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Scientific program for the Forward Physics Facility. [PDF]

open access: yesEur Phys J C Part Fields
Adhikary J   +25 more
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Strong Gravitational Lensing and Microlensing of Supernovae. [PDF]

open access: yesSpace Sci Rev
Suyu SH   +4 more
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High-Energy Phenomena in Extreme Astrophysical Objects and the Origin of High-Energy Cosmic Rays

open access: yesHigh-Energy Phenomena in Extreme Astrophysical Objects and the Origin of High-Energy Cosmic Rays
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Scaling astrophysical phenomena to high-energy-density laboratory experiments

Plasma Physics and Controlled Fusion, 2002
The spatial and temporal scales of astrophysical phenomena are typically 10–20 orders of magnitude greater than those of laboratory experiments intended to simulate them. Accordingly, the issue of similarity between the astrophysical phenomenon and its laboratory counterpart becomes quite important.
D D Ryutov, B A Remington
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Relationship between high-energy physical phenomena on the sun and in astrophysics

Solar Physics, 1988
High energy phenomena on the surface of the Sun are manifestations of part of the solar dynamo cycle. Convection and magnetic field give rise to unstable, twisted flux loops that become solar flares when the resistive tearing mode proceeds to the nonlinear limit.
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SUPERNOVAE AS PHENOMENA OF HIGH‐ENERGY ASTROPHYSICS*

Annals of the New York Academy of Sciences, 1977
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