theory. The present review focuses on recent research that bears on…

地球与行星天体物理 · 物理学 2014-03-27 Guillermo Gonzalez

We argue that models in which an observable variation of the fine structure constant is explained by motion of a cosmic scalar field, are not stable under renormalization, and require massive fine tuning that cannot be explained by any…

高能物理 - 唯象学 · 物理学 2009-11-07 T. Banks , M. Dine , M. R. Douglas

Conventional definitions of habitability require abundant liquid surface water to exist continuously over geologic timescales. Water in each of its thermodynamic phases interacts with solar and thermal radiation and is the cause for strong…

地球与行星天体物理 · 物理学 2017-03-15 Eric T. Wolf , Aomawa L. Shields , Ravi K. Kopparapu , Jacob Haqq-Misra , Owen B. Toon

A general Friedmann big-bang cosmology can be specified by fixing a half-dozen cosmological parameters such as the photon-to-baryon ratio Eta, the cosmological constant Lambda, the curvature scale R, and the amplitude Q of (assumed…

天体物理学 · 物理学 2009-11-06 Anthony Aguirre

In radiative layers of rotating stars the luminosity carried by circulation currents through a surface of constant entropy (circulation luminosity) is shown to be positive. The corresponding decrease in the temperature gradient is important…

天体物理学 · 物理学 2009-11-10 H. Kaehler

We investigate the hypothesis that the size of the habitable zone around hardened binaries in dense star-forming regions increases. Our results indicate that this hypothesis is essentially incorrect. Although certain binary star…

地球与行星天体物理 · 物理学 2019-06-12 Nikolaos Georgakarakos , Siegfried Eggl

Recently, we have performed research on the subject of the cosmological constant problem. The scenario is based on two postulates for inflationary theory: one is that inflaton $\phi$ can interact with radiation (relativistic particles); the…

广义相对论与量子宇宙学 · 物理学 2012-03-07 Yu-Chung Chen

There are indications from the study of quasar absorption spectra that the fine structure constant $\alpha$ may have been measurably smaller for redshifts $z>2.$ Analyses of other data ($^{149}$Sm fission rate for the Oklo natural reactor,…

高能物理 - 唯象学 · 物理学 2009-11-10 Luis Anchordoqui , Haim Goldberg