Dark matter particle annihilation or decay can produce monochromatic gamma-ray lines and contribute to the diffuse gamma-ray background. Flux upper limits are presented for gamma-ray spectral lines from 7 to 200 GeV and for the diffuse gamma-ray background from 4.8 GeV to 264 GeV obtained from two years of Fermi Large Area Telescope data integrated over most of the sky. We give cross- section upper limits and decay lifetime lower limits for dark matter models that produce gamma-ray lines or contribute to the diffuse spectrum, including models proposed as explanations of the PAMELA and Fermi cosmic-ray data.

Fermi LAT search for dark matter in gamma-ray lines and the inclusive photon spectrum / Ackermann M; Ajello M; Albert A; Baldini L; Barbiellini G; Bechtol K; Bellazzini R; Berenji B; Blandford R D; Bloom E D; Bonamente E; Borgland A W; Brigida M; Buehler R; Buson S; Caliandro G A; Cameron R A; Caraveo P A; Casandjian J M; Cecchi C; Charles E; Chekhtman A; Chiang J; Ciprini S; Claus R; Cohen-Tanugi J; Conrad J; DAmmando F; de Palma F; Dermer C D; do Couto e Silva E; Drell P S; Drlica-Wagner A; Edmonds Y; Essig R; Favuzzi C; Fegan S J; Focke W B; Fukazawa Y; Funk S; Fusco P; Gargano F; Gasparrini D; Germani S; Giglietto N; Giordano F; Giroletti M; Glanzman T; Godfrey G; Grenier I A; Guiriec S; Gustafsson M; Hadasch D; Hayashida M; Horan D; Hughes R E; Kamae T; Knödlseder J; Kuss M; Lande J; Lionetto A M; Llena Garde M; Longo F; Loparco F; Lovellette M N; Lubrano P; Mazziotta M N; Michelson P F; Mitthumsiri W; Mizuno T; Moiseev A A; Monte C; Monzani M E; Morselli A; Moskalenko I V; Murgia S; Naumann-Godo M; Norris J P; Nuss E; Ohsugi T; Okumura A; Orlando E; Ormes J F; Paneque D; Panetta J H; Pesce-Rollins M; Piron F; Pivato G; Porter T A; Prokhorov D; Rainò S; Rando R; Razzano M; Reimer O; Roth M; Sbarra C; Scargle J D; Sgrò C; Siskind E J; Snyder A; Spinelli P; Suson D J; Takahashi H; Tanaka T; Thayer J G; Thayer J B; Tibaldo L; Tinivella M; Torres D F; Tosti G; Troja E; Vandenbroucke J; Vasileiou V; Vianello G; Vitale V; Waite A P; Winer B L; Wood K S; Yang Z; Zimmer S. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - STAMPA. - 86:2(2012), pp. 022002.1-022002.21. [10.1103/PhysRevD.86.022002]

Fermi LAT search for dark matter in gamma-ray lines and the inclusive photon spectrum

