Zobrazeno 1 - 10
of 1 635
pro vyhledávání: '"LEMOINE, M."'
Autor:
Lemoine, M., Rieger, F.
Recent results from the IceCube detector and their phenomenological interpretation suggest that the corona of nearby X-ray luminous Seyfert galaxies can produce $\sim 1-10\,$TeV neutrinos via photo-hadronic interactions. We investigate in detail the
Externí odkaz:
http://arxiv.org/abs/2412.01457
Autor:
Appiah, B., Dani, P., Ge, W., Hudson, C., Jain, S., Lemoine, M., Murphy, J., Murray, J., Pandikkadan, A., Schreve, K., Vo, H.
Genevois recently classified which graph braid groups on $\ge 3$ strands are word hyperbolic. In the $3$-strand case, he asked whether all such word hyperbolic groups are actually free; this reduced to checking two infinite classes of graphs: sun and
Externí odkaz:
http://arxiv.org/abs/2403.08623
Publikováno v:
Phys.Rev.D 109 (2024) 063006
In turbulent magnetized plasmas, charged particles can be accelerated to high energies through their interactions with the turbulent motions. As they do so, they draw energy from the turbulence, possibly up to the point where they start modifying the
Externí odkaz:
http://arxiv.org/abs/2312.04443
We simulate, using a particle-in-cell code, the chain of acceleration processes at work during the Compton-based interaction of a dilute electron-ion plasma with an extreme-intensity, incoherent gamma-ray flux with a photon density several orders of
Externí odkaz:
http://arxiv.org/abs/2309.00366
Autor:
Vanthieghem, A., Lemoine, M., Plotnikov, I., Grassi, A., Grech, M., Gremillet, L., Pelletier, G.
Weakly magnetized, relativistic collisionless shock waves are not only the natural offsprings of relativistic jets in high-energy astrophysical sources, they are also associated with some of the most outstanding displays of energy dissipation through
Externí odkaz:
http://arxiv.org/abs/2002.01141
Publikováno v:
Phys. Rev. E 100, 033209 (2019)
In this second paper of a series, we discuss the dynamics of a plasma entering the precursor of an unmagnetized, relativistic collisionless pair shock. We discuss how this background plasma is decelerated and heated through its interaction with a mic
Externí odkaz:
http://arxiv.org/abs/1907.08219
Publikováno v:
Physical Review E 100, 013205 (2019)
In this first paper of a series dedicated to the microphysics of unmagnetized, relativistic collisionless pair shocks, we discuss the physics of the Weibel-type transverse current filamentation instability (CFI) that develops in the shock precursor,
Externí odkaz:
http://arxiv.org/abs/1907.07750
We develop a comprehensive theoretical model of relativistic collisionless pair shocks mediated by the current filamentation instability. We notably characterize the noninertial frame in which this instability is of a mostly magnetic nature, and desc
Externí odkaz:
http://arxiv.org/abs/1907.07595