• Corpus ID: 240419823

Fundamental Physics Searches with IACTs

@inproceedings{Doro2021FundamentalPS,
  title={Fundamental Physics Searches with IACTs},
  author={Michele Doro and Miguel A. S'anchez-Conde and Moritz Hutten University of Padova and Dep. of Physics and Astronomy and Padova and Italy Instituto de F'isica Teorica and Ift UAM-CSIC and Departamento de F'isica Teorica and Universidad Aut'onoma de Madrid and Madrid and Spain Icrr and The University of Tokyo and Kashiwa and Chiba and Japan.},
  year={2021}
}
Michele Doro1, M.A. Sánchez-Conde2, M. Hütten3 1 University of Padova, Department of Physics and Astronomy, I-35131 Padova (Italy) michele. doro@unipd.it 2 Instituto de F́ısica Teórica, IFT UAM-CSIC, Departamento de F́ısica Teórica, Universidad Autónoma de Madrid, ES-28049 Madrid (Spain) miguel.sanchezconde@uam.es 3 Institute for Cosmic Ray Research, the University of Tokyo (Japan) huetten@icrr.u-tokyo.ac. jp 
Classification of gamma-ray targets for velocity-dependent and subhalo-boosted dark-matter annihilation
. Gamma-ray observations have long been used to constrain the properties of dark matter (DM), with a strong focus on weakly interacting massive particles annihilating through velocity-independent
TeV Dark Matter searches in the extragalactic gamma-ray sky
: High-energetic gamma rays from astrophysical targets constitute a unique probe for annihilation or decay of heavy particle Dark Matter (DM). After several decades, diverse null detections have
Gamma-Ray Cosmology and Tests of Fundamental Physics
The propagation of gamma-rays over cosmological distances is the subject of extensive theoretical and observational research at GeV and TeV energies. The mean free path of gamma-rays in the cosmic
Snowmass2021 Cosmic Frontier White Paper:Primordial Black Hole Dark Matter
Primordial Black Holes (PBHs) are a viable candidate to comprise some or all of the dark matter and provide a unique window into the high-energy physics of the early universe. This white paper
1 Production and evolution : modelling the EBL

References

SHOWING 1-10 OF 386 REFERENCES
Upper limits on the WIMP annihilation cross section from a joint analysis of dwarf spheroidal satellite galaxy observations with the MAGIC telescopes
Camilla Maggio,a,∗ Daniel Kerzsberg,b Daniele Nincic and Vincenzo Vitaled on behalf of the MAGIC Collaboration (a complete list of authors can be found at the end of the proceedings) Departament de
Trinity: an imaging air Cherenkov telescope to search for Ultra-High-Energy neutrinos.
Centre for Advanced Instrumentation, Durham University, South Road, Durham, DH1 3LE, UK Georgia Institute of Technology, School of Physics & Center for Relativistic Astrophysics, 837 State Street NW,
First results from the CERN axion solar telescope.
TLDR
An upper limit to the axion-photon coupling g(agamma)<1.16x10(-10) GeV-1 at 95% C.L. for m(a) less, similar to the limit from stellar energy-loss arguments and considerably more restrictive than any previous experiment over a broad range of axion masses.
Future axion searches with the International Axion Observatory (IAXO)
The International Axion Observatory (IAXO) is a new generation axion helioscope aiming at a sensitivity to the axion-photon coupling of gaγ ≳ few × 10−12 GeV−1, i.e. 1–1.5 orders of magnitude beyond
Near future MeV telescopes can discover asteroid-mass primordial black hole dark matter
Anupam Ray ID , a Ranjan Laha ID , b Julian B. Muñoz ID , c and Regina Caputo ID 4, d Tata Institute of Fundamental Research, Homi Bhabha Road, Mumbai 400005, India Centre for High Energy Physics,
Tau neutrino search with the MAGIC telescope
The MAGIC telescope located on the Roque de los Muchachos on the Canary Island La Palma at a height of 2200 m a.s.l. is able to point to the sea. This permits a search for air shower signatures
A Search for Dark Matter Annihilation with the Whipple 10m Telescope
Department of Physics and Astronomy, University of California, Los Angeles, CA 90095, USA Department of Physics, University of Massachussetts, Amherst, MA 01003-4525, USA School of Physics and
Sensitivity for tau neutrinos at PeV energies and beyond with the MAGIC telescopes
The MAGIC telescopes, located at the Roque de los Muchachos Observatory (2200 a.s.l.) in the Canary Island of La Palma, are placed on the top of a mountain, from where a window of visibility of about
The EMU view of the Large Magellanic Cloud: troubles for sub-TeV WIMPs
We present a radio search for WIMP dark matter in the Large Magellanic Cloud (LMC). We make use of a recent deep image of the LMC obtained from observations of the Australian Square Kilometre Array
...
...