Underdense relativistically thermal plasma produced by magnetically assisted direct laser acceleration
Underdense relativistically thermal plasma produced by magnetically assisted direct laser acceleration
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DOI:
10.1103/physrevresearch.4.l042017
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发表时间:
2022-02
影响因子:
4.2
通讯作者:
K. Weichman;J. Palastro;A. Robinson;R. Bingham;A. Arefiev
中科院分区:
文献类型:
--
作者:
K. Weichman;J. Palastro;A. Robinson;R. Bingham;A. Arefiev
The discovery of special relativity in 1905 transformed the fields of electromagnetism and charged-particle kinetics that, some 20 years later, would coalesce into the field of plasma physics. Predictions have continually emphasized the importance of special relativity in plasmas where the majority of electrons are relativistic regardless of reference frame, but, even today, experimental verifications of these predictions remain relatively rare. The laboratory generation of these relativistically thermal plasmas is needed to address open questions in astrophysics regarding shock acceleration and the origin of cosmic rays, 1 fast radio bursts, 2,3 and c -ray bursts. 4 Relativistically thermal plasmas also feature a substantially modified response to electromagnetic radiation relative to the nonrelativistic or nonthermal cases, which is of significant interest in basic plasma physics, 5 laboratory astrophysics, 6,7 and laser-plasma physics. 8–11 m few-hundred-micron spot size and 50-fs/multipicosecond duration. approach is thereby anticipated to offer the practical access to the relativistically thermal plasma regime, enabling experimental verification of longstanding, foundational predictions in basic plasma physics, laboratory astrophysics, and laser-plasma physics.