2012
DOI: 10.1098/rsta.2011.0351
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Astrophysical explosions: from solar flares to cosmic gamma-ray bursts

Abstract: Astrophysical explosions result from the release of magnetic, gravitational or thermonuclear energy on dynamical time scales, typically the sound-crossing time for the system. These explosions include solar and stellar flares, eruptive phenomena in accretion discs, thermonuclear combustion on the surfaces of white dwarfs and neutron stars, violent magnetic reconnection in neutron stars, thermonuclear and gravitational collapse supernovae and cosmic gamma-ray bursts, each representing a different type and amoun… Show more

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Cited by 8 publications
(4 citation statements)
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References 82 publications
(119 reference statements)
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“…One can see from Table 1 that the energy released through the conversion of gravitons to photons using the mechanism detailed by Raffelt and Stodolsky remains significant, similar in magnitude to solar flares occurring on the surface of the sun [16]. Furthermore the fluxes are quite bright and therefore potentially detectable.…”
Section: Resultsmentioning
confidence: 88%
“…One can see from Table 1 that the energy released through the conversion of gravitons to photons using the mechanism detailed by Raffelt and Stodolsky remains significant, similar in magnitude to solar flares occurring on the surface of the sun [16]. Furthermore the fluxes are quite bright and therefore potentially detectable.…”
Section: Resultsmentioning
confidence: 88%
“…Firestone (2014; hereafter F14) bases arguments for abundant moderately nearby SNe (Wheeler 2012) on data of measured cosmogenic isotope deposition and nitrate accumulation in terrestrial archives. The claimed rate of 23 SNe within 300 pc of the Earth within the last 300 kyr would exceed the average galactic rate by a factor of 4; so the claim is suspicious if only on this basis.…”
Section: Introduction: Ionizing Radiation From Supernovae (Sne)mentioning
confidence: 99%
“…the ratio of the characteristic physical size (R) and the propagation speed (v) of any kind of disturbance initiated during the release (see, e.g. Wheeler 2012). A typical characteristic of these explosions is that the rising time of energy release is very short in comparison with the decay phase independently of the physics behind these explosions.…”
Section: Introductionmentioning
confidence: 99%