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Fermi large area telescope search for photon lines from 30 to 200 GeV and dark matter implications

Dark matter (DM) particle annihilation or decay can produce monochromatic gamma rays readily distinguishable from astrophysical sources. gamma-ray line limits from 30 to 200 GeV obtained from 11 months of Fermi Large Area Space Telescope data from 20-300 GeV are presented using a selection based on... Full description

Journal Title: Physical review letters 05 March 2010, Vol.104(9), pp.091302
Main Author: Abdo, A A
Other Authors: Ackermann, M , Ajello, M , Atwood, W B , Baldini, L , Ballet, J , Barbiellini, G , Bastieri, D , Bechtol, K , Bellazzini, R , Berenji, B , Bloom, E D , Bonamente, E , Borgland, A W , Bouvier, A , Bregeon, J , Brez, A , Brigida, M , Bruel, P , Burnett, T H , Buson, S , Caliandro, G A , Cameron, R A , Caraveo, P A , Carrigan, S , Casandjian, J M , Cecchi, C , Celik, O , Chekhtman, A , Chiang, J , Ciprini, S , Claus, R , Cohen-Tanugi, J , Conrad, J , Dermer, C D , De Angelis, A , De Palma, F , Digel, S W , Do Couto E Silva, E , Drell, P S , Drlica-Wagner, A , Dubois, R , Dumora, D , Edmonds, Y , Essig, R , Farnier, C , Favuzzi, C , Fegan, S J , Focke, W B , Fortin, P , Frailis, M , Fukazawa, Y , Funk, S , Fusco, P , Gargano, F , Gasparrini, D , Gehrels, N , Germani, S , Giglietto, N , Giordano, F , Glanzman, T , Godfrey, G , Grenier, I A , Grove, J E , Guillemot, L , Guiriec, S , Gustafsson, M , Hadasch, D , Harding, A K , Horan, D , Hughes, R E , Jackson, M S , Jóhannesson, G , Johnson, A S , Johnson, R P , Johnson, W N , Kamae, T , Katagiri, H , Kataoka, J , Kawai, N , Kerr, M , Knödlseder, J , Kuss, M , Lande, J , Latronico, L , Llena Garde, M , Longo, F , Loparco, F , Lott, B , Lovellette, M N , Lubrano, P , Makeev, A , Mazziotta, M N , Mcenery, J E , Meurer, C , Michelson, P F , Mitthumsiri, W , Mizuno, T , Moiseev, A A , Monte, C , Monzani, M E , Morselli, A , Moskalenko, I V , Murgia, S , Nolan, P L , Norris, J P , Nuss, E , Ohsugi, T , Omodei, N , Orlando, E , Ormes, J F , Ozaki, M , Paneque, D , Panetta, J H , Parent, D , Pelassa, V , Pepe, M , Pesce-Rollins, M , Piron, F , Rainò, S , Rando, R , Razzano, M , Reimer, A , Reimer, O , Reposeur, T , Ripken, J , Ritz, S , Rodriguez, A Y , Roth, M , Sadrozinski, H F-W , Sander, A , Parkinson, P M Saz , Scargle, J D , Schalk, T L , Sellerholm, A , Sgrò, C , Siskind, E J , Smith, D A , Smith, P D , Spandre, G , Spinelli, P , Starck, J-L , Strickman, M S , Suson, D J , Tajima, H , Takahashi, H , Tanaka, T , Thayer, J B , Thayer, J G , Tibaldo, L , Torres, D F , Uchiyama, Y , Usher, T L , Vasileiou, V , Vilchez, N , Vitale, V , Waite, A P , Wang, P , Winer, B L , Wood, K S , Ylinen, T , Ziegler, M
Format: Electronic Article Electronic Article
Language: English
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ID: E-ISSN: 1079-7114 ; PMID: 20366979 Version:1
Link: http://pubmed.gov/20366979
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title: Fermi large area telescope search for photon lines from 30 to 200 GeV and dark matter implications
format: Article
creator:
  • Abdo, A A
  • Ackermann, M
  • Ajello, M
  • Atwood, W B
  • Baldini, L
  • Ballet, J
  • Barbiellini, G
  • Bastieri, D
