Skip to content
DraconiticResearch
Search Sources API
197,768 studies31 sourcesUpdated 3 min ago
PreprintarXiv licencearXiv

Nonthermal Particle Acceleration by Magnetic Pumping in Pulsating Plasmas

Abstract

We present a new pulsating box setup to investigate particle acceleration in high-beta plasmas undergoing compression--expansion cycles. Our fully kinetic simulations show that particles are efficiently accelerated by magnetic pumping, producing nonthermal energy distributions with power-law tails. Numerical results are in excellent agreement with a generalized maximum entropy model that we derive, linking the power-law index of distributions to the injected energy. Our results could be relevant for understanding the origin of high-energy particles in certain high-beta space and astrophysical plasmas.

Related

  1. Guide field effects on particle acceleration in three-dimensional relativistic magnetic reconnection
    Despina Karavola, Lorenzo Sironi, Maria Petropoulou
    arXivPreprintarXiv licenceFull textHigh-energy astrophysicsPlasma physicsarXiv
  2. Direct Observational Constraint on Upstream Magnetic Field Amplification Reveals the Particle Acceleration Limit in a Supernova Remnant
    Yuya Kawabata, Takaaki Tanaka, Hiromasa Suzuki +1
    arXivPreprintarXiv licenceFull textHigh-energy astrophysicsarXiv
  3. Energetic Nonthermal Electrons within the Above-the-looptop Regions in Solar Flares: Acceleration, Feedback, and Quasi-Periodic Pulsations
    Jeongbhin Seo, Fan Guo, Xiaocan Li +3
    arXivPreprintCC BY 4.0Full textHigh-energy astrophysicsSolar & stellar physicsarXiv
  4. Aditya-L1 and SDO Observations of a Confined X-Class Flare with an EUV Late Phase: Thermal and Nonthermal Emission, Magnetic Topology, and Flux Rope Confinement
    Vishwa Vijay Singh, Bhuwan Joshi, N. P. S. Mithun
    arXivPreprintCC BY 4.0Full textSolar & stellar physicsarXiv
  5. Aditya-L1 and SDO Observations of a Confined X-Class Flare with an EUV Late Phase: Thermal and Nonthermal Emission, Magnetic Topology, and Flux Rope Confinement
    Vishwa Vijay Singh, Bhuwan Joshi, N.P.S. Mithun
    The Astrophysical JournalPeer-reviewedCC BY 4.0Full textSolar & stellar physicsCrossref
BibTeX
@misc{arro2026nonthermal,
  title = {{Nonthermal Particle Acceleration by Magnetic Pumping in Pulsating Plasmas}},
  author = {Giuseppe Arrò and Vladimir Zhdankin and Fabio Bacchini},
  howpublished = {arXiv},
  year = {2026},
  month = oct,
  doi = {10.48550/arxiv.2606.05286},
  eprint = {2606.05286},
  archivePrefix = {arXiv},
  url = {https://arxiv.org/abs/2606.05286},
}
RIS
TY  - UNPB
TI  - Nonthermal Particle Acceleration by Magnetic Pumping in Pulsating Plasmas
AU  - Giuseppe Arrò
AU  - Vladimir Zhdankin
AU  - Fabio Bacchini
PY  - 2026
DA  - 2026/10/26
PB  - arXiv
DO  - 10.48550/arxiv.2606.05286
UR  - https://arxiv.org/abs/2606.05286
AB  - We present a new pulsating box setup to investigate particle acceleration in high-beta plasmas undergoing compression--expansion cycles. Our fully kinetic simulations show that particles are efficiently accelerated by magnetic pumping, producing nonthermal energy distributions with power-law tails. Numerical results are in excellent agreement with a generalized maximum entropy model that we derive, linking the power-law index of distributions to the injected energy. Our results could be relevant for understanding the origin of high-energy particles in certain high-beta space and astrophysical plasmas.
ER  -