2022
DOI: 10.1088/1674-1137/ac4704
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Implications of gamma-ray photon measurements at the LHAASO on Lorentz symmetry *

Abstract: The Large High Altitude Air Shower Observatory (LHAASO) has reported the measurement of photons with high energy up to 1.42 PeV from 12 gamma-ray sources. We are concerned with the implications of LHAASO data on the fate of Lorenz symmetry at such high energy level, thus we consider the interaction of the gamma ray with those photons in cosmic microwave background (CMB), and compute the optical depth, the mean free path as well as the survival probability for photons from all these gamma-ray sources. Employing… Show more

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Cited by 2 publications
(3 citation statements)
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“…This comparison indicates that a few illuminated clouds are possibly within the reach of CTA already with 50 hr of observations. However, one should consider that a degradation of performances is expected when observing extended sources, mostly because of the increased background rate involved in the analysis, as investigated in [22] for a different configuration of CTA telescopes adopted in the past. The molecular clouds under investigation are on average extended structures for both CTA and LHAASO, though the larger point spread function of the latter might mitigate the impact of sensitivity worsening.…”
Section: Pos(icrc2023)775mentioning
confidence: 99%
See 1 more Smart Citation
“…This comparison indicates that a few illuminated clouds are possibly within the reach of CTA already with 50 hr of observations. However, one should consider that a degradation of performances is expected when observing extended sources, mostly because of the increased background rate involved in the analysis, as investigated in [22] for a different configuration of CTA telescopes adopted in the past. The molecular clouds under investigation are on average extended structures for both CTA and LHAASO, though the larger point spread function of the latter might mitigate the impact of sensitivity worsening.…”
Section: Pos(icrc2023)775mentioning
confidence: 99%
“…These continuous accelerators might in fact provide, during a lifetime of several million years, comparable energetics with respect to SNR outputs: in fact, in order to sustain an average wind luminosity of 3×10 37 erg/s for 10 6 yr, an energy injection of 10 51 erg is needed, similarly to the kinetic energy release of SuperNova (SN) explosions. Besides energetic considerations, acceleration of particles from the wind of massive stars appears to be a necessary component to explain the 22 Ne/ 20 Ne anomaly in CR composition [1]: the enhancement observed with respect to Solar abundances requires acceleration from a carbon-enriched medium rather than from the standard interstellar medium (ISM), e.g. from the wind of Wolf-Rayet stars.…”
Section: Introductionmentioning
confidence: 99%
“…Detailed morphological and spectral analysis suggest a continuous injection of possible hadronic origin [4,5]. The Cygnus cocoon has even been observed at the highest energies ever probed by gamma-ray astronomy: a 1.4 PeV photon was detected from LHAASO [7], strengthen the idea that stellar clusters may act as PeVatrons.…”
Section: Introductionmentioning
confidence: 99%