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相关论文: The Fine Structure Constant and Habitable Planets

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A numerical coincidence relating the values of the cosmological, gravitational and electromagnetic fine structure constants is presented and discussed in relation to the apparent anthropic fine-tuning of these three fundamental constants of…

广义相对论与量子宇宙学 · 物理学 2015-10-26 Laurence Eaves

Within the framework of an eternal inflationary scenario, a natural question regarding the production of eternal bubbles is the essential condition requires to have a universe capable of generating life. In either an open or a closed…

宇宙学与河外天体物理 · 物理学 2017-08-30 Sohrab Rahvar

The effective coupling `constants' of physics, especially the cosmological constant, are observed to have highly biophilic values. If this is not a hugely improbable accident, or a consequence of some mysterious logical necessity or of some…

高能物理 - 理论 · 物理学 2011-01-31 Don N. Page

The habitability of a planet depends on various factors, such as delivery of water during the formation, the co-evolution of the interior and the atmosphere, as well as the stellar irradiation which changes in time. Since an unknown number…

地球与行星天体物理 · 物理学 2019-05-01 Mareike Godolt , Nicola Tosi , Barbara Stracke , J. Lee Grenfell , Thomas Ruedas , Tilman Spohn , Heike Rauer

An anthropic explanation for evident smallness of the value of the dark energy implies the existence of a time-dependent component of the scalar field, serving, together with a negative-valued cosmological constant, as one of two components…

广义相对论与量子宇宙学 · 物理学 2020-01-08 A. A. Yurova , A. V. Yurov , V. A. Yurov

Star-like objects with effective temperatures of less than 2,700 kelvin are referred to as ultracool dwarfs. This heterogeneous group includes stars of extremely low mass as well as brown dwarfs (substellar objects not massive enough to…

Habitability is usually defined as the requirement for a terrestrial planet's atmosphere to sustain liquid water. This definition can be complemented by the dynamical requirement that other planets in the system do not gravitationally…

天体物理学 · 物理学 2009-11-07 Kristen Menou , Serge Tabachnik

The constraints on the time variation of the fine structure constant at recombination epoch relative to its present value, $\Delta\alpha/\alpha \equiv (\alpha_{\mathrm{rec}} - \alpha_{\mathrm{now}})/\alpha_{\mathrm{now}}$, are obtained from…

天体物理学 · 物理学 2014-11-18 Masahiro Nakashima , Ryo Nagata , Jun'ichi Yokoyama

The melt productivity of a differentiated planet's mantle is primarily controlled by its iron content, which is itself approximated by the planet's core mass fraction (CMF). Here we show that estimates of an exo-planet's CMF allows robust…

地球与行星天体物理 · 物理学 2021-06-02 Brendan Dyck , Jon Wade , Richard Palin

The habitable zone is defined as the orbital region around a star where planetary feedback cycles buffer atmospheric greenhouse gases that, in combination with solar luminosity, maintain surface temperatures suitable for liquid water.…

地球与行星天体物理 · 物理学 2025-09-04 Morgan Underwood , Adrian Lenardic , Johnny Seales , Benjamin Kwait-Gonchar

New and rather controversial observations hint that the fine structure constant \alpha may have been smaller in the early universe, suggesting that some of the fundamental ``constants'' of physics may be dynamical. In a recent paper,…

高能物理 - 理论 · 物理学 2010-04-28 S. Carlip , S. Vaidya

We critically assess recent claims suggesting that upper limits on the time variation of the fine-structure constant tightly constrain the coupling of a dark energy scalar field to the electromagnetic sector, and, indirectly, the violation…

宇宙学与河外天体物理 · 物理学 2016-04-20 P. P. Avelino

We study the effect of a finite topology on the temperature correlations of the cosmic microwave background in a flat universe. Analytic expressions for the angular power spectrum are given for all possible finite flat models. We examine…

天体物理学 · 物理学 2009-10-31 Evan Scannapieco , Janna Levin , Joseph Silk

The possibility of variations of the values of fundamental constants is a phenomenon predicted by a number of scenarios beyond General Relativity. This can happen if ``our'' fundamental constants are not the actual constants of the…

广义相对论与量子宇宙学 · 物理学 2024-07-12 Cosimo Bambi

At present, because of observational selection effects, we know of no exoplanetary systems with any planetary masses close to that of the Earth. We have therefore used computer models to see whether such planets could be dynamically stable…

天体物理学 · 物理学 2008-11-26 Barrie W Jones , P Nick Sleep , David R Underwood

We summarize the results of two experiments to address important issues related to the correlation between planet frequencies and properties and the metallicity of the hosts. Our results can usefully inform formation, structural, and…

Observations of exoplanets and protoplanetary disks show that binary stellar systems can host planets in stable orbits. Given the high binary fraction among stars, the contribution of binary systems to Galactic habitability should be…

地球与行星天体物理 · 物理学 2020-11-18 Paolo Simonetti , Giovanni Vladilo , Laura Silva , Alessandro Sozzetti

The notion of ``fundamental constant'' is heavily theory-laden. A natural, fairly precise formulation is possible in the context of the standard model (here defined to include gravity). Some fundamental constants have profound geometric…

高能物理 - 唯象学 · 物理学 2007-09-03 Frank Wilczek

We present updated constraints on the variation of the fine structure constant, $\alpha_{\rm EM}$, and effective electron rest mass, $m_{\rm e}$, during the cosmological recombination era. These two fundamental constants directly affect the…

宇宙学与河外天体物理 · 物理学 2020-05-25 Luke Hart , Jens Chluba

If the recent observations suggesting a time variation of the fine structure constant are correct, they imply the existence of an ultra light scalar particle. This particle inevitably couples to nucleons through the \alpha-dependence of…

高能物理 - 唯象学 · 物理学 2009-11-07 Gia Dvali , Matias Zaldarriaga