Cosmic ray acceleration by shocks: spectral steepening due to turbulent magnetic field amplification
Monthly Notices of the Royal Astronomical Society Oxford University Press 488*:2 (2019) 2466-2472
Abstract:
We show that the energy required to turbulently amplify magnetic field during cosmic ray (CR) acceleration by shocks extracts energy from the CR and steepens the CR energy spectrum.Prospects for the Use of Photosensor Timing Information with Machine Learning Techniques in Background Rejection.
Sissa Medialab Srl (2019) 798
Synchrotron self absorption and the minimum energy of optically thick radio flares from stellar mass black holes
(2019)
Mass and spin measurements for the neutron star 4U1608−52 through the relativistic precession model
Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 486:4 (2019) 4485-4497
Prospects for the Use of Photosensor Timing Information with Machine Learning Techniques in Background Rejection
(2019)