  • Bechtol, K
  • Bellazzini, R
  • Berenji, B
  • Bloom, E D
  • Bonamente, E
  • Borgland, A W
  • Bouvier, A
  • Bregeon, J
  • Brez, A
  • Brigida, M
  • Bruel, P
  • Burnett, T H
  • Buson, S
  • Caliandro, G A
  • Cameron, R A
  • Caraveo, P A
  • Carrigan, S
  • Casandjian, J M
  • Cecchi, C
  • Celik, O
  • Chekhtman, A
  • Chiang, J
  • Ciprini, S
  • Claus, R
  • Cohen-Tanugi, J
  • Conrad, J
  • Dermer, C D
  • De Angelis, A
  • De Palma, F
  • Digel, S W
  • Do Couto E Silva, E
  • Drell, P S
  • Drlica-Wagner, A
  • Dubois, R
  • Dumora, D
  • Edmonds, Y
  • Essig, R
  • Farnier, C
  • Favuzzi, C
  • Fegan, S J
  • Focke, W B
  • Fortin, P
  • Frailis, M
  • Fukazawa, Y
  • Funk, S
  • Fusco, P
  • Gargano, F
  • Gasparrini, D
  • Gehrels, N
  • Germani, S
  • Giglietto, N
  • Giordano, F
  • Glanzman, T
  • Godfrey, G
  • Grenier, I A
  • Grove, J E
  • Guillemot, L
  • Guiriec, S
  • Gustafsson, M
  • Hadasch, D
  • Harding, A K
  • Horan, D
  • Hughes, R E
  • Jackson, M S
  • Jóhannesson, G
  • Johnson, A S
  • Johnson, R P
  • Johnson, W N
  • Kamae, T
  • Katagiri, H
  • Kataoka, J
  • Kawai, N
  • Kerr, M
  • Knödlseder, J
  • Kuss, M
  • Lande, J
  • Latronico, L
  • Llena Garde, M
  • Longo, F
  • Loparco, F
  • Lott, B
  • Lovellette, M N
  • Lubrano, P
  • Makeev, A
  • Mazziotta, M N
  • Mcenery, J E
  • Meurer, C
  • Michelson, P F
  • Mitthumsiri, W
  • Mizuno, T
  • Moiseev, A A
  • Monte, C
  • Monzani, M E
  • Morselli, A
  • Moskalenko, I V
  • Murgia, S
  • Nolan, P L
  • Norris, J P
  • Nuss, E
  • Ohsugi, T
  • Omodei, N
  • Orlando, E
  • Ormes, J F
  • Ozaki, M
  • Paneque, D
  • Panetta, J H
  • Parent, D
  • Pelassa, V
  • Pepe, M
  • Pesce-Rollins, M
  • Piron, F
  • Rainò, S
  • Rando, R
  • Razzano, M
  • Reimer, A
  • Reimer, O
  • Reposeur, T
  • Ripken, J
  • Ritz, S
  • Rodriguez, A Y
  • Roth, M
  • Sadrozinski, H F-W
  • Sander, A
  • Parkinson, P M Saz
  • Scargle, J D
  • Schalk, T L
  • Sellerholm, A
  • Sgrò, C
  • Siskind, E J
  • Smith, D A
  • Smith, P D
  • Spandre, G
  • Spinelli, P
  • Starck, J-L
  • Strickman, M S
  • Suson, D J
  • Tajima, H
  • Takahashi, H
  • Tanaka, T
  • Thayer, J B
  • Thayer, J G
  • Tibaldo, L
  • Torres, D F
  • Uchiyama, Y
  • Usher, T L
  • Vasileiou, V
  • Vilchez, N
  • Vitale, V
  • Waite, A P
  • Wang, P
  • Winer, B L
  • Wood, K S
  • Ylinen, T
  • Ziegler, M
subjects:
  • Astrophysics - High Energy Astrophysical Phenomena
  • Astrophysics - Cosmology And Extragalactic Astrophysics
  • High Energy Physics - Experiment
  • High Energy Physics - Phenomenology
ispartof: Physical review letters, 05 March 2010, Vol.104(9), pp.091302
description: Dark matter (DM) particle annihilation or decay can produce monochromatic gamma rays readily distinguishable from astrophysical sources. gamma-ray line limits from 30 to 200 GeV obtained from 11 months of Fermi Large Area Space Telescope data from 20-300 GeV are presented using a selection based on requirements for a gamma-ray line analysis, and integrated over most of the sky. We obtain gamma-ray line flux upper limits in the range 0.6-4.5x10{-9} cm{-2} s{-1}, and give corresponding DM annihilation cross-section and decay lifetime limits. Theoretical implications are briefly discussed.
