Pregled bibliografske jedinice broj: 673435
Optimized dark matter searches in deep observations of Segue 1 with MAGIC
Optimized dark matter searches in deep observations of Segue 1 with MAGIC // Journal of cosmology and astroparticle physics, (2014), 008-1 doi:10.1088/1475-7516/2014/02/008 (međunarodna recenzija, članak, znanstveni)
CROSBI ID: 673435 Za ispravke kontaktirajte CROSBI podršku putem web obrasca
Naslov
Optimized dark matter searches in deep observations of Segue 1 with MAGIC
Autori
Aleksić, Jelena ; ... ; Babić, Ana ; ... ; Dominis Prester, Dijana ; ... ; Ferenc, Daniel ; ... ; Godinović, Nikola ; ... ; Hrupec, Dario ; ... ; Lelas, Damir ; ... ; Puljak, Ivica ; ... ; Surić, Tihomir ; ... ; Šnidarić, Iva ; ... ; Terzić, Tomislav ; ...
Izvornik
Journal of cosmology and astroparticle physics (1475-7516)
(2014);
008-1
Vrsta, podvrsta i kategorija rada
Radovi u časopisima, članak, znanstveni
Ključne riječi
dark matter; indirect searches; gamma-ray experiments; Imaging Air Cherenkov Telescopes; dwarf spheroidal galaxies; Segue 1
Sažetak
We present the results of stereoscopic observations of the satellite galaxy Segue 1 with the MAGIC Telescopes, carried out between 2011 and 2013. With almost 160 hours of good- quality data, this is the deepest observational campaign on any dwarf galaxy performed so far in the very high energy range of the electromagnetic spectrum. We search this large data sample for signals of dark matter particles in the mass range between 100 GeV and 20 TeV. For this we use the full likelihood analysis method, which provides optimal sensitivity to characteristic gamma-ray spectral features, like those expected from dark matter annihilation or decay. In particular, we focus our search on gamma-rays produced from different final state Standard Model particles, annihilation with internal bremsstrahlung, monochromatic lines and box- shaped signals. Our results represent the most stringent constraints to the annihilation cross-section or decay lifetime obtained from observations of satellite galaxies, for masses above few hundred GeV. In particular, our strongest limit (95% confidence level) corresponds to a ~500 GeV dark matter particle annihilating into tau+tau-, and is of order <sigma v> ~ 1.2x10^{; ; ; ; ; ; -24}; ; ; ; ; ; cm^3 s^{; ; ; ; ; ; -1}; ; ; ; ; ; - a factor ~40 above the <sigma v> thermal value.
Izvorni jezik
Engleski
Znanstvena područja
Fizika
POVEZANOST RADA
Projekti:
HRZZ-09/176 - Visokoenergijska astronomija gama zraka teleskopima MAGIC (Godinović, Nikola, HRZZ ) ( CroRIS)
Ustanove:
Fakultet elektrotehnike, strojarstva i brodogradnje, Split,
Institut "Ruđer Bošković", Zagreb,
Sveučilište u Rijeci - Odjel za fiziku
Profili:
Dario Hrupec
(autor)
Damir Lelas
(autor)
Ivica Puljak
(autor)
Dijana Dominis Prester
(autor)
Iva Šnidarić
(autor)
Nikola Godinović
(autor)
Tomislav Terzić
(autor)
Ana Babić
(autor)
Daniel Ferenc
(autor)
Tihomir Surić
(autor)
Poveznice na cjeloviti tekst rada:
Pristup cjelovitom tekstu rada doi fulir.irb.hr
Citiraj ovu publikaciju:
Časopis indeksira:
- Current Contents Connect (CCC)
- Web of Science Core Collection (WoSCC)
- Science Citation Index Expanded (SCI-EXP)
- SCI-EXP, SSCI i/ili A&HCI
- Scopus