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Prospective constraints on Lorentz violation from ultrahigh-energy photon detection

We point out that violation of Lorentz invariance affects the interaction of high-energy photons with the Earth's atmosphere and magnetic field. In certain parameter region this interaction becomes suppressed and the photons escape observation passing through the atmosphere without producing ai...

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Autores principales: Rubtsov, Grigory, Satunin, Petr, Sibiryakov, Sergey
Lenguaje:eng
Publicado: 2013
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.89.123011
http://cds.cern.ch/record/1637253
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author Rubtsov, Grigory
Satunin, Petr
Sibiryakov, Sergey
author_facet Rubtsov, Grigory
Satunin, Petr
Sibiryakov, Sergey
author_sort Rubtsov, Grigory
collection CERN
description We point out that violation of Lorentz invariance affects the interaction of high-energy photons with the Earth's atmosphere and magnetic field. In certain parameter region this interaction becomes suppressed and the photons escape observation passing through the atmosphere without producing air showers. We argue that a detection of photon-induced air showers with energies above 10^19 eV, implying the absence of suppression as well as the absence of photon decay, will put tight double-sided limits on Lorentz violation in the sector of quantum electrodynamics. These constraints will be by several orders of magnitude stronger than the existing ones and will be robust against any assumptions about the astrophysical origin of the detected photons.
id cern-1637253
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2013
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spelling cern-16372532023-03-14T18:25:39Zdoi:10.1103/PhysRevD.89.123011http://cds.cern.ch/record/1637253engRubtsov, GrigorySatunin, PetrSibiryakov, SergeyProspective constraints on Lorentz violation from ultrahigh-energy photon detectionAstrophysics and AstronomyWe point out that violation of Lorentz invariance affects the interaction of high-energy photons with the Earth's atmosphere and magnetic field. In certain parameter region this interaction becomes suppressed and the photons escape observation passing through the atmosphere without producing air showers. We argue that a detection of photon-induced air showers with energies above 10^19 eV, implying the absence of suppression as well as the absence of photon decay, will put tight double-sided limits on Lorentz violation in the sector of quantum electrodynamics. These constraints will be by several orders of magnitude stronger than the existing ones and will be robust against any assumptions about the astrophysical origin of the detected photons.<p>We point out that violation of Lorentz invariance affects the interaction of high-energy photons with the Earth’s atmosphere and magnetic field. In a certain parameter region this interaction becomes suppressed and the photons escape observation, passing through the atmosphere without producing air showers. We argue that a detection of photon-induced air showers with energies above <inline-formula><mml:math display="inline"><mml:mrow><mml:mn>1</mml:mn><mml:msup><mml:mrow><mml:mn>0</mml:mn></mml:mrow><mml:mrow><mml:mn>19</mml:mn></mml:mrow></mml:msup><mml:mtext> </mml:mtext><mml:mtext> </mml:mtext><mml:mi>eV</mml:mi></mml:mrow></mml:math></inline-formula>, implying the absence of suppression as well as the absence of photon decay, will put tight double-sided limits on Lorentz violation in the sector of quantum electrodynamics. These constraints will be by several orders of magnitude stronger than the existing ones and will be robust against any assumptions about the astrophysical origin of the detected photons.</p>We point out that violation of Lorentz invariance affects the interaction of high-energy photons with the Earth's atmosphere and magnetic field. In certain parameter region this interaction becomes suppressed and the photons escape observation passing through the atmosphere without producing air showers. We argue that a detection of photon-induced air showers with energies above 10^19 eV, implying the absence of suppression as well as the absence of photon decay, will put tight double-sided limits on Lorentz violation in the sector of quantum electrodynamics. These constraints will be by several orders of magnitude stronger than the existing ones and will be robust against any assumptions about the astrophysical origin of the detected photons.arXiv:1312.4368CERN-PH-TH-2013-308CERN-PH-TH-2013-308oai:cds.cern.ch:16372532013-12-16
spellingShingle Astrophysics and Astronomy
Rubtsov, Grigory
Satunin, Petr
Sibiryakov, Sergey
Prospective constraints on Lorentz violation from ultrahigh-energy photon detection
title Prospective constraints on Lorentz violation from ultrahigh-energy photon detection
title_full Prospective constraints on Lorentz violation from ultrahigh-energy photon detection
title_fullStr Prospective constraints on Lorentz violation from ultrahigh-energy photon detection
title_full_unstemmed Prospective constraints on Lorentz violation from ultrahigh-energy photon detection
title_short Prospective constraints on Lorentz violation from ultrahigh-energy photon detection
title_sort prospective constraints on lorentz violation from ultrahigh-energy photon detection
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1103/PhysRevD.89.123011
http://cds.cern.ch/record/1637253
work_keys_str_mv AT rubtsovgrigory prospectiveconstraintsonlorentzviolationfromultrahighenergyphotondetection
AT satuninpetr prospectiveconstraintsonlorentzviolationfromultrahighenergyphotondetection
AT sibiryakovsergey prospectiveconstraintsonlorentzviolationfromultrahighenergyphotondetection