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IRIS
: 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 10^{5} and 10^{9} GeV. Our results with LHAASO are robust, and have important implications for dark matter interpretations of the diffuse astrophysical high-energy neutrino emission.
Constraints on Heavy Decaying Dark Matter from 570 Days of LHAASO Observations / Cao, Zhen; Aharonian, F; An, Q; Axikegu, Null; Bai, L X; Bai, Y X; Bao, Y W; Bastieri, D; Bi, X J; Bi, Y J; Cai, J T; Cao, Zhe; Chang, J; Chang, J F; Chen, E S; Chen, Liang; Chen, Liang; Chen, Long; Chen, M J; Chen, M L; Chen, Q H; Chen, S H; Chen, S Z; Chen, T L; Chen, Y; Cheng, H L; Cheng, N; Cheng, Y D; Cui, S W; Cui, X H; Cui, Y D; D'Ettorre Piazzoli, B; Dai, B Z; Dai, H L; Dai, Z G; Danzengluobu, Null; Della Volpe, D; Duan, K K; Fan, J H; Fan, Y Z; Fan, Z X; Fang, J; Fang, K; Feng, C F; Feng, L; Feng, S H; Feng, X T; Feng, Y L; Gao, B; Gao, C D; Gao, L Q; Gao, Q; Gao, W; Gao, W K; Ge, M M; Geng, L S; Gong, G H; Gou, Q B; Gu, M H; Guo, F L; Guo, J G; Guo, X L; Guo, Y Q; Guo, Y Y; Han, Y A; He, H H; He, H N; He, S L; He, X B; He, Y; Heller, M; Hor, Y K; Hou, C; Hou, X; Hu, H B; Hu, Q; Hu, S; Hu, S C; Hu, X J; Huang, D H; Huang, W H; Huang, X T; Huang, X Y; Huang, Y; Huang, Z C; Ji, X L; Jia, H Y; Jia, K; Jiang, K; Jiang, Z J; Jin, M; Kang, M M; Ke, T; Kuleshov, D; Levochkin, K; Li, B B; Li, Cheng; Li, Cong; Li, F; Li, H B; Li, H C; Li, H Y; Li, J; Li, Jian; Li, Jie; Li, K; Li, W L; Li, X R; Li, Xin; Li, Xin; Li, Y Z; Li, Zhe; Li, Zhuo; Liang, E W; Liang, Y F; Lin, S J; Liu, B; Liu, C; Liu, D; Liu, H; Liu, H D; Liu, J; Liu, J L; Liu, J S; Liu, J Y; Liu, M Y; Liu, R Y; Liu, S M; Liu, W; Liu, Y; Liu, Y N; Long, W J; Lu, R; Luo, Q; Lv, H K; Ma, B Q; Ma, L L; Ma, X H; Mao, J R; Masood, A; Min, Z; Mitthumsiri, W; Nan, Y C; Ou, Z W; Pang, B Y; Pattarakijwanich, P; Pei, Z Y; Qi, M Y; Qi, Y Q; Qiao, B Q; Qin, J J; Ruffolo, D; Sáiz, A; Shao, C Y; Shao, L; Shchegolev, O; Sheng, X D; Shi, J Y; Song, H C; Stenkin, Yu V; Stepanov, V; Su, Y; Sun, Q N; Sun, X N; Sun, Z B; Tam, P H T; Tang, Z B; Tian, W W; Wang, B D; Wang, C; Wang, H; Wang, H G; Wang, J C; Wang, J S; Wang, L P; Wang, L Y; Wang, R; Wang, R N; Wang, W; Wang, X G; Wang, X Y; Wang, Y; Wang, Y D; Wang, Y J; Wang, Y P; Wang, Z H; Wang, Z X; Wang, Zhen; Wang, Zheng; Wei, D M; Wei, J J; Wei, Y J; Wen, T; Wu, C Y; Wu, H R; Wu, S; Wu, X F; Wu, Y S; Xi, S Q; Xia, J; Xia, J J; Xiang, G M; Xiao, D X; Xiao, G; Xin, G G; Xin, Y L; Xing, Y; Xiong, Z; Xu, D L; Xu, R X; Xue, L; Yan, D H; Yan, J Z; Yang, C W; Yang, F