C B Rulten
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Explore the profile of C B Rulten including associated specialties, affiliations and a list of published articles.
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Articles
9
Citations
16
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Recent Articles
1.
Abdallah H, Abramowski A, Aharonian F, Benkhali F, Anguner E, Arakawa M, et al.
Phys Rev Lett
. 2018 Jun;
120(20):201101.
PMID: 29864326
Spectral lines are among the most powerful signatures for dark matter (DM) annihilation searches in very-high-energy γ rays. The central region of the Milky Way halo is one of the...
2.
Abdalla H, Abramowski A, Aharonian F, Benkhali F, Akhperjanian A, Andersson T, et al.
Phys Rev Lett
. 2016 Oct;
117(15):151302.
PMID: 27768338
Results: No significant excess associated with dark matter annihilations was found in the energy range of 100 GeV to 2 TeV and upper limits on the gamma-ray flux and the...
3.
Abdallah H, Abramowski A, Aharonian F, Benkhali F, Akhperjanian A, Anguner E, et al.
Phys Rev Lett
. 2016 Sep;
117(11):111301.
PMID: 27661677
The inner region of the Milky Way halo harbors a large amount of dark matter (DM). Given its proximity, it is one of the most promising targets to look for...
4.
Abramowski A, Aharonian F, Benkhali F, Akhperjanian A, Anguner E, Backes M, et al.
Phys Rev Lett
. 2015 Mar;
114(8):081301.
PMID: 25768750
An annihilation signal of dark matter is searched for from the central region of the Milky Way. Data acquired in dedicated on-off observations of the Galactic center region with H.E.S.S....
5.
Abramowski A, Acero F, Aharonian F, Akhperjanian A, Anton G, Balenderan S, et al.
Phys Rev Lett
. 2014 Aug;
110(4):041301.
PMID: 25166149
Gamma-ray line signatures can be expected in the very-high-energy (E(γ)>100 GeV) domain due to self-annihilation or decay of dark matter (DM) particles in space. Such a signal would be readily...
6.
Abramowski A, Acero F, Aharonian F, Akhperjanian A, Anton G, Barnacka A, et al.
Phys Rev Lett
. 2011 May;
106(16):161301.
PMID: 21599352
A search for a very-high-energy (VHE; ≥100 GeV) γ-ray signal from self-annihilating particle dark matter (DM) is performed towards a region of projected distance r∼45-150 pc from the Galactic center....
7.
Acero F, Aharonian F, Akhperjanian A, Anton G, Barres de Almeida U, Bazer-Bachi A, et al.
Science
. 2009 Sep;
326(5956):1080-2.
PMID: 19779150
Starburst galaxies exhibit in their central regions a highly increased rate of supernovae, the remnants of which are thought to accelerate energetic cosmic rays up to energies of approximately 10(15)...
8.
Acciari V, Aliu E, Arlen T, Bautista M, Beilicke M, Benbow W, et al.
Science
. 2009 Jul;
325(5939):444-8.
PMID: 19574351
The accretion of matter onto a massive black hole is believed to feed the relativistic plasma jets found in many active galactic nuclei (AGN). Although some AGN accelerate particles to...
9.
Aharonian F, Akhperjanian A, Barres de Almeida U, Bazer-Bachi A, Becherini Y, Behera B, et al.
Phys Rev Lett
. 2009 May;
101(26):261104.
PMID: 19437632
The very large collection area of ground-based gamma-ray telescopes gives them a substantial advantage over balloon or satellite based instruments in the detection of very-high-energy (>600 GeV) cosmic-ray electrons. Here...