English
 
Help Privacy Policy Disclaimer
  Advanced SearchBrowse

Item

ITEM ACTIONSEXPORT
  Very high-energy gamma-ray emission beyond 10 TeV from GRB 221009A

LHASSO Collaboration, Zhen, C., Aharonian, F., An, Q., Axikegu, Bai, Y., et al. (2023). Very high-energy gamma-ray emission beyond 10 TeV from GRB 221009A. Science Advances, 9(46): eadj2778. doi:10.1126/sciadv.adj2778.

Item is

Files

show Files

Locators

show
hide
Description:
-
OA-Status:
Gold

Creators

show
hide
 Creators:
LHASSO Collaboration, Author              
Zhen, Cao, Author
Aharonian, F.1, Author                 
An, Q., Author
Axikegu, Author
Bai, Y.X., Author
Bao, Y.W., Author
Bastieri, D., Author
Bi, X.J., Author
Bi, Y.J., Author
Cai, J.T., Author
Cao, Q., Author
Cao, W.Y., Author
Zhe, Cao, Author
Chang, J., Author
Chang, J.F., Author
Chen, A.M., Author
Chen, E.S., Author
Liang, Chen, Author
Lin, Chen, Author
Long, Chen, AuthorChen, M.J., AuthorChen, M.L., AuthorChen, Q.H., AuthorChen, S.H., AuthorChen, S.Z., AuthorChen, T.L., AuthorChen, Y., AuthorCheng, N., AuthorCheng, Y.D., AuthorCui, M.Y., AuthorCui, S.W., AuthorCui, X.H., AuthorCui, Y.D., AuthorDai, B.Z., AuthorDai, H.L., AuthorDai, Z.G., AuthorDanzengluobu, Authordella Volpe, D., AuthorDong, X.Q., AuthorDuan, K.K., AuthorFan, J.H., AuthorFan, Y.Z., AuthorFang, J., AuthorFang, K., AuthorFeng, C.F., AuthorFeng, L., AuthorFeng, S.H., AuthorFeng, X.T., AuthorFeng, Y.L., AuthorGabici, S., AuthorGao, B., AuthorGao, C.D., AuthorGao, L.Q., AuthorGao, Q., AuthorGao, W., AuthorGao, W.K., AuthorGe, M.M., AuthorGeng, L.S., AuthorGiacinti, G., AuthorGong, G.H., AuthorGou, Q.B., AuthorGu, M.H., AuthorGuo, F.L., AuthorGuo, X.L., AuthorGuo, Y.Q., AuthorGuo, Y.Y., AuthorHan, Y.A., AuthorHe, H.H., AuthorHe, H.N., AuthorHe, J.Y., AuthorHe, X.B., AuthorHe, Y., AuthorHeller, M., AuthorHor, Y.K., AuthorHou, B.W., AuthorHou, C., AuthorHou, X., AuthorHu, H.B., AuthorHu, Q., AuthorHu, S.C., AuthorHuang, D.H., AuthorHuang, T.Q., AuthorHuang, W.J., AuthorHuang, X.T., AuthorHuang, X.Y., AuthorHuang, Y., AuthorHuang, Z.C., AuthorJi, X.L., AuthorJia, H.Y., AuthorJia, K., AuthorJiang, K., AuthorJiang, X.W., AuthorJiang, Z.J., AuthorJin, M., AuthorKang, M.M., AuthorKe, T., AuthorKuleshov, D., AuthorKurinov, K., AuthorLi, B.B., AuthorCheng, Li, AuthorCong, Li, AuthorLi, D., AuthorLi, F., AuthorLi, H.B., AuthorLi H.Y.Li, H.C., AuthorLi, J., AuthorJian, Li, AuthorJie, Li, AuthorLi, K., AuthorLi, W.L., AuthorLi, W.L., AuthorLi, X.R., AuthorXin, Li, AuthorLi, Y.Z., AuthorZhe, Li, AuthorZhuo, Li, AuthorLiang, E.W., AuthorLiang, Y.F., AuthorLin, S.J., AuthorLiu, B., AuthorLiu, C., AuthorLiu, D., AuthorLiu, H., AuthorLiu, H.D., AuthorLiu, J., AuthorLiu, J.L., AuthorLiu, J.Y., AuthorLiu, M.Y., AuthorLiu, R.Y., AuthorLiu W.Liu, S.M., AuthorLiu, Y., AuthorLiu, Y.N., AuthorLu, R., AuthorLuo, Q., AuthorLv, H.K., AuthorMa, B.Q., AuthorMa, L.L., AuthorMa, X.H., AuthorMao, J.R., AuthorMin, Z., AuthorMitthumsiri, W., AuthorMu, H.J., AuthorNan, Y.C., AuthorNeronov, A., AuthorOu, Z.W., AuthorPang, B.Y., AuthorPattarakijwanich, P., AuthorPei, Z.Y., AuthorQi, M.Y., AuthorQi, Y.Q., AuthorQiao, B.Q., AuthorQin, J.J., AuthorRuffolo, D., AuthorS´aiz, A., AuthorSemikoz, D., AuthorShao, C.Y., AuthorShao, L., AuthorShchegolev, O., AuthorSheng, X.D., AuthorShu, F.W., AuthorSong, H.C., AuthorStenkin, Yu.V., AuthorStepanov, V., AuthorSu, Y., AuthorSun, Q.N., AuthorSun, X.N., AuthorSun, Z.B., AuthorTam, P.H.T., AuthorTang, Q.W., AuthorTang, Z.B., AuthorTian, W.W., AuthorWang, C., AuthorWang, C.B., AuthorWang, G.W., AuthorWang, H.G., AuthorWang, H.H., AuthorWang, J.C., AuthorWang, K., AuthorWang, L.P., AuthorWang, L.Y., AuthorWang, P.H., AuthorWang, R., AuthorWang, W., AuthorWang, X.G., AuthorWang, X.Y., AuthorWang, Y., AuthorWang, Y.D., AuthorWang, Y.J., AuthorWang, Z.H., AuthorWang, Z.X., AuthorZhen, Wang, AuthorZheng, Wang, AuthorWei, D.M., AuthorWei, J.J., AuthorWei, Y.J., AuthorWen, T., AuthorWu, C.Y., AuthorWu, H.R., AuthorWu, S., AuthorWu, X.F., AuthorWu, Y.S., AuthorXi, S.Q., AuthorXia, J., AuthorXia, J.J., AuthorXiang, G.M., AuthorXiao, D.X., AuthorXiao, G., AuthorXin, G.G., AuthorXin, Y.L., AuthorXing, Y., AuthorXiong, Z., AuthorXu, D.L., AuthorXu, R.F., AuthorXu, R.X., AuthorXu, W.L., AuthorXue, L., AuthorYan, D.H., AuthorYan, J.Z., AuthorYan, T., AuthorYang, C.W., AuthorYang, F., AuthorYang, F.F., AuthorYang, H.W., AuthorYang, J.Y., AuthorYang, L.L., AuthorYang, M.J., AuthorYang, R.Z., AuthorYang, S.B., AuthorYao, Y.H., AuthorYao, Z.G., AuthorYe, Y.M., AuthorYin, L.Q., AuthorYin, N., AuthorYou, X.H., AuthorYou, Z.Y., AuthorYu, Y.H., AuthorYuan, Q., AuthorYue, H., AuthorZeng, H.D., AuthorZeng, T.X., AuthorZeng, W., AuthorZha, M., AuthorZhang, B.B., AuthorZhang, F., AuthorZhang, H.M., AuthorZhang, H.Y., AuthorZhang, J.L., AuthorZhang, L.X., AuthorLi, Zhang, AuthorZhang, P.F., AuthorZhang, P.P., AuthorZhang, R., AuthorZhang, S.B., AuthorZhang, S.R., AuthorZhang, S.S., AuthorZhang, X., AuthorZhang, X.P., AuthorZhang, Y.F., AuthorYi, Zhang, AuthorYong, Zhang, AuthorZhao, B., AuthorZhaoac, J., AuthorZhao, L., AuthorZhao, L.Z., AuthorZhao, S.P., AuthorZheng, F., AuthorZheng, J.H., AuthorZhou, B., AuthorZhou, H., AuthorZhou, J.N., AuthorZhou, M., AuthorZhou, P., AuthorZhou, R., AuthorZhou, X.X., AuthorZhu, C.G., AuthorZhu, F.R., AuthorZhu, H., AuthorZhu, K.J., AuthorZuo, X., Author more..
Affiliations:
1Division Prof. Dr. James A. Hinton, MPI for Nuclear Physics, Max Planck Society, ou_2074298              

