Weakly interacting massive particle diffusion in the solar system including solar depletion and its effect on Earth capture rates

Physical Review D - Particles, Fields, Gravitation and Cosmology

Volumn 69, Issue 12, 2004, Pages

  Lundberg, Johan ^a   Edsjö, Joakim ^b  

^a UPPSALA UNIVERSITY   (Sweden)

^b ALBANOVA UNIVERSITY CENTER   (Sweden)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 37649029522     PISSN: 15507998     EISSN: 15502368     Source Type: Journal    
DOI: 10.1103/PhysRevD.69.123505     Document Type: Article

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35. It is unclear if Venus has a liquid iron core or not. Our results are not sensitive to this, and we choose a model with only a solid iron core.
36. Note that if du is not small, the volume of the cell is not (Formula presented) but (Formula presented) When numerical values are called for, we use the latter expression for accurate results.
37. We introduce the velocity distribution (Formula presented) here to be as close as possible to Gould’s expressions. This distribution is related to (Formula presented) in Sec. II A through (Formula presented)