F; Yang, H W; Yang, J Y; Yang, L L; Yang, M J; Yang, R Z; Yang, S B; Yao, Y H; Yao, Z G; Ye, Y M; Yin, L Q; Yin, N; You, X H; You, Z Y; Yu, Y H; Yuan, Q; Yue, H; Zeng, H D; Zeng, T X; Zeng, W; Zeng, Z K; Zha, M; Zhai, X X; Zhang, B B; Zhang, F; Zhang, H M; Zhang, H Y; Zhang, J L; Zhang, L X; Zhang, Li; Zhang, Lu; Zhang, P F; Zhang, P P; Zhang, R; Zhang, S B; Zhang, S R; Zhang, S S; Zhang, X; Zhang, X P; Zhang, Y F; Zhang, Y L; Zhang, Yi; Zhang, Yong; Zhao, B; Zhao, J; Zhao, L; Zhao, L Z; Zhao, S P; Zheng, F; Zheng, Y; Zhou, B; Zhou, H; Zhou, J N; Zhou, P; Zhou, R; Zhou, X X; Zhu, C G; Zhu, F R; Zhu, H; Zhu, K J; Zuo, X; Ando, S; Chianese, M; Fiorillo, D F G; Miele, G; Ng, K C Y. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - 129:26(2022), p. 261103. [10.1103/PhysRevLett.129.261103]
Constraints on Heavy Decaying Dark Matter from 570 Days of LHAASO Observations
Cao, Zhen;Aharonian, F;An, Q;Axikegu, null;Bai, L X;Bai, Y X;Bao, Y W;Bastieri, D;Bi, X J;Bi, Y J;Cai, J T;Cao, Zhe;Chang, J;Chang, J F;Chen, E S;Chen, Liang;Chen, Liang;Chen, Long;Chen, M J;Chen, M L;Chen, Q H;Chen, S H;Chen, S Z;Chen, T L;Chen, Y;Cheng, H L;Cheng, N;Cheng, Y D;Cui, S W;Cui, X H;Cui, Y D;D'Ettorre Piazzoli, B;Dai, B Z;Dai, H L;Dai, Z G;Danzengluobu, null;Della Volpe, D;Duan, K K;Fan, J H;Fan, Y Z;Fan, Z X;Fang, J;Fang, K;Feng, C F;Feng, L;Feng, S H;Feng, X T;Feng, Y L;Gao, B;Gao, C D;Gao, L Q;Gao, Q;Gao, W;Gao, W K;Ge, M M;Geng, L S;Gong, G H;Gou, Q B;Gu, M H;Guo, F L;Guo, J G;Guo, X L;Guo, Y Q;Guo, Y Y;Han, Y A;He, H H;He, H N;He, S L;He, X B;He, Y;Heller, M;Hor, Y K;Hou, C;Hou, X;Hu, H B;Hu, Q;Hu, S;Hu, S C;Hu, X J;Huang, D H;Huang, W H;Huang, X T;Huang, X Y;Huang, Y;Huang, Z C;Ji, X L;Jia, H Y;Jia, K;Jiang, K;Jiang, Z J;Jin, M;Kang, M M;Ke, T;Kuleshov, D;Levochkin, K;Li, B B;Li, Cheng;Li, Cong;Li, F;Li, H B;Li, H C;Li, H Y;Li, J;Li, Jian;Li, Jie;Li, K;Li, W L;Li, X R;Li, Xin;Li, Xin;Li, Y Z;Li, Zhe;Li, Zhuo;Liang, E W;Liang, Y F;Lin, S J;Liu, B;Liu, C;Liu, D;Liu, H;Liu, H D;Liu, J;Liu, J L;Liu, J S;Liu, J Y;Liu, M Y;Liu, R Y;Liu, S M;Liu, W;Liu, Y;Liu, Y N;Long, W J;Lu, R;Luo, Q;Lv, H K;Ma, B Q;Ma, L L;Ma, X H;Mao, J R;Masood, A;Min, Z;Mitthumsiri, W;Nan, Y C;Ou, Z W;Pang, B Y;Pattarakijwanich, P;Pei, Z Y;Qi, M Y;Qi, Y Q;Qiao, B Q;Qin, J J;Ruffolo, D;Sáiz, A;Shao, C Y;Shao, L;Shchegolev, O;Sheng, X D;Shi, J Y;Song, H C;Stenkin, Yu V;Stepanov, V;Su, Y;Sun, Q N;Sun, X N;Sun, Z B;Tam, P H T;Tang, Z B;Tian, W W;Wang, B D;Wang, C;Wang, H;Wang, H G;Wang, J C;Wang, J S;Wang, L P;Wang, L Y;Wang, R;Wang, R N;Wang, W;Wang, X G;Wang, X Y;Wang, Y;Wang, Y