D'AMMANDO, FILIPPO;
2012

Abstract

Dark matter particle annihilation or decay can produce monochromatic gamma-ray lines and contribute to the diffuse gamma-ray background. Flux upper limits are presented for gamma-ray spectral lines from 7 to 200 GeV and for the diffuse gamma-ray background from 4.8 GeV to 264 GeV obtained from two years of Fermi Large Area Telescope data integrated over most of the sky. We give cross- section upper limits and decay lifetime lower limits for dark matter models that produce gamma-ray lines or contribute to the diffuse spectrum, including models proposed as explanations of the PAMELA and Fermi cosmic-ray data.
2012
Fermi LAT search for dark matter in gamma-ray lines and the inclusive photon spectrum / Ackermann M; Ajello M; Albert A; Baldini L; Barbiellini G; Bechtol K; Bellazzini R; Berenji B; Blandford R D; Bloom E D; Bonamente E; Borgland A W; Brigida M; Buehler R; Buson S; Caliandro G A; Cameron R A; Caraveo P A; Casandjian J M; Cecchi C; Charles E; Chekhtman A; Chiang J; Ciprini S; Claus R; Cohen-Tanugi J; Conrad J; DAmmando F; de Palma F; Dermer C D; do Couto e Silva E; Drell P S; Drlica-Wagner A; Edmonds Y; Essig R; Favuzzi C; Fegan S J; Focke W B; Fukazawa Y; Funk S; Fusco P; Gargano F; Gasparrini D; Germani S; Giglietto N; Giordano F; Giroletti M; Glanzman T; Godfrey G; Grenier I A; Guiriec S; Gustafsson M; Hadasch D; Hayashida M; Horan D; Hughes R E; Kamae T; Knödlseder J; Kuss M; Lande J; Lionetto A M; Llena Garde M; Longo F; Loparco F; Lovellette M N; Lubrano P; Mazziotta M N; Michelson P F; Mitthumsiri W; Mizuno T; Moiseev A A; Monte C; Monzani M E; Morselli A; Moskalenko I V; Murgia S; Naumann-Godo M; Norris J P; Nuss E; Ohsugi T; Okumura A; Orlando E; Ormes J F; Paneque D; Panetta J H; Pesce-Rollins M; Piron F; Pivato G; Porter T A; Prokhorov D; Rainò S; Rando R; Razzano M; Reimer O; Roth M; Sbarra C; Scargle J D; Sgrò C; Siskind E J; Snyder A; Spinelli P; Suson D J; Takahashi H; Tanaka T; Thayer J G; Thayer J B; Tibaldo L; Tinivella M; Torres D F; Tosti G; Troja E; Vandenbroucke J; Vasileiou V; Vianello G; Vitale V; Waite A P; Winer B L; Wood K S; Yang Z; Zimmer S. - In: PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY. - ISSN 1550-7998. - STAMPA. - 86:2(2012), pp. 022002.1-022002.21. [10.1103/PhysRevD.86.022002]
Ackermann M; Ajello M; Albert A; Baldini L; Barbiellini G; Bechtol K; Bellazzini R; Berenji B; Blandford R D; Bloom E D; Bonamente E; Borgland A W; Brigida M; Buehler R; Buson S; Caliandro G A; Cameron R A; Caraveo P A; Casandjian J M; Cecchi C; Charles E; Chekhtman A; Chiang J; Ciprini S; Claus R; Cohen-Tanugi J; Conrad J; DAmmando F; de Palma F; Dermer C D; do Couto e Silva E; Drell P S; Drlica-Wagner A; Edmonds Y; Essig R; Favuzzi C; Fegan S J; Focke W B; Fukazawa Y; Funk S; Fusco P; Gargano F; Gasparrini D; Germani S; Giglietto N; Giordano F; Giroletti M; Glanzman T; Godfrey G; Grenier I A; Guiriec S; Gustafsson M; Hadasch D; Hayashida M; Horan D; Hughes R E; Kamae T; Knödlseder J; Kuss M; Lande J; Lionetto A M; Llena Garde M; Longo F; Loparco F; Lovellette M N; Lubrano P; Mazziotta M N; Michelson P F; Mitthumsiri W; Mizuno T; Moiseev A A; Monte C; Monzani M E; Morselli A; Moskalenko I V; Murgia S; Naumann-Godo M; Norris J P; Nuss E; Ohsugi T; Okumura A; Orlando E; Ormes J F; Paneque D; Panetta J H; Pesce-Rollins M; Piron F; Pivato G; Porter T A; Prokhorov D; Rainò S; Rando R; Razzano M; Reimer O; Roth M; Sbarra C; Scargle J D; Sgrò C; Siskind E J; Snyder A; Spinelli P; Suson D J; Takahashi H; Tanaka T; Thayer J G; Thayer J B; Tibaldo L; Tinivella M; Torres D F; Tosti G; Troja E; Vandenbroucke J; Vasileiou V; Vianello G; Vitale V; Waite A P; Winer B L; Wood K S; Yang Z; Zimmer S
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/595733
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