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Related papers: A biotic cosmos demystified?

200 papers

Whereas the Solar System has Mars and Europa as the best candidates for finding fossil/extant life as we know it - based on complex carbon compounds and liquid water - the 263 (non-pulsar) planetary systems around other stars as known at 15…

Earth and Planetary Astrophysics · Physics 2018-12-05 Barrie W Jones

Modelling of Extreme Scattering Events suggests that the Galaxy's dark matter is an undetected population of cold, AU-sized, planetary-mass gas clouds. None of the direct observational constraints on this picture -- thermal/non-thermal…

Astrophysics · Physics 2015-06-24 Mark Walker , Mark Wardle

Solar, atmospheric and reactor neutrino experiments established that neutrinos are massive. It is quite natural then to consider neutrinos as candidate particles for explaining the dark matter in halos around galaxies. We study the…

High Energy Physics - Phenomenology · Physics 2015-06-04 A. Nicolaidis

A habitable zone of a star is defined as a range of orbits within which a rocky planet can support liquid water on its surface. The most intriguing question driving the search for habitable planets is whether they host life. But is the age…

Earth and Planetary Astrophysics · Physics 2016-03-24 M. Safonova , J. Murthy , Yu. A. Shchekinov

The recently constructed Dehnen-Binney set of mass models for the Galaxy is used to show that the decaying neutrino theory for the ionisation of the interstellar medium (Sciama 1990a, 1993) requires the neutrino halo of the Galaxy to be as…

Astrophysics · Physics 2007-05-23 D. W. Sciama

The Fermi paradox is the discrepancy between the strong likelihood of alien intelligent life emerging (under a wide variety of assumptions) and the absence of any visible evidence for such emergence. We use this intriguing unlikeness to…

High Energy Astrophysical Phenomena · Physics 2019-08-06 Luis A. Anchordoqui , Susanna M. Weber , Jorge F. Soriano

The Great Filter interpretation of Fermi's great silence asserts that $Npq$ is not a very large number, where $N$ is the number of potentially life-supporting planets in the observable universe, $p$ is the probability that a randomly chosen…

Popular Physics · Physics 2015-11-19 Vilhelm Verendel , Olle Häggström

One signature of an expanding universe is the time-variation of the cosmological abundances of its different components. For example, a radiation-dominated universe inevitably gives way to a matter-dominated universe, and critical moments…

Cosmology and Nongalactic Astrophysics · Physics 2022-02-09 Keith R. Dienes , Lucien Heurtier , Fei Huang , Doojin Kim , Tim M. P. Tait , Brooks Thomas

Neutralino dark matter leads to the formation of numerous earth mass dark matter haloes at redshifts z\approx 60 (Diemand et al. 2005). These abundant CDM micro-haloes have cuspy density profiles that can easily withstand the Galactic tidal…

Astrophysics · Physics 2007-05-23 Ben Moore , Juerg Diemand , Joachim Stadel , Thomas Quinn

The number of people able to end Earth's technical civilization has heretofore been small. Emerging dual-use technologies, such as biotechnology, may give similar power to thousands or millions of individuals. To quantitatively investigate…

Popular Physics · Physics 2019-08-15 John G. Sotos

The history of life on Earth and in other potential life-bearing planetary platforms is deeply linked to the history of the universe. Since life as we know it relies on chemical elements forged in dying heavy stars, the universe needs to be…

Popular Physics · Physics 2015-06-04 Marcelo Gleiser

The brightnesses of supernovae are commonly understood to indicate that cosmological expansion is accelerating due to dark energy. However the entire discussion presumes a perfectly transparent universe because no effects of reddening…

Astrophysics · Physics 2015-06-24 Rudolph E. Schild , Marius Dekker

Understanding the concept of habitability is related to an evolutionary knowledge of the particular planet-in-question. Additional indications so-called "systemic aspects" of the planetary system as a whole governs a particular planet's…

It is investigated how biofriendly is the Milky Way for photosynthetic life. Special attention is dedicated to the role of the photobiological regime in the emergence and evolution of this kind of life in terrestrial planets. Following this…

Earth and Planetary Astrophysics · Physics 2011-03-02 Osmel Martín , Rolando Cárdenas , Jorge Horvath

With the discovery of hundreds of exoplanets and a potentially huge number of Earth-like planets waiting to be discovered, the conditions for their habitability have become a focal point in exoplanetary research. The classical picture of…

Earth and Planetary Astrophysics · Physics 2015-06-22 M. Guedel , R. Dvorak , N. Erkaev , J. Kasting , M. Khodachenko , H. Lammer , E. Pilat-Lohinger , H. Rauer , I. Ribas , B. E. Wood

Earth-scale planets in the classical habitable zone (HZ) are more likely to be habitable if they possess active geophysics. Without a constant internal energy source, planets cool as they age, eventually terminating tectonic activity and…

Earth and Planetary Astrophysics · Physics 2015-06-18 Christa Van Laerhoven , Rory Barnes , Richard Greenberg

Cosmology yields the most restrictive limits on neutrino masses and conversely, massive neutrinos would contribute to the cosmic dark-matter density and would play an important role for the formation of structure in the universe. Neutrino…

High Energy Physics - Phenomenology · Physics 2015-06-25 G. G. Raffelt

The habitable zone is the circumstellar region in which a terrestrial-mass planet with an atmosphere can sustain liquid water on its surface. However, despite the usefulness of this concept, it is being found to be increasingly limiting in…

Popular Physics · Physics 2020-08-05 Ian von Hegner

We address the possibility that intelligent civilisations that destroy themselves could present signatures observable by humanity. Placing limits on the number of self-destroyed civilisations in the Milky Way has strong implications for the…

Earth and Planetary Astrophysics · Physics 2020-12-16 Adam Stevens , Duncan Forgan , Jack O'Malley-James

We derive general constraints on the relic abundances of a long-lived particle which mainly decays into a neutrino (and something else) at cosmological time scales. Such an exotic particle may show up in various particle-physics models…

High Energy Physics - Phenomenology · Physics 2008-11-26 Toru Kanzaki , Masahiro Kawasaki , Kazunori Kohri , Takeo Moroi