schliessen

Filtern

 

Bibliotheken

Fermi LAT 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 GeV to 200 GeV obtained from 11 months of Fermi Large Area Space Telescope data from 20-300 GeV are presented using a selec... Full description

Journal Title: arXiv.org Jan 27, 2010
Main Author: Abdo, A
Other Authors: Ackermann, M , Ajello, M , Atwood, W , Baldini, L , Ballet, J , Barbiellini, G , Bastieri, D , Bechtol, K , Bellazzini, R , Berenji, B , Bloom, E , Bonamente, E , Borgland, A , Bouvier, A , Bregeon, J , Brez, A , Brigida, M , Bruel, P , Burnett
Format: Electronic Article Electronic Article
Language: English
Subjects:
ID: DOI: 10.1103/PhysRevLett.104.091302
Zum Text:
SendSend as email Add to Book BagAdd to Book Bag
Staff View
recordid: proquest2086319609
title: Fermi LAT Search for Photon Lines from 30 to 200 GeV and Dark Matter Implications
format: Article
creator:
  • Abdo, A
  • Ackermann, M
  • Ajello, M
  • Atwood, W
  • Baldini, L
  • Ballet, J
  • Barbiellini, G
  • Bastieri, D
  • Bechtol, K
  • Bellazzini, R
  • Berenji, B
  • Bloom, E
  • Bonamente, E
  • Borgland, A
  • Bouvier, A
  • Bregeon, J
  • Brez, A
  • Brigida, M
  • Bruel, P
  • Burnett
subjects:
  • Space Telescopes
  • Dark Matter
  • Particle Decay
  • High Energy Astrophysical Phenomena
  • Cosmology and Nongalactic Astrophysics
ispartof: arXiv.org, Jan 27, 2010
description: Dark matter (DM) particle annihilation or decay can produce monochromatic \(\gamma\)-rays readily distinguishable from astrophysical sources. \(\gamma\)-ray line limits from 30 GeV 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 \(0.6-4.5\times 10^{-9}\mathrm{cm}^{-2}\mathrm{s}^{-1}\), and give corresponding DM annihilation cross-section and decay lifetime limits. Theoretical implications are briefly discussed.
language: eng
source:
identifier: DOI: 10.1103/PhysRevLett.104.091302
fulltext: fulltext_linktorsrc
url: Link


@attributes
ID917847720
RANK0.07
NO1
SEARCH_ENGINEprimo_central_multiple_fe
SEARCH_ENGINE_TYPEPrimo Central Search Engine
LOCALfalse
PrimoNMBib
record
control
sourcerecordid2086319609
sourceidproquest
recordidTN_proquest2086319609
sourcesystemPC
pqid2086319609
display
typearticle
titleFermi LAT Search for Photon Lines from 30 to 200 GeV and Dark Matter Implications
creatorAbdo, A ; Ackermann, M ; Ajello, M ; Atwood, W ; Baldini, L ; Ballet, J ; Barbiellini, G ; Bastieri, D ; Bechtol, K ; Bellazzini, R ; Berenji, B ; Bloom, E ; Bonamente, E ; Borgland, A ; Bouvier, A ; Bregeon, J ; Brez, A ; Brigida, M ; Bruel, P ; Burnett
contributorZiegler, M (pacrepositoryorg)
ispartofarXiv.org, Jan 27, 2010
identifierDOI: 10.1103/PhysRevLett.104.091302
subjectSpace Telescopes ; Dark Matter ; Particle Decay ; High Energy Astrophysical Phenomena ; Cosmology and Nongalactic Astrophysics
descriptionDark matter (DM) particle annihilation or decay can produce monochromatic \(\gamma\)-rays readily distinguishable from astrophysical sources. \(\gamma\)-ray line limits from 30 GeV 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 \(0.6-4.5\times 10^{-9}\mathrm{cm}^{-2}\mathrm{s}^{-1}\), and give corresponding DM annihilation cross-section and decay lifetime limits. Theoretical implications are briefly discussed.
