Exploring Lorentz Invariance Violation from Ultrahigh-Energy γ Rays Observed by LHAASO
dc.contributor.author | Cao Z. | |
dc.contributor.author | Aharonian F. | |
dc.contributor.author | An Q. | |
dc.contributor.author | Axikegu | |
dc.contributor.author | Bai L.X. | |
dc.contributor.author | Bai Y.X. | |
dc.contributor.author | Bao Y.W. | |
dc.contributor.author | Bastieri D. | |
dc.contributor.author | Bi X.J. | |
dc.contributor.author | Bi Y.J. | |
dc.contributor.author | Cai H. | |
dc.contributor.author | Cai J.T. | |
dc.contributor.author | Cao Z. | |
dc.contributor.author | Chang J. | |
dc.contributor.author | Chang J.F. | |
dc.contributor.author | Chen B.M. | |
dc.contributor.author | Chen E.S. | |
dc.contributor.author | Chen J. | |
dc.contributor.author | Chen L. | |
dc.contributor.author | Chen L. | |
dc.contributor.author | Chen M.J. | |
dc.contributor.author | Chen M.L. | |
dc.contributor.author | Chen Q.H. | |
dc.contributor.author | Chen S.H. | |
dc.contributor.author | Chen S.Z. | |
dc.contributor.author | Chen T.L. | |
dc.contributor.author | Chen X.L. | |
dc.contributor.author | Chen Y. | |
dc.contributor.author | Cheng N. | |
dc.contributor.author | Cheng Y.D. | |
dc.contributor.author | Cui S.W. | |
dc.contributor.author | Cui X.H. | |
dc.contributor.author | Cui Y.D. | |
dc.contributor.author | Piazzoli B.D.E. | |
dc.contributor.author | Dai B.Z. | |
dc.contributor.author | Dai H.L. | |
dc.contributor.author | Dai Z.G. | |
dc.contributor.author | Danzengluobu | |
dc.contributor.author | Della Volpe D. | |
dc.contributor.author | Dong X.J. | |
dc.contributor.author | Duan K.K. | |
dc.contributor.author | Fan J.H. | |
dc.contributor.author | Fan Y.Z. | |
dc.contributor.author | Fan Z.X. | |
dc.contributor.author | Fang J. | |
dc.contributor.author | Fang K. | |
dc.contributor.author | Feng C.F. | |
dc.contributor.author | Feng L. | |
dc.contributor.author | Feng S.H. | |
dc.contributor.author | Feng Y.L. | |
dc.contributor.author | Gao B. | |
dc.contributor.author | Gao C.D. | |
dc.contributor.author | Gao L.Q. | |
dc.contributor.author | Gao Q. | |
dc.contributor.author | Gao W. | |
dc.contributor.author | Ge M.M. | |
dc.contributor.author | Geng L.S. | |
dc.contributor.author | Gong G.H. | |
dc.contributor.author | Gou Q.B. | |
dc.contributor.author | Gu M.H. | |
dc.contributor.author | Guo F.L. | |
dc.contributor.author | Guo J.G. | |
dc.contributor.author | Guo X.L. | |
dc.contributor.author | Guo Y.Q. | |
dc.contributor.author | Guo Y.Y. | |
dc.contributor.author | Han Y.A. | |
dc.contributor.author | He H.H. | |
dc.contributor.author | He H.N. | |
dc.contributor.author | He J.C. | |
dc.contributor.author | He S.L. | |
dc.contributor.author | He X.B. | |
dc.contributor.author | He Y. | |
dc.contributor.author | Heller M. | |
dc.contributor.author | Hor Y.K. | |
dc.contributor.author | Hou C. | |
dc.contributor.author | Hou X. | |
dc.contributor.author | Hu H.B. | |
dc.contributor.author | Hu S. | |
dc.contributor.author | Hu S.C. | |
dc.contributor.author | Hu X.J. | |
dc.contributor.author | Huang D.H. | |
dc.contributor.author | Huang Q.L. | |
dc.contributor.author | Huang W.H. | |
dc.contributor.author | Huang X.T. | |
dc.contributor.author | Huang X.Y. | |
dc.contributor.author | Huang Z.C. | |
dc.contributor.author | Ji F. | |
dc.contributor.author | Ji X.L. | |
dc.contributor.author | Jia H.Y. | |
dc.contributor.author | Jiang K. | |
dc.contributor.author | Jiang Z.J. | |
dc.contributor.author | Jin C. | |
dc.contributor.author | Ke T. | |
dc.contributor.author | Kuleshov D. | |
dc.contributor.author | Levochkin K. | |
dc.contributor.author | Li B.B. | |
dc.contributor.author | Li C. | |
dc.contributor.author | Li C. | |
