Unraveling the Effects of Dense Medium on a Near to Bohm-Limit Acceleration in Kepler's SNR
Unraveling the Effects of Dense Medium on a Near to Bohm-Limit Acceleration in Kepler's SNR
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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The maximum energy of electrons accelerated by supernova remnants (SNR) is typically limited by radiative losses. In this scenario, the synchrotron cooling time scale is equal to the acceleration time scale. On the other hand, the low propagation speed of a shock in a dense medium is expected to result in an extended acceleration time scale, thus i...
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Unraveling the Effects of Dense Medium on a Near to Bohm-Limit Acceleration in Kepler's SNR
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TN_cdi_proquest_journals_2858093276
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2858093276
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2308.13435