languageeng
source
version8
oafree_for_read
lds50peer_reviewed
links
openurl$$Topenurl_article
openurlfulltext$$Topenurlfull_article
linktorsrc$$Uhttp://search.proquest.com/docview/2086319609/?pq-origsite=primo$$EView_record_in_ProQuest_(subscribers_only)
search
creatorcontrib
0Abdo, A
1Ackermann, M
2Ajello, M
3Atwood, W
4Baldini, L
5Ballet, J
6Barbiellini, G
7Bastieri, D
8Bechtol, K
9Bellazzini, R
10Berenji, B
11Bloom, E
12Bonamente, E
13Borgland, A
14Bouvier, A
15Bregeon, J
16Brez, A
17Brigida, M
18Bruel, P
19Burnett, T
20Buson, S
21Caliandro, G
22Cameron, R
23Caraveo, P
24Carrigan, S
25Casandjian, J
26Cecchi, C
27Elik, O
28Chekhtman, A
29Chiang, J
30Ciprini, S
31Claus, R
32Cohen-Tanugi, J
33Conrad, J
34Dermer, C
35de Angelis, A
36de Palma, F
37Digel, S
38Drell, P
39Drlica-Wagner, A
40Dubois, R
41Dumora, D
42Edmonds, Y
43Essig, R
44Farnier, C
45Favuzzi, C
46Fegan, S
47Focke, W
48Fortin, P
49Frailis, M
50Fukazawa, Y
51Funk, S
52Fusco, P
53Gargano, F
54Gasparrini, D
55Gehrels, N
56Germani, S
57Giglietto, N
58Giordano, F
59Glanzman, T
60Godfrey, G
61Grenier, I
62Grove, J
63Guillemot, L
64Guiriec, S
65Gustafsson, M
66Hadasch, D
67Harding, A
68Horan, D
69Hughes, R
70Jackson, M
71Ohannesson, G
72Johnson, A
73Johnson, R
74Johnson, W
75Kamae, T
76Katagiri, H
77Kataoka, J
78Kawai, N
79Kerr, M
80Dlseder, J
81Kuss, M
82Lande, J
83Latronico, L
84Longo, F
85Loparco, F
86Lott, B
87Lovellette, M
88Lubrano, P
89Makeev, A
90Mazziotta, M
91Mcenery, J
92Meurer, C
93Michelson, P
94Mitthumsiri, W
95Mizuno, T
96Moiseev, A
97Monte, C
98Monzani, M
99Morselli, A
100...
titleFermi LAT 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 GeV 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 \(0.6-4.5\times 10^{-9}\mathrm{cm}^{-2}\mathrm{s}^{-1}\), and give corresponding DM annihilation cross-section and decay lifetime limits. Theoretical implications are briefly discussed.
subject
0Space Telescopes
1Dark Matter
2Particle Decay
3High Energy Astrophysical Phenomena
4Cosmology and Nongalactic Astrophysics
general
0English
1Cornell University Library, arXiv.org
210.1103/PhysRevLett.104.091302
3Engineering Database
4Publicly Available Content Database
5ProQuest Engineering Collection
6ProQuest Technology Collection
7ProQuest SciTech Collection
8Materials Science & Engineering Database
9ProQuest Central (new)
10ProQuest Central Korea
11SciTech Premium Collection
12Technology Collection
13ProQuest Central Essentials
14ProQuest One Academic
15Engineering Collection (ProQuest)
sourceidproquest
recordidproquest2086319609
rsrctypearticle
creationdate2010
addtitlearXiv.org
searchscope
01007853
11008875
21008886
31009127
41009240
510000041
610000053
710000120
810000250
910000255
1010000256
1110000258
1210000260
1310000265
1410000268
1510000281
1610000348
1710000356
1810000360
19proquest
scope
01007853
11008875
21008886
31009127
41009240
510000041
610000053