Content

show
hide
Free keywords: -
 MPINP: Hochenergie-Astrophysik Theorie - Abteilung Hinton
 Abstract: The highest-energy gamma-rays from gamma-ray bursts (GRBs) have important implications for their radiation mechanism. Here we report the detection of gamma-rays up to 13 teraelectronvolts from the brightest GRB 221009A by the Large High Altitude Air-shower Observatory (LHAASO). The LHAASO-KM2A detector registered more than 140 gamma-rays with energies above 3 teraelectronvolts during 230 to 900 seconds after the trigger. The intrinsic energy spectrum of gamma-rays can be described by a power-law after correcting for extragalactic background light absorption. Such a hard spectrum challenges the synchrotron self-Compton scenario of relativistic electrons for the afterglow emission above several teraelectronvolts. Observations of gamma-rays up to 13 teraelectronvolts from a source with a measured redshift of z = 0.151 hints more transparency in intergalactic space than previously expected. Alternatively, one may invoke new physics such as Lorentz invariance violation or an axion origin of very high-energy signals.

Details

show
hide
Language(s):
 Dates: 2023-11-15
 Publication Status: Published online
 Pages: 29
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: DOI: 10.1126/sciadv.adj2778
 Degree: -

Event

show

Legal Case

show

Project information

show

Source 1

show
hide
Title: Science Advances
  Other : Sci. Adv.
Source Genre: Journal
 Creator(s):
Affiliations:
Publ. Info: Washington : AAAS
Pages: - Volume / Issue: 9 (46) Sequence Number: eadj2778 Start / End Page: - Identifier: ISSN: 2375-2548
CoNE: https://pure.mpg.de/cone/journals/resource/2375-2548