language: eng
source:
identifier: E-ISSN: 1079-7114 ; PMID: 20366979 Version:1
fulltext: no_fulltext
issn:
  • 10797114
  • 1079-7114
url: Link


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titleFermi large area telescope search for photon lines from 30 to 200 GeV and dark matter implications
creatorAbdo, A A ; Ackermann, M ; Ajello, M ; Atwood, W B ; Baldini, L ; Ballet, J ; Barbiellini, G ; Bastieri, D ; Bechtol, K ; Bellazzini, R ; Berenji, B ; Bloom, E D ; Bonamente, E ; Borgland, A W ; Bouvier, A ; Bregeon, J ; Brez, A ; Brigida, M ; Bruel, P ; Burnett, T H ; Buson, S ; Caliandro, G A ; Cameron, R A ; Caraveo, P A ; Carrigan, S ; Casandjian, J M ; Cecchi, C ; Celik, O ; Chekhtman, A ; Chiang, J ; Ciprini, S ; Claus, R ; Cohen-Tanugi, J ; Conrad, J ; Dermer, C D ; De Angelis, A ; De Palma, F ; Digel, S W ; Do Couto E Silva, E ; Drell, P S ; Drlica-Wagner, A ; Dubois, R ; Dumora, D ; Edmonds, Y ; Essig, R ; Farnier, C ; Favuzzi, C ; Fegan, S J ; Focke, W B ; Fortin, P ; Frailis, M ; Fukazawa, Y ; Funk, S ; Fusco, P ; Gargano, F ; Gasparrini, D ; Gehrels, N ; Germani, S ; Giglietto, N ; Giordano, F ; Glanzman, T ; Godfrey, G ; Grenier, I A ; Grove, J E ; Guillemot, L ; Guiriec, S ; Gustafsson, M ; Hadasch, D ; Harding, A K ; Horan, D ; Hughes, R E ; Jackson, M S ; Jóhannesson, G ; Johnson, A S ; Johnson, R P ; Johnson, W N ; Kamae, T ; Katagiri, H ; Kataoka, J ; Kawai, N ; Kerr, M ; Knödlseder, J ; Kuss, M ; Lande, J ; Latronico, L ; Llena Garde, M ; Longo, F ; Loparco, F ; Lott, B ; Lovellette, M N ; Lubrano, P ; Makeev, A ; Mazziotta, M N ; Mcenery, J E ; Meurer, C ; Michelson, P F ; Mitthumsiri, W ; Mizuno, T ; Moiseev, A A ; Monte, C ; Monzani, M E ; Morselli, A ; Moskalenko, I V ; Murgia, S ; Nolan, P L ; Norris, J P ; Nuss, E ; Ohsugi, T ; Omodei, N ; Orlando, E ; Ormes, J F ; Ozaki, M ; Paneque, D ; Panetta, J H ; Parent, D ; Pelassa, V ; Pepe, M ; Pesce-Rollins, M ; Piron, F ; Rainò, S ; Rando, R ; Razzano, M ; Reimer, A ; Reimer, O ; Reposeur, T ; Ripken, J ; Ritz, S ; Rodriguez, A Y ; Roth, M ; Sadrozinski, H F-W ; Sander, A ; Parkinson, P M Saz ; Scargle, J D ; Schalk, T L ; Sellerholm, A ; Sgrò, C ; Siskind, E J ; Smith, D A ; Smith, P D ; Spandre, G ; Spinelli, P ; Starck, J-L ; Strickman, M S ; Suson, D J ; Tajima, H ; Takahashi, H ; Tanaka, T ; Thayer, J B ; Thayer, J G ; Tibaldo, L ; Torres, D F ; Uchiyama, Y ; Usher, T L ; Vasileiou, V ; Vilchez, N ; Vitale, V ; Waite, A P ; Wang, P ; Winer, B L ; Wood, K S ; Ylinen, T ; Ziegler, M
ispartofPhysical review letters, 05 March 2010, Vol.104(9), pp.091302
identifierE-ISSN: 1079-7114 ; PMID: 20366979 Version:1
descriptionDark matter (DM) particle annihilation or decay can produce monochromatic gamma rays readily distinguishable from astrophysical sources. gamma-ray line limits from 30 to 200 GeV obtained from 11 months of Fermi Large Area Space Telescope data from 20-300 GeV are presented using a selection based on requirements for a gamma-ray line analysis, and integrated over most of the sky. We obtain gamma-ray line flux upper limits in the range 0.6-4.5x10{-9} cm{-2} s{-1}, and give corresponding DM annihilation cross-section and decay lifetime limits. Theoretical implications are briefly discussed.
