M.Patil:Over-spinning Kerr geometry and UHECR
Posted: Fri 4 Mar 2016 18:25VIA lecture by Prof. Mandar Patil ''Can over-spinning Kerr geometry be the source of ultra-high-energy cosmic rays and neutrinos ?'' was given on 04.03.2016. It's presentation is attached and the record is in VIA library
http://viavca.in2p3.fr/mandar_patil.html
The following questions were put in the Discussion:
Shantanu: so can you get this acceleration given the observed spins from the LIGO detection? Since the spins were less than 1.
Mandar: Acceleration is not possible if spins are less than one. Spin has to be larger than one
Shantanu: so presumably LIGO should be able to detect a population of black holes with spin > 1 as evidence for your model?
You are welcome to continue discussion in replies to this post.
http://viavca.in2p3.fr/mandar_patil.html
The following questions were put in the Discussion:
Shantanu: so can you get this acceleration given the observed spins from the LIGO detection? Since the spins were less than 1.
Mandar: Acceleration is not possible if spins are less than one. Spin has to be larger than one
Shantanu: so presumably LIGO should be able to detect a population of black holes with spin > 1 as evidence for your model?
You are welcome to continue discussion in replies to this post.