dc.contributor.author | Li F. | |
dc.contributor.author | Li H.B. | |
dc.contributor.other | Mahidol University | |
dc.date.accessioned | 2023-06-22T11:22:15Z | |
dc.date.available | 2023-06-22T11:22:15Z | |
dc.date.issued | 2022-02-04 | |
dc.description.abstract | Recently, the LHAASO Collaboration published the detection of 12 ultrahigh-energy γ-ray sources above 100 TeV, with the highest energy photon reaching 1.4 PeV. The first detection of PeV γ rays from astrophysical sources may provide a very sensitive probe of the effect of the Lorentz invariance violation (LIV), which results in decay of high-energy γ rays in the superluminal scenario and hence a sharp cutoff of the energy spectrum. Two highest energy sources are studied in this work. No signature of the existence of the LIV is found in their energy spectra, and the lower limits on the LIV energy scale are derived. Our results show that the first-order LIV energy scale should be higher than about 105 times the Planck scale MPl and that the second-order LIV scale is >10-3MPl. Both limits improve by at least one order of magnitude the previous results. | |
dc.identifier.citation | Physical Review Letters Vol.128 No.5 (2022) | |
dc.identifier.doi | 10.1103/PhysRevLett.128.051102 | |
dc.identifier.eissn | 10797114 | |
dc.identifier.issn | 00319007 | |
dc.identifier.pmid | 35179919 | |
dc.identifier.scopus | 2-s2.0-85124922741 | |
dc.identifier.uri | https://repository.li.mahidol.ac.th/handle/20.500.14594/87586 | |
dc.rights.holder | SCOPUS | |
dc.subject | Physics and Astronomy | |
dc.title | Exploring Lorentz Invariance Violation from Ultrahigh-Energy γ Rays Observed by LHAASO | |
dc.type | Article | |
mu.datasource.scopus | https://www.scopus.com/inward/record.uri?partnerID=HzOxMe3b&scp=85124922741&origin=inward | |
oaire.citation.issue | 5 | |
oaire.citation.title | Physical Review Letters | |
oaire.citation.volume | 128 | |
oairecerif.author.affiliation | State Key Laboratory of Particle Detection & Electronics | |
oairecerif.author.affiliation | Yunnan Observatories | |
oairecerif.author.affiliation | Nanjing University | |
oairecerif.author.affiliation | Shanghai Astronomical Observatory Chinese Academy of Sciences | |
oairecerif.author.affiliation | Institute for Nuclear Research of the Russian Academy of Sciences | |
oairecerif.author.affiliation | Shandong University | |
oairecerif.author.affiliation | Wuhan University | |
oairecerif.author.affiliation | Yunnan University | |
oairecerif.author.affiliation | Institute of High Energy Physics Chinese Academy of Science | |
oairecerif.author.affiliation | University of Chinese Academy of Sciences | |
oairecerif.author.affiliation | Guangzhou University | |
oairecerif.author.affiliation | Tsinghua University | |
oairecerif.author.affiliation | Sun Yat-Sen University | |
oairecerif.author.affiliation | University of Science and Technology of China | |
oairecerif.author.affiliation | Zhengzhou University | |
oairecerif.author.affiliation | Institiúid Ard-Lénn Bhaile Átha Cliath | |
oairecerif.author.affiliation | Università degli Studi di Napoli Federico II | |
oairecerif.author.affiliation | Sichuan University | |
oairecerif.author.affiliation | National Astronomical Observatories Chinese Academy of Sciences | |
oairecerif.author.affiliation | Max-Planck-Institut für Kernphysik | |
oairecerif.author.affiliation | Southwest Jiaotong University | |
oairecerif.author.affiliation | Purple Mountain Observatory Chinese Academy of Sciences | |
oairecerif.author.affiliation | Université de Genève | |
oairecerif.author.affiliation | Hebei Normal University | |
oairecerif.author.affiliation | Tibet University | |
oairecerif.author.affiliation | TIANFU Cosmic Ray Research Center |