languageeng
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1Ackermann, M
2Ajello, M
3Atwood, W B
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5Ballet, J
6Barbiellini, G
7Bastieri, D
8Bechtol, K
9Bellazzini, R
10Berenji, B
11Bloom, E D
12Bonamente, E
13Borgland, A W
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15Bregeon, J
16Brez, A
17Brigida, M
18Bruel, P
19Burnett, T H
20Buson, S
21Caliandro, G A
22Cameron, R A
23Caraveo, P A
24Carrigan, S
25Casandjian, J M
26Cecchi, C
27Celik, O
28Chekhtman, A
29Chiang, J
30Ciprini, S
31Claus, R
32Cohen-Tanugi, J
33Conrad, J
34Dermer, C D
35de Angelis, A
36de Palma, F
37Digel, S W
38do Couto E Silva, E
39Drell, P S
40Drlica-Wagner, A
41Dubois, R
42Dumora, D
43Edmonds, Y
44Essig, R
45Farnier, C
46Favuzzi, C
47Fegan, S J
48Focke, W B
49Fortin, P
50Frailis, M
51Fukazawa, Y
52Funk, S
53Fusco, P
54Gargano, F
55Gasparrini, D
56Gehrels, N
57Germani, S
58Giglietto, N
59Giordano, F
60Glanzman, T
61Godfrey, G
62Grenier, I A
63Grove, J E
64Guillemot, L
65Guiriec, S
66Gustafsson, M
67Hadasch, D
68Harding, A K
69Horan, D
70Hughes, R E
71Jackson, M S
72Jóhannesson, G
73Johnson, A S
74Johnson, R P
75Johnson, W N
76Kamae, T
77Katagiri, H
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81Knödlseder, J
82Kuss, M
83Lande, J
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85Llena Garde, M
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88Lott, B
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91Makeev, A
92Mazziotta, M N
93McEnery, J E
94Meurer, C
95Michelson, P F
96Mitthumsiri, W
97Mizuno, T
98Moiseev, A A
99Monte, C
100...
titleFermi large area telescope search for photon lines from 30 to 200 GeV and dark matter implications
descriptionDark matter (DM) particle annihilation or decay can produce monochromatic gamma rays readily distinguishable from astrophysical sources. gamma-ray line limits from 30 to 200 GeV obtained from 11 months of Fermi Large Area Space Telescope data from 20-300 GeV are presented using a selection based on requirements for a gamma-ray line analysis, and integrated over most of the sky. We obtain gamma-ray line flux upper limits in the range 0.6-4.5x10{-9} cm{-2} s{-1}, and give corresponding DM annihilation cross-section and decay lifetime limits. Theoretical implications are briefly discussed.