710000120
810000250
910000255
1010000256
1110000258
1210000260
1310000265
1410000268
1510000281
1610000348
1710000356
1810000360
19proquest
lsr43
01007853true
11008875true
21008886true
31009127true
41009240true
510000041true
610000053true
710000120true
810000250true
910000255true
1010000256true
1110000258true
1210000260true
1310000265true
1410000268true
1510000281true
1610000348true
1710000356true
1810000360true
startdate20100127
enddate20100127
lsr30VSR-Enriched:[eissn, vol, pages, pqid, orcidid, issn, issue]
sort
titleFermi LAT Search for Photon Lines from 30 to 200 GeV and Dark Matter Implications
authorAbdo, A ; Ackermann, M ; Ajello, M ; Atwood, W ; Baldini, L ; Ballet, J ; Barbiellini, G ; Bastieri, D ; Bechtol, K ; Bellazzini, R ; Berenji, B ; Bloom, E ; Bonamente, E ; Borgland, A ; Bouvier, A ; Bregeon, J ; Brez, A ; Brigida, M ; Bruel, P ; Burnett
creationdate20100127
lso0120100127
facets
frbrgroupid1560913599114439166
frbrtype5
newrecords20180917
languageeng
creationdate2010
topic
0Space Telescopes
1Dark Matter
2Particle Decay
3High Energy Astrophysical Phenomena
4Cosmology and Nongalactic Astrophysics
collection
0Engineering Database
1Publicly Available Content Database
2ProQuest Engineering Collection
3ProQuest Technology Collection
4ProQuest SciTech Collection
5Materials Science & Engineering Database
6ProQuest Central (new)
7ProQuest Central Korea
8SciTech Premium Collection
9Technology Collection
10ProQuest Central Essentials
11ProQuest One Academic
12Engineering Collection (ProQuest)
prefilterarticles
rsrctypearticles
creatorcontrib
0Abdo, A
1Ackermann, M
2Ajello, M
3Atwood, W
4Baldini, L
5Ballet, J
6Barbiellini, G
7Bastieri, D
8Bechtol, K
9Bellazzini, R
10Berenji, B
11Bloom, E
12Bonamente, E
13Borgland, A
14Bouvier, A
15Bregeon, J
16Brez, A
17Brigida, M
18Bruel, P
19Burnett, T
20Buson, S
21Caliandro, G
22Cameron, R
23Caraveo, P
24Carrigan, S
25Casandjian, J
26Cecchi, C
27Elik, O
28Chekhtman, A
29Chiang, J
30Ciprini, S
31Claus, R
32Cohen-Tanugi, J
33Conrad, J
34Dermer, C
35de Angelis, A
36de Palma, F
37Digel, S
38Drell, P
39Drlica-Wagner, A
40Dubois, R
41Dumora, D
42Edmonds, Y
43Essig, R
44Farnier, C
45Favuzzi, C
46Fegan, S
47Focke, W
48Fortin, P
49Frailis, M
50Fukazawa, Y
51Funk, S
52Fusco, P
53Gargano, F
54Gasparrini, D
55Gehrels, N
56Germani, S
57Giglietto, N
58Giordano, F
59Glanzman, T
60Godfrey, G
61Grenier, I
62Grove, J
63Guillemot, L
64Guiriec, S
65Gustafsson, M
66Hadasch, D
67Harding, A
68Horan, D
69Hughes, R
70Jackson, M
71Ohannesson, G
72Johnson, A
73Johnson, R
74Johnson, W
75Kamae, T
76Katagiri, H
77Kataoka, J
78Kawai, N
79Kerr, M
80Dlseder, J
81Kuss, M
82Lande, J
83Latronico, L
84Longo, F
85Loparco, F
86Lott, B
87Lovellette, M
88Lubrano, P
89Makeev, A
90Mazziotta, M
91Mcenery, J
92Meurer, C
93Michelson, P
94Mitthumsiri, W
95Mizuno, T
96Moiseev, A
97Monte, C
98Monzani, M
99Morselli, A
100...
