Repository of University of Nova Gorica

Search the repository
A+ | A- | Help | SLO | ENG

Query: search in
search in
search in
search in
* old and bolonia study programme

Options:
  Reset


1 - 4 / 4
First pagePrevious page1Next pageLast page
1.
HESS J1731-347
Serguei Vorobiov, F. Acero, 2010, published scientific conference contribution abstract

Found in: osebi
Keywords: ground based y-ray telescopes, H.E.S.S. system, Cherenkov telescopes, shell-type supernova remnants
Published: 25.04.2014; Views: 3289; Downloads: 16
URL Fulltext (0,00 KB)

2.
3.
Fermi Large Area Telescope fourth source catalog
S. Abdollahi, F. Acero, M. Ajello, W. B. Atwood, M. Axelsson, L. Baldini, J. Ballet, G. Barbiellini, D. Bastieri, Gabrijela Zaharijas, 2020, original scientific article

Found in: osebi
Keywords: astronomy, gamma rays, sky surveys
Published: 22.05.2020; Views: 996; Downloads: 42
.pdf Fulltext (2,55 MB)
This document has many files! More...

4.
Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation
Serguei Vorobiov, Samo Stanič, Christopher Eckner, R. Adam, A. Acharyya, F. Acero, H. Abe, H. Abdalla, Gabrijela Zaharijas, Marko Zavrtanik, Danilo Zavrtanik, Miha Živec, 2021, original scientific article

Abstract: The Cherenkov Telescope Array (CTA), the new-generation ground-based observatory for γ astronomy, provides unique capabilities to address significant open questions in astrophysics, cosmology, and fundamental physics. We study some of the salient areas of γ cosmology that can be explored as part of the Key Science Projects of CTA, through simulated observations of active galactic nuclei (AGN) and of their relativistic jets. Observations of AGN with CTA will enable a measurement of γ absorption on the extragalactic background light with a statistical uncertainty below 15% up to a redshift z=2 and to constrain or detect γ halos up to intergalactic-magnetic-field strengths of at least 0.3 pG . Extragalactic observations with CTA also show promising potential to probe physics beyond the Standard Model. The best limits on Lorentz invariance violation from γ astronomy will be improved by a factor of at least two to three. CTA will also probe the parameter space in which axion-like particles could constitute a significant fraction, if not all, of dark matter. We conclude on the synergies between CTA and other upcoming facilities that will foster the growth of γ cosmology.
Found in: osebi
Keywords: Cherenkov Telescope Array, active galactic nuclei, gamma-ray experiments, axions, extragalactic magnetic fields
Published: 02.03.2021; Views: 500; Downloads: 21
URL Fulltext (0,00 KB)
This document has many files! More...

Search done in 0 sec.
Back to top