D;Wang, Y J;Wang, Y P;Wang, Z H;Wang, Z X;Wang, Zhen;Wang, Zheng;Wei, D M;Wei, J J;Wei, Y J;Wen, T;Wu, C Y;Wu, H R;Wu, S;Wu, X F;Wu, Y S;Xi, S Q;Xia, J;Xia, J J;Xiang, G M;Xiao, D X;Xiao, G;Xin, G G;Xin, Y L;Xing, Y;Xiong, Z;Xu, D L;Xu, R X;Xue, L;Yan, D H;Yan, J Z;Yang, C W;Yang, F F;Yang, H W;Yang, J Y;Yang, L L;Yang, M J;Yang, R Z;Yang, S B;Yao, Y H;Yao, Z G;Ye, Y M;Yin, L Q;Yin, N;You, X H;You, Z Y;Yu, Y H;Yuan, Q;Yue, H;Zeng, H D;Zeng, T X;Zeng, W;Zeng, Z K;Zha, M;Zhai, X X;Zhang, B B;Zhang, F;Zhang, H M;Zhang, H Y;Zhang, J L;Zhang, L X;Zhang, Li;Zhang, Lu;Zhang, P F;Zhang, P P;Zhang, R;Zhang, S B;Zhang, S R;Zhang, S S;Zhang, X;Zhang, X P;Zhang, Y F;Zhang, Y L;Zhang, Yi;Zhang, Yong;Zhao, B;Zhao, J;Zhao, L;Zhao, L Z;Zhao, S P;Zheng, F;Zheng, Y;Zhou, B;Zhou, H;Zhou, J N;Zhou, P;Zhou, R;Zhou, X X;Zhu, C G;Zhu, F R;Zhu, H;Zhu, K J;Zuo, X;Ando, S;Chianese, M;Fiorillo, D F G;Miele, G;Ng, K C Y
2022
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 10^{5} and 10^{9} GeV. Our results with LHAASO are robust, and have important implications for dark matter interpretations of the diffuse astrophysical high-energy neutrino emission.
Constraints on Heavy Decaying Dark Matter from 570 Days of LHAASO Observations / Cao, Zhen; Aharonian, F; An, Q; Axikegu, Null; Bai, L X; Bai, Y X; Bao, Y W; Bastieri, D; Bi, X J; Bi, Y J; Cai, J T; Cao, Zhe; Chang, J; Chang, J F; Chen, E S; Chen, Liang; Chen, Liang; Chen, Long; Chen, M J; Chen, M L; Chen, Q H; Chen, S H; Chen, S Z; Chen, T L; Chen, Y; Cheng, H L; Cheng, N; Cheng, Y D; Cui, S W; Cui, X H; Cui, Y D; D'Ettorre Piazzoli, B; Dai, B Z; Dai, H L; Dai, Z G; Danzengluobu, Null; Della Volpe, D; Duan, K K; Fan, J H; Fan, Y Z; Fan, Z X; Fang, J; Fang, K; Feng, C F; Feng, L; Feng, S H; Feng, X T; Feng, Y L; Gao, B; Gao, C D; Gao, L Q; Gao, Q; Gao, W; Gao, W K; Ge, M M; Geng, L S; Gong, G H; Gou, Q B; Gu, M H; Guo, F L; Guo, J G; Guo, X L; Guo, Y Q; Guo, Y Y; Han, Y A; He, H H; He, H N; He, S L; He, X B; He, Y; Heller, M; Hor, Y K; Hou, C; Hou, X; Hu, H B; Hu, Q; Hu, S; Hu, S C; Hu, X J; Huang, D H; Huang, W H; Huang, X T; Huang, X Y; Huang, Y; Huang, Z C; Ji, X L; Jia, H Y; Jia, K; Jiang, K; Jiang, Z J; Jin, M; Kang, M M; Ke, T; Kuleshov, D; Levochkin, K; Li, B B; Li, Cheng; Li, Cong; Li, F; Li, H B; Li, H C; Li, H Y; Li, J; Li, Jian; Li, Jie; Li, K; Li, W L; Li, X R; Li, Xin; Li, Xin; Li, Y Z; Li, Zhe; Li, Zhuo; Liang, E W; Liang, Y F; Lin, S J; Liu, B; Liu, C; Liu, D; Liu, H; Liu, H D; Liu, J; Liu, J L; Liu, J S; Liu, J Y; Liu, M Y; Liu, R Y; Liu, S M; Liu, W; Liu, Y; Liu, Y N; Long, W