Cosmic-Ray Acceleration in Supernova Remnants.

Astrophysical studies makes possible to use natural cosmic objects as unique particle laboratories. Effects of new physics in cosmic rays and electromagnetic radiation, in stars and galaxies, indirect effects of dark matter , in particular, are the subjects of this topic of Forum

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Cosmic-Ray Acceleration in Supernova Remnants.

New postby Maxim Khlopov on Fri 4 May 2012 20:12

APC Colloquium on 4 May 2012
Prof. Patrick Slane (CfA, Harvard University, USA)
"Cosmic-Ray Acceleration in Supernova Remnants."
Distant participants put their questions and comments with the use of VIA system
APC:Please, questions
APC:Comments?
Fabo Feng:Very good presentation. I have a question about the Inverse compton scattering process of the CMB photon.
APC:Please
Fabo Feng:Can we reveal the CMB temperature from the spectrum?
Michael De Becker:Very nice talk! Thanks for the organization. Bye!
Attachments
snr_cr2.pdf
Presentation of P.Slane's talk
(10.64 MiB) Downloaded 192 times
[i]Хлопов Максим Юрьевич
Maxim Khlopov[/i]
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