scholarly journals Perturbation theory calculation of the black hole elastic scattering cross section

2002 ◽  
Vol 66 (2) ◽  
Author(s):  
Chris Doran ◽  
Anthony Lasenby
Keyword(s):  
Black Hole ◽  
Perturbation Theory ◽  
Elastic Scattering ◽  
Cross Section ◽  
Scattering Cross Section ◽  
Scattering Cross ◽  
Elastic Scattering Cross Section ◽  
Theory Calculation

scholarly journals New measurement of the elastic scattering cross section of μd muonic atoms off deuterons

1979 ◽  
Vol 85 (4) ◽  
pp. 458-462 ◽  
Author(s):  
A. Bertin ◽  
I. Massa ◽  
M. Piccinini ◽  
A. Vacchi ◽  
G. Vannini ◽  
...  
Keyword(s):  
Elastic Scattering ◽  
Cross Section ◽  
Scattering Cross Section ◽  
Muonic Atoms ◽  
Scattering Cross ◽  
Elastic Scattering Cross Section

scholarly journals INTERPRETING THE BOUNDS ON SOLAR DARK MATTER INDUCED MUONS AT SUPER-KAMIOKANDE IN THE LIGHT OF CDMS RESULTS

2010 ◽  
Vol 25 (18n19) ◽  
pp. 3741-3747
Author(s):  
ABHIJIT BANDYOPADHYAY ◽  
SOVAN CHAKRABORTY ◽  
DEBASISH MAJUMDAR
Keyword(s):  
Dark Matter ◽  
Elastic Scattering ◽  
Cross Section ◽  
Enhancement Factor ◽  
Scattering Cross Section ◽  
The Sun ◽  
Detection Rates ◽  
Scattering Cross ◽  
Elastic Scattering Cross Section ◽  
Upper Limits

We consider the recent limits on dark matter–nucleon elastic scattering cross-section from the analysis of CDMS II collaboration using the two signal events observed in CDMS experiment. With these limits we try to interpret the super-Kamiokande (SK) bounds on the detection rates of up-going muons induced by the neutrinos that are produced in the sun from the decay of annihilation products of dark matter (WIMP's) captured in the solar core. Calculated rates of up-going muons for different annihilation channels at SK using CDMS bounds are found to be orders below the predicted upper limits of such up-going muon rates at SK. Thus there exists room for enhancement (boost) of the calculated rates using CDMS limits for interpreting SK bounds. Such a feature is expected to represent the PAMELA data with the current CDMS limits. We also show the dependence of such a possible enhancement factor (boost) on WIMP mass for different WIMP annihilation channels.

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