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  Constraints on Heavy Decaying Dark Matter from 570 Days of LHAASO Observations

LHASSO Collaboration, Aharonian, F., An, Q., Axikegu, L. X., B., Bai, Y. X., et al. (2022). Constraints on Heavy Decaying Dark Matter from 570 Days of LHAASO Observations. Physical Review Letters, 129(26): 261103. doi:10.1103/PhysRevLett.129.261103.

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LHASSO Collaboration, Author              
Aharonian, F.1, Author                 
An, Q., Author
Axikegu , Author
L. X., Bai, 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, Zhe, Author
Cao, Zhen, Author
Chang, J., Author
Chang, J. F., Author
Chen, E. S., Author
Chen, Liang, Author
Chen, Liang, Author
Chen, Long, Author
Chen, M. J., Author
Chen, M. L., AuthorChen, Q. H., AuthorChen, S. H., AuthorChen, S. Z., AuthorChen, T. L., AuthorChen, Y., AuthorCheng, H. L., AuthorCheng, N., AuthorCheng, Y. D., AuthorCui, S. W., AuthorCui, X. H., AuthorCui, Y. D., AuthorD’Ettorre Piazzoli, B., AuthorDai, B. Z., AuthorDai, H. L., AuthorDai, Z. G., AuthorDanzengluobu , Authordella Volpe, D., AuthorDuan, K. K., AuthorFan, J. H., AuthorFan, Y. Z., AuthorFan, Z. X., AuthorFang, J., AuthorFang, K., AuthorFeng, C. F., AuthorFeng, L., AuthorFeng, S. H., AuthorFeng, X. T., AuthorFeng, Y. L., AuthorGao, B., AuthorGao, C. D., AuthorGao, L. Q., AuthorGao, Q., AuthorGao, W., AuthorGao, W. K., AuthorGe, M. M., AuthorGeng, L. S., AuthorGong, G. H., AuthorGou, Q. B., AuthorGu, M. H., AuthorGuo, F. L., AuthorGuo, J. G., AuthorGuo, X. L., AuthorGuo, Y. Q., AuthorGuo, Y. Y., AuthorHan, Y. A., AuthorHe, H. H., AuthorHe, H. N., AuthorHe, S. L., AuthorHe, X. B., AuthorHe, Y., AuthorHeller, M., AuthorHor, Y. K., AuthorHou, C., AuthorHou, X., AuthorHu, H. B., AuthorHu, Q., AuthorHu, S., AuthorHu, S. C., AuthorHu, X. J., AuthorHuang, D. H., AuthorHuang, W. H., AuthorHuang, X. T., AuthorHuang, X. Y., AuthorHuang, Y., AuthorHuang, Z. C., AuthorJi, X. L., AuthorJia, H. Y., AuthorJia, K., AuthorJiang, K., AuthorJiang, Z. J., AuthorJin, M., AuthorKang, M. M., AuthorKe, T., AuthorKuleshov, D., AuthorLevochkin, K., AuthorLi, B. B., AuthorLi, Cheng, AuthorLi, Cong, AuthorLi, F., AuthorLi, H. B., AuthorLi, H. C., AuthorLi, H. Y., AuthorLi, J., AuthorLi, Jian, AuthorLi, Jie, AuthorLi, K., AuthorLi, W. L., AuthorLi, X. R., AuthorLi, Xin, AuthorLi, Xin, AuthorLi, Y. Z., AuthorLi, Zhe, AuthorLi, Zhuo, 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. S., AuthorLiu, J. Y., AuthorLiu, M. Y., AuthorLiu, R. Y., AuthorLiu, S. M., AuthorLiu, W., AuthorLiu, Y., AuthorLiu, Y. N., AuthorLong, W. J., AuthorLu, R., AuthorLuo, Q., AuthorLv, H. K., AuthorMa, B. Q., AuthorMa, L. L., AuthorMa, X. H., AuthorMao, J. R., AuthorMasood, A., AuthorMin, Z., AuthorMitthumsiri, W., AuthorNan, Y. C., 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., AuthorSáiz, A., AuthorShao, C. Y., AuthorShao, L., AuthorShchegolev, O., AuthorSheng, X. D., AuthorShi, J. Y., AuthorSong, H. C., AuthorStenkin, Yu. V., AuthorStepanov, V., AuthorSu, Y., AuthorSun, Q. N., AuthorSun, X. N., AuthorSun, Z. B., AuthorTam, P. H. T., AuthorTang, Z. B., AuthorTian, W. W., AuthorWang, B. D., AuthorWang, C., AuthorWang, H., AuthorWang, H. G., AuthorWang, J. C., AuthorWang, J. S., AuthorWang, L. P., AuthorWang, L. Y., AuthorWang, R., AuthorWang, R. N., AuthorWang, W., AuthorWang, X. G., AuthorWang, X. Y., AuthorWang, Y., AuthorWang, Y. D., AuthorWang, Y. J., AuthorWang, Y. P., AuthorWang, Z. H., AuthorWang, Z. X., AuthorWang, Zhen, AuthorWang, Zheng, 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. X., AuthorXue, L., AuthorYan, D. H., AuthorYan, J. Z., AuthorYang, C. W., 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., AuthorZeng, Z. K., AuthorZha, M., AuthorZhai, X. X., AuthorZhang, B. B., AuthorZhang, F., AuthorZhang, H. M., AuthorZhang, H. Y., AuthorZhang, J. L., AuthorZhang, L. X., AuthorZhang, Li, AuthorZhang, Lu, 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., AuthorZhang, Y. L., AuthorZhang, Yi, AuthorZhang, Yong, AuthorZhao, B., AuthorZhao, J., AuthorZhao, L., AuthorZhao, L. Z., AuthorZhao, S. P., AuthorZheng, F., AuthorZheng, Y., AuthorZhou, B., AuthorZhou, H., AuthorZhou, J. N., 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              

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Free keywords: Dark matter, Gamma ray astronomy
 MPINP: Hochenergie-Astrophysik Theorie - Abteilung Hinton
 Abstract: The kilometer square array (KM2A) of the large high altitude air shower observatory (LHAASO) aims at surveying the northern γ-ray sky at energies above 10 TeV with unprecedented sensitivity. γ-ray observations have long been one of the most powerful tools for dark matter searches, as, e.g., high-energy γ rays could be produced by the decays of heavy dark matter particles. In this Letter, we present the first dark matter analysis with LHAASO-KM2A, using the first 340 days of data from 1/2-KM2A and 230 days of data from 3/4-KM2A. Several regions of interest are used to search for a signal and account for the residual cosmic-ray background after γ/hadron separation. We find no excess of dark matter signals, and thus place some of the strongest γ-ray constraints on the lifetime of heavy dark matter particles with mass between 105 and 109  GeV. Our results with LHAASO are robust, and have important implications for dark matter interpretations of the diffuse astrophysical high-energy neutrino emission.

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 Dates: 2022-12-21
 Publication Status: Published online
 Pages: 9
 Publishing info: -
 Table of Contents: -
 Rev. Type: -
 Identifiers: DOI: 10.1103/PhysRevLett.129.261103
 Degree: -

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Title: Physical Review Letters
  Abbreviation : Phys. Rev. Lett.
Source Genre: Journal
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Publ. Info: Woodbury, N.Y. : American Physical Society
Pages: - Volume / Issue: 129 (26) Sequence Number: 261103 Start / End Page: - Identifier: ISSN: 0031-9007
CoNE: https://pure.mpg.de/cone/journals/resource/954925433406_1