Results 131 to 140 of about 1,300,084 (347)
Interactions of Cosmic Ray Nuclei [PDF]
We present convenient formulae for the energy losses of energetic atomic nuclei over the entire energy range relevant to the physics of cosmic rays. Results are applied to a leaky-box equation with a complete loss term. Thereby we derive the equilibrium spectrum of cosmic rays in various types of galaxies.
arxiv
Abstract Short‐lived, unobservable, and not subject to the usual rules of conservation of energy and momentum, virtual particles—an integral part of the conceptual framework of quantum field theory (QFT)—exhibit a number of curious characteristics which, in recent decades, have in part fueled important discussions about their ontological status ...
Jean‐Philippe Martinez
wiley +1 more source
Mercury's small magnetosphere is embedded in the dynamic and intense solar wind environment characteristic of the inner heliosphere. Both the magnitude and orientation of the interplanetary magnetic field (IMF) significantly influence the solar wind ...
Charles F. Bowers+7 more
doaj +1 more source
ALICE, the dedicated heavy-ion experiment at the LHC, has also a rich pp program benefiting from its low material budget, low magnetic field, and its extensive particle identification capabilities.
Grosse-Oetringhaus Jan Fiete
doaj +1 more source
Astronomy and Cosmical Physics at the British Association [PDF]
A. R. H.
openalex +1 more source
Cosmic-ray physics at the South Pole
The geographic South Pole provides unique opportunities to study cosmic particles in the Southern Hemisphere. It represents an optimal location to deploy large-scale neutrino telescopes in the deep Antarctic ice, such as AMANDA or IceCube. In both cases, the presence of an array, constructed to observe extensive air showers, enables hybrid measurements
Soldin, Dennis+3 more
openaire +5 more sources
The Vlasov Equation Cannot Fully Account for Collisionless Shocks
ABSTRACT It is argued that the Vlasov equation cannot fully account for collisionless shocks since it conserves entropy, while a shock does not. A rigorous mathematical theory of collisionless shocks could require working at the Klimontovich level.
Antoine Bret
wiley +1 more source
Janossy: COSMIC RAYS AND NUCLEAR PHYSICS/Powell und Occhialini: NUCLEAR PHYSICS IN PHOTOGRAPHS [PDF]
Schopper
openalex +1 more source
Abstract Exposure levels without appreciable human health risk may be determined by dividing a point of departure on a dose–response curve (e.g., benchmark dose) by a composite adjustment factor (AF). An “effect severity” AF (ESAF) is employed in some regulatory contexts.
Barbara L. Parsons+17 more
wiley +1 more source