Suppression of pair beam instabilities in a laboratory analogue of blazar pair cascades

Fuente: arXiv
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Autores principales: Arrowsmith, Charles D., Miniati, Francesco, Bilbao, Pablo J., Simon, Pascal, Bott, Archie F. A., Burger, Stephane, Chen, Hui, Cruz, Filipe D., Davenne, Tristan, Dyson, Anthony, Efthymiopoulos, Ilias, Froula, Dustin H., Goillot, Alice, Gudmundsson, Jon T., Haberberger, Dan, Halliday, Jack W. D., Hodge, Tom, Huffman, Brian T., Iaquinta, Sam, Marshall, G., Reville, Brian, Sarkar, Subir, Schekochihin, Alexander A., Silva, Luis O., Simpson, Raspberry, Stergiou, Vasiliki, Trines, Raoul M. G. M., Vieu, Thibault, Charitonidis, Nikolaos, Bingham, Robert, Gregori, Gianluca
Formato: Preprint
Publicado: 2025
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author Arrowsmith, Charles D.
Miniati, Francesco
Bilbao, Pablo J.
Simon, Pascal
Bott, Archie F. A.
Burger, Stephane
Chen, Hui
Cruz, Filipe D.
Davenne, Tristan
Dyson, Anthony
Efthymiopoulos, Ilias
Froula, Dustin H.
Goillot, Alice
Gudmundsson, Jon T.
Haberberger, Dan
Halliday, Jack W. D.
Hodge, Tom
Huffman, Brian T.
Iaquinta, Sam
Marshall, G.
Reville, Brian
Sarkar, Subir
Schekochihin, Alexander A.
Silva, Luis O.
Simpson, Raspberry
Stergiou, Vasiliki
Trines, Raoul M. G. M.
Vieu, Thibault
Charitonidis, Nikolaos
Bingham, Robert
Gregori, Gianluca
author_facet Arrowsmith, Charles D.
Miniati, Francesco
Bilbao, Pablo J.
Simon, Pascal
Bott, Archie F. A.
Burger, Stephane
Chen, Hui
Cruz, Filipe D.
Davenne, Tristan
Dyson, Anthony
Efthymiopoulos, Ilias
Froula, Dustin H.
Goillot, Alice
Gudmundsson, Jon T.
Haberberger, Dan
Halliday, Jack W. D.
Hodge, Tom
Huffman, Brian T.
Iaquinta, Sam
Marshall, G.
Reville, Brian
Sarkar, Subir
Schekochihin, Alexander A.
Silva, Luis O.
Simpson, Raspberry
Stergiou, Vasiliki
Trines, Raoul M. G. M.
Vieu, Thibault
Charitonidis, Nikolaos
Bingham, Robert
Gregori, Gianluca
contents The generation of dense electron-positron pair beams in the laboratory can enable direct tests of theoretical models of $γ$-ray bursts and active galactic nuclei. We have successfully achieved this using ultra-relativistic protons accelerated by the Super Proton Synchrotron at CERN. In the first application of this experimental platform, the stability of the pair beam is studied as it propagates through a metre-length plasma, analogous to TeV $γ$-ray induced pair cascades in the intergalactic medium. It has been argued that pair beam instabilities disrupt the cascade, thus accounting for the observed lack of reprocessed GeV emission from TeV blazars. If true this would remove the need for a moderate strength intergalactic magnetic field to explain the observations. We find that the pair beam instability is suppressed if the beam is not perfectly collimated or monochromatic, hence the lower limit to the intergalactic magnetic field inferred from $γ$-ray observations of blazars is robust.
format Preprint
id arxiv_https___arxiv_org_abs_2509_09040
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Suppression of pair beam instabilities in a laboratory analogue of blazar pair cascades
Arrowsmith, Charles D.
Miniati, Francesco
Bilbao, Pablo J.
Simon, Pascal
Bott, Archie F. A.
Burger, Stephane
Chen, Hui
Cruz, Filipe D.
Davenne, Tristan
Dyson, Anthony
Efthymiopoulos, Ilias
Froula, Dustin H.
Goillot, Alice
Gudmundsson, Jon T.
Haberberger, Dan
Halliday, Jack W. D.
Hodge, Tom
Huffman, Brian T.
Iaquinta, Sam
Marshall, G.
Reville, Brian
Sarkar, Subir
Schekochihin, Alexander A.
Silva, Luis O.
Simpson, Raspberry
Stergiou, Vasiliki
Trines, Raoul M. G. M.
Vieu, Thibault
Charitonidis, Nikolaos
Bingham, Robert
Gregori, Gianluca
High Energy Astrophysical Phenomena
Plasma Physics
The generation of dense electron-positron pair beams in the laboratory can enable direct tests of theoretical models of $γ$-ray bursts and active galactic nuclei. We have successfully achieved this using ultra-relativistic protons accelerated by the Super Proton Synchrotron at CERN. In the first application of this experimental platform, the stability of the pair beam is studied as it propagates through a metre-length plasma, analogous to TeV $γ$-ray induced pair cascades in the intergalactic medium. It has been argued that pair beam instabilities disrupt the cascade, thus accounting for the observed lack of reprocessed GeV emission from TeV blazars. If true this would remove the need for a moderate strength intergalactic magnetic field to explain the observations. We find that the pair beam instability is suppressed if the beam is not perfectly collimated or monochromatic, hence the lower limit to the intergalactic magnetic field inferred from $γ$-ray observations of blazars is robust.
title Suppression of pair beam instabilities in a laboratory analogue of blazar pair cascades
topic High Energy Astrophysical Phenomena
Plasma Physics
url https://arxiv.org/abs/2509.09040