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titleFermi large area telescope search for photon lines from 30 to 200 GeV and dark matter implications
authorAbdo, A A ; Ackermann, M ; Ajello, M ; Atwood, W B ; Baldini, L ; Ballet, J ; Barbiellini, G ; Bastieri, D ; Bechtol, K ; Bellazzini, R ; Berenji, B ; Bloom, E D ; Bonamente, E ; Borgland, A W ; Bouvier, A ; Bregeon, J ; Brez, A ; Brigida, M ; Bruel, P ; Burnett, T H ; Buson, S ; Caliandro, G A ; Cameron, R A ; Caraveo, P A ; Carrigan, S ; Casandjian, J M ; Cecchi, C ; Celik, O ; Chekhtman, A ; Chiang, J ; Ciprini, S ; Claus, R ; Cohen-Tanugi, J ; Conrad, J ; Dermer, C D ; De Angelis, A ; De Palma, F ; Digel, S W ; Do Couto E Silva, E ; Drell, P S ; Drlica-Wagner, A ; Dubois, R ; Dumora, D ; Edmonds, Y ; Essig, R ; Farnier, C ; Favuzzi, C ; Fegan, S J ; Focke, W B ; Fortin, P ; Frailis, M ; Fukazawa, Y ; Funk, S ; Fusco, P ; Gargano, F ; Gasparrini, D ; Gehrels, N ; Germani, S ; Giglietto, N ; Giordano, F ; Glanzman, T ; Godfrey, G ; Grenier, I A ; Grove, J E ; Guillemot, L ; Guiriec, S ; Gustafsson, M ; Hadasch, D ; Harding, A K ; Horan, D ; Hughes, R E ; Jackson, M S ; Jóhannesson, G ; Johnson, A S ; Johnson, R P ; Johnson, W N ; Kamae, T ; Katagiri, H ; Kataoka, J ; Kawai, N ; Kerr, M ; Knödlseder, J ; Kuss, M ; Lande, J ; Latronico, L ; Llena Garde, M ; Longo, F ; Loparco, F ; Lott, B ; Lovellette, M N ; Lubrano, P ; Makeev, A ; Mazziotta, M N ; Mcenery, J E ; Meurer, C ; Michelson, P F ; Mitthumsiri, W ; Mizuno, T ; Moiseev, A A ; Monte, C ; Monzani, M E ; Morselli, A ; Moskalenko, I V ; Murgia, S ; Nolan, P L ; Norris, J P ; Nuss, E ; Ohsugi, T ; Omodei, N ; Orlando, E ; Ormes, J F ; Ozaki, M ; Paneque, D ; Panetta, J H ; Parent, D ; Pelassa, V ; Pepe, M ; Pesce-Rollins, M ; Piron, F ; Rainò, S ; Rando, R ; Razzano, M ; Reimer, A ; Reimer, O ; Reposeur, T ; Ripken, J ; Ritz, S ; Rodriguez, A Y ; Roth, M ; Sadrozinski, H F-W ; Sander, A ; Parkinson, P M Saz ; Scargle, J D ; Schalk, T L ; Sellerholm, A ; Sgrò, C ; Siskind, E J ; Smith, D A ; Smith, P D ; Spandre, G ; Spinelli, P ; Starck, J-L ; Strickman, M S ; Suson, D J ; Tajima, H ; Takahashi, H ; Tanaka, T ; Thayer, J B ; Thayer, J G ; Tibaldo, L ; Torres, D F ; Uchiyama, Y ; Usher, T L ; Vasileiou, V ; Vilchez, N ; Vitale, V ; Waite, A P ; Wang, P ; Winer, B L ; Wood, K S ; Ylinen, T ; Ziegler, M
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45P L
46J P
47J F
48J H
49V
50A Y
51H F-W
52P M Saz
53J D
54T L
55E J
56D A
57P D
58J-L
59D J
60J B
61J G
62D F
63A P
64B L
65K S
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atitleFermi large area telescope search for photon lines from 30 to 200 GeV and dark matter implications
jtitlePhysical review letters
risdate20100305
volume104
issue9
spage091302
pages091302
eissn1079-7114
formatjournal
genrearticle
ristypeJOUR
abstractDark matter (DM) particle annihilation or decay can produce monochromatic gamma rays readily distinguishable from astrophysical sources. gamma-ray line limits from 30 to 200 GeV obtained from 11 months of Fermi Large Area Space Telescope data from 20-300 GeV are presented using a selection based on requirements for a gamma-ray line analysis, and integrated over most of the sky. We obtain gamma-ray line flux upper limits in the range 0.6-4.5x10{-9} cm{-2} s{-1}, and give corresponding DM annihilation cross-section and decay lifetime limits. Theoretical implications are briefly discussed.
pmid20366979
doi10.1103/PhysRevLett.104.091302
orcidid0000-0002-0014-7809: 0000-0001-6885-7156
issn00319007
oafree_for_read
date2010-03-05