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A recently proposed mechanism of acceleration of highest energy cosmic rays by polarization electric fields arising in plasmoids injected into neutron star magnetospheres is discussed.

天体物理学 · 物理学 2009-11-06 C. Litwin , R. Rosner

The available data on isolated X-ray pulsars, their wind nebulae, and the supernova remnants which are connected to some of these sources are analyzed. It is shown that electric fields of neutron stars tear off charged particles from the…

天体物理学 · 物理学 2009-11-13 Sevinc O. Tagieva , Askin Ankay , Arzu M. Ankay

The available data of single X-ray pulsars, their wind nebulae, and the SNRs which are connected to some of these sources are analysed. It is shown that electric field intensity of neutron stars tears off charged particles from the surface…

天体物理学 · 物理学 2007-05-23 Oktay H. Guseinov , Askin Ankay , Sevinc O. Tagieva

Particle acceleration at plasma shocks appears to be ubiquitous in the universe, spanning systems in the heliosphere, supernova remnants, and relativistic jets in distant active galaxies and gamma-ray bursts. This review addresses some of…

天体物理学 · 物理学 2008-11-26 Matthew G. Baring

Theoretical concepts ofn cosmic ray particle acceleration at relativistic plasma flows -- shocks and shear layers -- are reviewed. We begin with a discussion of mildly relativistic shock waves. The role of oblique field configurations and…

天体物理学 · 物理学 2007-05-23 M. Ostrowski

The acceleration of ultra high energy cosmic rays is conjectured to occur through various interactions with the electromagnetic fields in different astrophysical objects, like magnetic matter clumps, besides the well-known shock and…

高能天体物理现象 · 物理学 2014-03-18 A. Tawfik , A. Saleh , M. T. Ghoneim , A. A. Hady

The acceleration of charged particles at astrophysical collisionless shock waves is one of the best studied processes for the energization of particles to ultrarelativistic energies, required by multifrequency observations in a variety of…

天体物理学 · 物理学 2009-11-10 Pasquale Blasi

We investigate acceleration of cosmic rays by shocks and accretion flows in galaxy clusters. Numerical results for spectra of accelerated particles and nonthermal emission are presented. It is shown that the acceleration of protons and…

高能天体物理现象 · 物理学 2019-05-22 V. N. Zirakashvili , V. S. Ptuskin

Charged particles at the crust of compact stars may be ejected and accelerated by the electric field generated due to the rotation of the magnetized star. For neutron or hybrid stars, the negatively charged particles are usually electrons,…

高能天体物理现象 · 物理学 2020-10-28 Debojoti Kuzur , Rupamoy Bhattacharyya , Ritam Mallick

The highest energy cosmic rays observed possess macroscopic energies and their origin is likely to be associated with the most energetic processes in the Universe. Their existence triggered a flurry of theoretical explanations ranging from…

高能物理 - 唯象学 · 物理学 2014-11-17 Guenter Sigl

The description of the transport of cosmic rays in magnetized media is central to both acceleration and propagation of these particles in our Galaxy and outside. The investigation of the process of particle acceleration, especially at shock…

高能天体物理现象 · 物理学 2017-03-21 P. Blasi

Cosmic rays are often modeled as charged particles. This allows their non-ballistic propagation in magnetized structures to be captured. In certain situations, a neutral cosmic ray component can arise. For example, cosmic ray neutrons are…

高能天体物理现象 · 物理学 2025-04-23 Ellis R. Owen , Yoshiyuki Inoue , Tatsuki Fujiwara , Qin Han , Kinwah Wu

We consider the diffusive shock acceleration in interstellar bubbles created by powerful stellar winds of supernova progenitors. Under the moderate stellar wind magnetization the bubbles are filled by the strongly magnetized low density…

高能天体物理现象 · 物理学 2018-02-14 V. N. Zirakashvili , V. S. Ptuskin

Spin-polarized particle beams are of interest for applications like deep-inelastic scattering, e.g. to gain further understanding of the proton's nuclear structure. With the advent of high-intensity laser facilities, laser-plasma-based…

等离子体物理 · 物理学 2025-11-06 Lars Reichwein , Zheng Gong , Chuan Zheng , Liangliang Ji , Alexander Pukhov , Markus Büscher

Based on the generic acceleration model, which suggests different types of electromagnetic interactions between the cosmic charged particles and the different configurations of the electromagnetic (plasma) fields, the ultra high energy…

高能天体物理现象 · 物理学 2014-03-21 A. Tawfik , A. Saleh , M. T. Ghoneim , A. Hady

The origin of the highest energy cosmic rays is still unknown. The discovery of their sources will reveal the workings of the most energetic astrophysical accelerators in the universe. Current observations show a spectrum consistent with an…

高能天体物理现象 · 物理学 2015-05-27 Kumiko Kotera , Angela V. Olinto

The enhanced star forming activity, typical of starburst galaxies, powers strong galactic winds expanding on kiloparsec (kpc) scales and characterized by bubble structures. Here we discuss the possibility that particle acceleration may take…

高能天体物理现象 · 物理学 2022-02-15 Enrico Peretti , Giovanni Morlino , Pasquale Blasi , Pierre Cristofari

Strong magnetic fields and plasmas are intrinsically linked in both terrestrial laboratory experiments and in space phenomena. One of the most profound consequences of that is the change in relationship between the frequency and the wave…

Pulsars have been identified as good candidates for the acceleration of cosmic rays, up to ultra-high energies. However, a precise description of the acceleration processes at play is still to be established. Using 2D particle-in-cell…

高能天体物理现象 · 物理学 2020-03-25 C. Guépin , B. Cerutti , K. Kotera

We review the physics of the highest energy cosmic rays. The discovery of their sources, still unknown, will reveal the most energetic astrophysical objects in the universe and could unveil new physics beyond the standard model of particle…

高能天体物理现象 · 物理学 2017-11-30 Roberto Aloisio
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