jtitlearXiv.org
toplevelpeer_reviewed
delivery
delcategoryRemote Search Resource
fulltextfulltext_linktorsrc
addata
aulast
0Abdo
1Ackermann
2Ajello
3Atwood
4Baldini
5Ballet
6Barbiellini
7Bastieri
8Bechtol
9Bellazzini
10Berenji
11Bloom
12Bonamente
13Borgland
14Bouvier
15Bregeon
16Brez
17Brigida
18Bruel
19Burnett
20Buson
21Caliandro
22Cameron
23Caraveo
24Carrigan
25Casandjian
26Cecchi
27Elik
28Chekhtman
29Chiang
30Ciprini
31Claus
32Cohen-Tanugi
33Conrad
34Dermer
35de Angelis
36de Palma
37Digel
38Drell
39Drlica-Wagner
40Dubois
41Dumora
42Edmonds
43Essig
44Farnier
45Favuzzi
46Fegan
47Focke
48Fortin
49Frailis
50Fukazawa
51Funk
52Fusco
53Gargano
54Gasparrini
55Gehrels
56Germani
57Giglietto
58Giordano
59Glanzman
60Godfrey
61Grenier
62Grove
63Guillemot
64Guiriec
65Gustafsson
66Hadasch
67Harding
68Horan
69Hughes
70Jackson
71ohannesson
72Johnson
73Kamae
74Katagiri
75Kataoka
76Kawai
77Kerr
78dlseder
79Kuss
80Lande
81Latronico
82Longo
83Loparco
84Lott
85Lovellette
86Lubrano
87Makeev
88Mazziotta
89McEnery
90Meurer
91Michelson
92Mitthumsiri
93Mizuno
94Moiseev
95Monte
96Monzani
97Morselli
98Moskalenko
99Murgia
100...
aufirst
0A
1M
2W
3L
4J
5G
6D
7K
8R
9B
10E
11P
12T
13S
14C
15O
16F
17Y
18N
19I
20H
21V
au
0Abdo, A
1Ackermann, M
2Ajello, M
3Atwood, W
4Baldini, L
5Ballet, J
6Barbiellini, G
7Bastieri, D
8Bechtol, K
9Bellazzini, R
10Berenji, B
11Bloom, E
12Bonamente, E
13Borgland, A
14Bouvier, A
15Bregeon, J
16Brez, A
17Brigida, M
18Bruel, P
19Burnett, T
20Buson, S
21Caliandro, G
22Cameron, R
23Caraveo, P
24Carrigan, S
25Casandjian, J
26Cecchi, C
27Elik, O
28Chekhtman, A
29Chiang, J
30Ciprini, S
31Claus, R
32Cohen-Tanugi, J
33Conrad, J
34Dermer, C
35de Angelis, A
36de Palma, F
37Digel, S
38Drell, P
39Drlica-Wagner, A
40Dubois, R
41Dumora, D
42Edmonds, Y
43Essig, R
44Farnier, C
45Favuzzi, C
46Fegan, S
47Focke, W
48Fortin, P
49Frailis, M
50Fukazawa, Y
51Funk, S
52Fusco, P
53Gargano, F
54Gasparrini, D
55Gehrels, N
56Germani, S
57Giglietto, N
58Giordano, F
59Glanzman, T
60Godfrey, G
61Grenier, I
62Grove, J
63Guillemot, L
64Guiriec, S
65Gustafsson, M
66Hadasch, D
67Harding, A
68Horan, D
69Hughes, R
70Jackson, M
71Ohannesson, G
72Johnson, A
73Johnson, R
74Johnson, W
75Kamae, T
76Katagiri, H
77Kataoka, J
78Kawai, N
79Kerr, M
80Dlseder, J
81Kuss, M
82Lande, J
83Latronico, L
84Longo, F
85Loparco, F
86Lott, B
87Lovellette, M
88Lubrano, P
89Makeev, A
90Mazziotta, M
91Mcenery, J
92Meurer, C
93Michelson, P
94Mitthumsiri, W
95Mizuno, T
96Moiseev, A
97Monte, C
98Monzani, M
99Morselli, A
100...
atitleFermi LAT Search for Photon Lines from 30 to 200 GeV and Dark Matter Implications
jtitlearXiv.org
risdate20100127
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 GeV 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 \(0.6-4.5\times 10^{-9}\mathrm{cm}^{-2}\mathrm{s}^{-1}\), and give corresponding DM annihilation cross-section and decay lifetime limits. Theoretical implications are briefly discussed.
copIthaca
pubCornell University Library, arXiv.org
doi10.1103/PhysRevLett.104.091302
urlhttp://search.proquest.com/docview/2086319609/
volume104
pages091302
orcidid0000-0002-0014-7809: 0000-0001-6885-7156
issue9
eissn10797114
issn00319007
oafree_for_read
date2010-01-27