J; Lu, R; Luo, Q; Lv, H K; Ma, B Q; Ma, L L; Ma, X H; Mao, J R; Masood, A; Min, Z; Mitthumsiri, W; Nan, Y C; Ou, Z W; Pang, B Y; Pattarakijwanich, P; Pei, Z Y; Qi, M Y; Qi, Y Q; Qiao, B Q; Qin, J J; Ruffolo, D; Sáiz, A; Shao, C Y; Shao, L; Shchegolev, O; Sheng, X D; Shi, J Y; Song, H C; Stenkin, Yu V; Stepanov, V; Su, Y; Sun, Q N; Sun, X N; Sun, Z B; Tam, P H T; Tang, Z B; Tian, W W; Wang, B D; Wang, C; Wang, H; Wang, H G; Wang, J C; Wang, J S; Wang, L P; Wang, L Y; Wang, R; Wang, R N; Wang, W; Wang, X G; Wang, X Y; Wang, Y; Wang, Y D; Wang, Y J; Wang, Y P; Wang, Z H; Wang, Z X; Wang, Zhen; Wang, Zheng; Wei, D M; Wei, J J; Wei, Y J; Wen, T; Wu, C Y; Wu, H R; Wu, S; Wu, X F; Wu, Y S; Xi, S Q; Xia, J; Xia, J J; Xiang, G M; Xiao, D X; Xiao, G; Xin, G G; Xin, Y L; Xing, Y; Xiong, Z; Xu, D L; Xu, R X; Xue, L; Yan, D H; Yan, J Z; Yang, C W; Yang, F F; Yang, H W; Yang, J Y; Yang, L L; Yang, M J; Yang, R Z; Yang, S B; Yao, Y H; Yao, Z G; Ye, Y M; Yin, L Q; Yin, N; You, X H; You, Z Y; Yu, Y H; Yuan, Q; Yue, H; Zeng, H D; Zeng, T X; Zeng, W; Zeng, Z K; Zha, M; Zhai, X X; Zhang, B B; Zhang, F; Zhang, H M; Zhang, H Y; Zhang, J L; Zhang, L X; Zhang, Li; Zhang, Lu; Zhang, P F; Zhang, P P; Zhang, R; Zhang, S B; Zhang, S R; Zhang, S S; Zhang, X; Zhang, X P; Zhang, Y F; Zhang, Y L; Zhang, Yi; Zhang, Yong; Zhao, B; Zhao, J; Zhao, L; Zhao, L Z; Zhao, S P; Zheng, F; Zheng, Y; Zhou, B; Zhou, H; Zhou, J N; Zhou, P; Zhou, R; Zhou, X X; Zhu, C G; Zhu, F R; Zhu, H; Zhu, K J; Zuo, X; Ando, S; Chianese, M; Fiorillo, D F G; Miele, G; Ng, K C Y. - In: PHYSICAL REVIEW LETTERS. - ISSN 0031-9007. - 129:26(2022), p. 261103. [10.1103/PhysRevLett.129.261103]
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Il report seguente simula gli indicatori relativi alla propria produzione scientifica in relazione alle soglie ASN 2023-2025 del proprio SC/SSD. Si ricorda che il superamento dei valori soglia (almeno 2 su 3) è requisito necessario ma non sufficiente al conseguimento dell'abilitazione. La simulazione si basa sui dati IRIS e sugli indicatori bibliometrici alla data indicata e non tiene conto di eventuali periodi di congedo obbligatorio, che in sede di domanda ASN danno diritto a incrementi percentuali dei valori. La simulazione può differire dall'esito di un’eventuale domanda ASN sia per errori di catalogazione e/o dati mancanti in IRIS, sia per la variabilità dei dati bibliometrici nel tempo. Si consideri che Anvur calcola i valori degli indicatori all'ultima data utile per la presentazione delle domande.
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