… of particle acceleration to high energies in the shock waves of supernova remnants. This …
It is worth noting that if proton acceleration is age-limited and electron acceleration is loss-…

… electrons are accelerated through all these orders of magnitude in energy up to the injection
energy where they continue to be accelerated … responsible for electron energization, which …

… supernova remnants, covering the whole electromagnetic spectrum and describe what these
observations tell us about the acceleration … Also, X-ray synchrotron emitting TeV electrons …

… diffusive shock acceleration, we model the total spectrum of cosmic ray (CR) electrons
accelerated by supernova remnants (SNRs). Because electrons experience synchrotron losses in …

… Here we report X-ray observations of the remnant of supernova 1006, made by the ASCA …
edges of the remnant shell is dominated by radiation from electrons accelerated to energies of …

… that synchrotron radiation from these electrons would in fact not be … Fermi acceleration, and
compare them with the observed radio spectra of Tycho's and Kepler's supernova remnants. …

… –t the local electron —ux up to 1 TeV), we show that an electron injection index of … electron
spectrum and (2) explain the above-mentioned gamma-ray excess above 1 GeV. An electron …

… For the shock speed v s < 4,500 km s -1 , as derived in this work, the acceleration time of
electrons responsible for X-rays significantly exceeds the timescales of the observed X-ray …

… acceleration—can be a clue for solution of the well known theoretical problem of electron
injection in supernova remnants. In … adequate number of energetic electrons and positrons for …

… shock, turbulence subjects electrons to stochastic re-acceleration. On … acceleration at z
= 0 provides accelerated electrons that are fed into the orange-shaded region of re-acceleration …