Journal articles
Constraining Dark Matter Models from a Combined Analysis of MilkyWay Satellites with the Fermi Large Area Telescope
Markus Ackermann
Marco Ajello
A. Albert
W. B. Atwood
Luca Baldini
Jean Ballet
1
Guido Barbiellini
D. Bastieri
K. Bechtol
R. Bellazzini
B. Berenji
R. D. Blandford
E. D. Bloom
E. Bonamente
A.W. Borgland
J. Bregeon
M. Brigida
Pascal Bruel
2
R. Buehler
T. H. Burnett
S. Buson
G. A. Caliandro
R. A. Cameron
B. Can˜adas
P. A. Caraveo
J. M. Casandjian
1
C. Cecchi
E. Charles
A. Chekhtman
J. Chiang
S. Ciprini
R. Claus
J. Cohen-Tanugi
3
J. Conrad
S. Cutini
A. de Angelis
F. de Palma
C. D. Dermer
S.W. Digel
E. Do Couto E Silva
P. S. Drell
A. Drlica-Wagner
L. Falletti
C. Favuzzi
S. J. Fegan
2
E. C. Ferrara
Y. Fukazawa
S. Funk
P. Fusco
F. Gargano
D. Gasparrini
N. Gehrels
S. Germani
N. Giglietto
F. Giordano
M. Giroletti
T. Glanzman
G. Godfrey
I. A. Grenier
1
S. Guiriec
M. Gustafsson
D. Hadasch
M. Hayashida
E. Hays
R. E. Hughes
T. E. Jeltema
G. Jo'Hannesson
R. P. Johnson
A. S. Johnson
T. Kamae
H. Katagiri
J. Kataoka
J. Kno¨dlseder
M. Kuss
J. Lande
L. Latronico
A. M. Lionetto
M. Llena Garde
F. Longo
F. Loparco
B. Lott
4
M. N. Lovellette
P. Lubrano
G. M. Madejski
M. N. Mazziotta
J. E. Mcenery
J. Mehault
3
P. F. Michelson
W. Mitthumsiri
T. Mizuno
C. Monte
M. E. Monzani
A. Morselli
I.V. Moskalenko
S. Murgia
M. Naumann-Godo
1
J. P. Norris
E. Nuss
3
T. Ohsugi
A. Okumura
N. Omodei
E. Orlando
J. F. Ormes
M. Ozaki
D. Paneque
D. Parent
M. Pesce-Rollins
M. Pierbattista
1
F. Piron
3
G. Pivato
T.A. Porter
S. Profumo
S. Raino'
M. Razzano
A. Reimer
O. Reimer
S. Ritz
M. Roth
H. F.-W. Sadrozinski
C. Sbarra
J. D. Scargle
T. L. Schalk
C. Sgro'
E. J. Siskind
G. Spandre
P. Spinelli
L. Strigari
D. J. Suson
H. Tajima
H. Takahashi
T. Tanaka
J. G. Thayer
J. B. Thayer
D. J. Thompson
L. Tibaldo
M. Tinivella
D. F. Torres
E. Troja
Y. Uchiyama
J. Vandenbroucke
V. Vasileiou
3
G. Vianello
V. Vitale
A. P. Waite
P. Wang
B. L. Winer
K. S. Wood
M. Wood
Z. Yang
S. Zimmer
Luca Baldini
Author
Jean Ballet 1
Author Employer institution : Département de Physique Nucléaire (ex SPhN)
Guido Barbiellini
Author
D. Bastieri
Author
E. D. Bloom
Author
E. Bonamente
Author
A.W. Borgland
Author
J. Bregeon
Author IdHAL : johan-bregeon arXiv : https://arxiv.org/a/bregeon ORCID : https://orcid.org/0000-0002-6790-5328
M. Brigida
Author
Pascal Bruel 2
Author Employer institution : Centre National de la Recherche Scientifique
R. Buehler
Author
T. H. Burnett
Author
J. Cohen-Tanugi 3
Author IdHAL : johann-cohen-tanugi arXiv : https://arxiv.org/a/johannct ORCID : https://orcid.org/0000-0001-9022-4232
J. Conrad
Author
S. Cutini
Author
A. de Angelis
Author
J. Kno¨dlseder
Author IdHAL : jurgen-knodlseder ORCID : https://orcid.org/0000-0002-0014-7809
M. Kuss
Author
J. Lande
Author
L. Latronico
Author
B. Lott 4
Author IdHAL : benoit-lott ORCID : https://orcid.org/0000-0003-2186-9242
M. N. Lovellette
Author
P. Lubrano
Author
G. M. Madejski
Author
F. Piron 3
Author IdHAL : frederic-piron ORCID : https://orcid.org/0000-0001-6885-7156
G. Pivato
Author
T.A. Porter
Author
S. Profumo
Author
1
AIM (UMR_7158 / UMR_E_9005 / UM_112) - Astrophysique Interprétation Modélisation (AIM - UMR 7158 - UMR E 9005,
ex "Astrophysique Interactions Multi-échelles",
Service d'astrophysique,
CEA/Saclay,
Orme des Merisiers
F-91191 GIF SUR YVETTE CEDEX - France)
- CNRS - Centre National de la Recherche Scientifique : UMR_7158 (France)
- INSU - CNRS - Institut national des sciences de l'Univers (INSU-CNRS 3 rue Michel-Ange, 75794 Paris Cedex 16 - France)
