Relativistic Magnetized Electron–Positron Quantum Plasma and Large-Amplitude Solitary Electromagnetic Waves

Author(s):  
F. Nooralishahi ◽  
M. K. Salem
2004 ◽  
Vol 11 (6) ◽  
pp. 3078-3082 ◽  
Author(s):  
Frank Verheest ◽  
Tom Cattaert

1989 ◽  
Vol 152 (2) ◽  
pp. 181-190 ◽  
Author(s):  
F. B. Rizzato ◽  
R. S. Schneider ◽  
D. Dillenburg

1997 ◽  
Vol 50 (2) ◽  
pp. 309 ◽  
Author(s):  
Y. N. Nejoh

The nonlinear wave structures of large amplitude ion-acoustic waves are studied in a plasma with positrons. We have presented the region of existence of the ion-acoustic waves by analysing the structure of the pseudopotential. The region of existence sensitively depends on the positron to electron density ratio, the ion to electron mass ratio and the positron to electron temperature ratio. It is shown that the maximum Mach number increases as the positron temperature increases and the region of existence of the ion-acoustic waves spreads as the positron temperature increases. The present theory is applicable to analyse large amplitude ion-acoustic waves associated with positrons which may occur in space plasmas.


2013 ◽  
Vol 20 (8) ◽  
pp. 082123 ◽  
Author(s):  
S. M. Khorashadizadeh ◽  
E. Rastbood ◽  
H. Zeinaddini Meymand ◽  
A. R. Niknam

2021 ◽  
Vol 2021 (7) ◽  
Author(s):  
Wan Zhen Chua ◽  
Niayesh Afshordi

Abstract We compute the albedo (or reflectivity) of electromagnetic waves off the electron-positron Hawking plasma that surrounds the horizon of a Quantum Black Hole. We adopt the “modified firewall conjecture” for fuzzballs [1, 2], where we consider significant electromagnetic interaction around the horizon. While prior work has treated this problem as an electron-photon scattering process, we find that the incoming quanta interact collectively with the fermionic excitations of the Hawking plasma at low energies. We derive this via two different methods: one using relativistic plasma dispersion relation, and another using the one-loop correction to photon propagator. Both methods find that the reflectivity of long wavelength photons off the Hawking plasma is significant, contrary to previous claims. This leads to the enhancement of the electromagnetic albedo for frequencies comparable to the Hawking temperature of black hole horizons in vacuum. We comment on possible observable consequences of this effect.


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