Zobrazeno 1 - 10
of 117
pro vyhledávání: '"Kilian, Patrick"'
Autor:
Rassel, Mohira, Kilian, Patrick, Aberham, Vito, Spanier, Felix, Lloyd-Ronning, Nicole, Fryer, Chris L.
The electromagnetic emission from neutron star mergers is comprised of multiple components. Synchrotron emission from the disk-powered jet as well as thermal emission from the merger ejecta (powered by a variety of sources) are among the most studied
Externí odkaz:
http://arxiv.org/abs/2305.12008
Autor:
Guo, Fan, Li, Xiaocan, French, Omar, Daughton, William, Matthaeus, William, Zhang, Qile, Liu, Yi-Hsin, Kilian, Patrick, Johnson, Grant, Li, Hui
Recently, Sironi (PRL, 128, 145102; S22) reported the correlation between particles accelerated into high energy and their crossings of regions with electric field larger than magnetic field (E>B regions) in kinetic simulations of relativistic magnet
Externí odkaz:
http://arxiv.org/abs/2208.03435
Particle acceleration during magnetic reconnection is a long-standing topic in space, solar and astrophysical plasmas. Recent 3D particle-in-cell simulations of magnetic reconnection show that particles can leave flux ropes due to 3D field-line chaos
Externí odkaz:
http://arxiv.org/abs/2205.08600
An oblique-rotating pulsar generates a relativistic striped wind in a pulsar wind nebula (PWN). The termination shock of the PWN compresses the Poynting-flux-dominated flow and drives magnetic reconnection. By carrying out particle-in-cell (PIC) simu
Externí odkaz:
http://arxiv.org/abs/2010.14089
Magnetic reconnection is a ubiquitous plasma process in which oppositely directed magnetic field lines break and rejoin, resulting in a change of the magnetic field topology. Reconnection generates magnetic islands: regions enclosed by magnetic field
Externí odkaz:
http://arxiv.org/abs/2010.01959
Autor:
Guo, Fan, Li, Xiaocan, Daughton, William, Li, Hui, Kilian, Patrick, Liu, Yi-Hsin, Zhang, Qile, Zhang, Haocheng
In strongly magnetized astrophysical plasma systems, magnetic reconnection is believed to be a primary process during which explosive energy release and particle acceleration occur, leading to significant high-energy emission. Past years have witness
Externí odkaz:
http://arxiv.org/abs/2008.02743
Magnetic reconnection in strongly magnetized astrophysical plasma environments is believed to be the primary process for fast energy release and particle energization. Currently there is strong interest in relativistic magnetic reconnection, in that
Externí odkaz:
http://arxiv.org/abs/2006.15288
A rotating pulsar creates a surrounding pulsar wind nebula (PWN) by steadily releasing an energetic wind into the interior of the expanding shockwave of supernova remnant or interstellar medium. At the termination shock of a PWN, the Poynting-flux-do
Externí odkaz:
http://arxiv.org/abs/2004.02277
The formation of collisionless shock fronts is an ubiquitous phenomenon in space plasma environments. In the solar wind shocks might accompany coronal mass ejections, while even more violent events, such as supernovae, produce shock fronts traveling
Externí odkaz:
http://arxiv.org/abs/2003.07293
Magnetic reconnection in the relativistic and trans-relativistic regimes is able to accelerate particles to hard power law energy spectra $f \propto \gamma^{-p}$ (approaching $p=1$). The underlying acceleration mechanism that determines the spectral
Externí odkaz:
http://arxiv.org/abs/2001.02732