- CEA - Commissariat à l'énergie atomique et aux énergies alternatives : UMR_E_9005 (Centre de Saclay Centre de Grenoble Centre de Cadarache etc - France)
- UPD7 - Université Paris Diderot - Paris 7 : UMR_7158 (5 rue Thomas-Mann - 75205 Paris cedex 13 - France)
2
LLR - Laboratoire Leprince-Ringuet (Route de Saclay - 91128 Palaiseau Cedex - France)
- CNRS - Centre National de la Recherche Scientifique : UMR7638 (France)
- X - École polytechnique (École polytechnique, 91128 Palaiseau Cedex - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
3
LUPM - Laboratoire Univers et Particules de Montpellier (Université de Montpellier Place Eugène Bataillon - CC 72 34095 Montpellier Cédex 05 - France)
- UM - Université de Montpellier (163 rue Auguste Broussonnet - 34090 Montpellier - France)
- UM2 - Université Montpellier 2 - Sciences et Techniques (Place Eugène Bataillon - 34095 Montpellier cedex 5 - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- CNRS - Centre National de la Recherche Scientifique : UMR5299 (France)
4
GLAST (France)
- CENBG - Centre d'Etudes Nucléaires de Bordeaux Gradignan (Chemin du Solarium - BP 120 - 33175 Gradignan Cedex - France)
- Université Sciences et Technologies - Bordeaux 1 (351 cours de la Libération - 33405 Talence cedex - France)
- IN2P3 - Institut National de Physique Nucléaire et de Physique des Particules du CNRS (France)
- CNRS - Centre National de la Recherche Scientifique : UMR5797 (France)
Abstract : Satellite galaxies of the Milky Way are among the most promising targets for dark matter searches in gamma rays. We present a search for dark matter consisting of weakly interacting massive particles, applying a joint likelihood analysis to 10 satellite galaxies with 24 months of data of the Fermi Large Area Telescope. No dark matter signal is detected. Including the uncertainty in the dark matter distribution, robust upper limits are placed on dark matter annihilation cross sections. The 95% confidence level upper limits range from about 10 26 cm3 s 1 at 5 GeV to about 5 10 23 cm3 s 1 at 1 TeV, depending on the dark matter annihilation final state. For the first time, using gamma rays, we are able to rule out models with the most generic cross section ( 3 10 26 cm3 s 1 for a purely s-wave cross section), without assuming additional boost factors.
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Journal articles
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http://hal.in2p3.fr/in2p3-00657896
Contributor : Nathalie Martin <>
Submitted on : Tuesday, January 10, 2012 - 11:17:25 AM
Last modification on : Friday, December 18, 2020 - 12:54:07 PM
Contributor : Nathalie Martin <>
Submitted on : Tuesday, January 10, 2012 - 11:17:25 AM
Last modification on : Friday, December 18, 2020 - 12:54:07 PM
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- HAL Id : in2p3-00657896, version 1
- DOI : 10.1103/PhysRevLett.107.241302
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CEA | INSU | IN2P3 | CENBG | LLR | CNRS | X | X-LLR | LUPM | MIPS | DSM-IRFU | IRFU-AIM | UNIV-MONTPELLIER | CEA-DRF | X-DEP-PHYS | UNIV-PARIS7 | USPC | LUPM_EMA | UNIV-PARIS | UP-SCIENCES
Citation
Markus Ackermann, Marco Ajello, A. Albert, W. B. Atwood, Luca Baldini, et al.. Constraining Dark Matter Models from a Combined Analysis of MilkyWay Satellites with the Fermi Large Area Telescope. Physical Review Letters, American Physical Society, 2011, 107, pp.241302. ⟨10.1103/PhysRevLett.107.241302⟩. ⟨in2p3-00657896⟩
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