The interaction of cosmic rays and magnetized plasma

By A. Bell. 2005

173 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/6f19e6272001f2cd9e081a6b720b9f4d335e3739

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. A. Spitkovsky
2. D. Caprioli
3. P. Blasi
4. J. Arons
5. A. Bret
6. L. Sironi
7. D. Ellison
8. A. Bykov

In Nuclear and High Energy Physics

1. A. Spitkovsky
2. D. Caprioli
3. P. Blasi
4. J. Arons
5. A. Bret
6. L. Sironi
7. D. Ellison
8. A. Bykov

Citations in the corpus

• Observational Signatures of Particle Acceleration in Supernova Remnants (2012, methodology): “Magnetic-field amplification mechanisms due to CR instabilities in nonlinear diffusive shock acceleration were proposed recently by several studies Bell (2004, 2005); Amato and Blasi (2006); Vladimirov et al. (2006); Marcowith et al. (2006); Vladimirov et al. (2009); Zirakashvili and Ptuskin…”
• SIMULATIONS OF ION ACCELERATION AT NON-RELATIVISTIC SHOCKS. II. MAGNETIC FIELD AMPLIFICATION (2014, background): “However, there is a short-wavelength instability (the non-resonant hybrid, NRH, instability; Bell 2004, 2005) that is predicted to grow faster than the resonant one.”
• NONLINEAR STUDY OF BELL'S COSMIC RAY CURRENT-DRIVEN INSTABILITY (2008, background): “The MHD studies (Bell 2004, 2005; Zirakashvili et al. 2008) have shown a substantial amplification of the ambient magnetic field and the formation of turbulence, which is characterized by prominent density fluctuations in the plasma.”
• Non-linear particle acceleration at non-relativistic shock waves in the presence of self-generated turbulence (2006, background): “An important role in explaining this level of amplification could be played by different versions of the streaming instability (Bell & Lucek (2001); Bell (2004, 2005)), not requiring resonant interactions of particles and waves.”
• The origin of galactic cosmic rays (2013, unknown): “Bell (2004, 2005) noticed that when the condition in Eq.”
• Cosmic ray acceleration and escape from supernova remnants (2013, background): “…shock acceleration as an explanation of the Galactic spectrum until it was shown that a plasma instability driven by streaming CR in the upstream precursor could amplify the magnetic field ahead of the shock and facilitate rapid acceleration to higher energies (Lucek & Bell 2000, Bell 2004, 2005).”
• Nonlinear Diffusive Shock Acceleration with Magnetic Field Amplification (2006, methodology): “…with B-Field Amplification Besides the limited results from PIC simulations, the only models of magnetic field generation with B3B0 in nonlinear DSA that we are aware of are the semianalytic results of Bell & Lucek (2001), Bell (2004, 2005), Ptuskin & Zirakashvili (2003), and Amato & Blasi (2006).”
• Cosmic-ray acceleration in supernova remnants: non-linear theory revised (2012, background): “18) which may play a relevant role, like for instance the excitation of Bell’s non-resonant modes [52, 53], or the development of large scales structures due to fire-hose instability [54, 55], which may be most effective where the CR distribution function is most anisotropic, i.”
• WEIBEL, TWO-STREAM, FILAMENTATION, OBLIQUE, BELL, BUNEMAN...WHICH ONE GROWS FASTER? (2009, methodology): “These modes are the present configuration analogs to the ones explained by Bell (2004, 2005).”
• Long-Term Evolution of Magnetic Turbulence in Relativistic Collisionless Shocks: Electron-Positron Plasmas (2007, background): “This is a relativistic version of Bell’s (1978) (also see Bell 2004, 2005) picture of particle acceleration in non-relativistic shocks.”