Very High Energy Cosmic Gamma Radiation: A Crucial Window on the Extreme Universe

By F. Aharonian. 2004

342 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics, Pulmonary and Respiratory Medicine

View Paper: https://www.semanticscholar.org/paper/f21103bbf8c67ec682dcae619dfa547318f71990

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. Andrii Y. Neronov
2. R. Durrer
3. S. Profumo
4. Sergio Colafrancesco
5. E. Carlson
6. Y. Fukui
7. P. Giommi
8. Sandro Mereghetti

In Nuclear and High Energy Physics

1. Andrii Y. Neronov
2. R. Durrer
3. S. Profumo
4. Sergio Colafrancesco
5. E. Carlson
6. Y. Fukui
7. P. Giommi
8. Sandro Mereghetti

In Pulmonary and Respiratory Medicine

1. Andrii Y. Neronov
2. S. Profumo
3. E. Carlson
4. R. Durrer

Citations in the corpus

• Cosmological Magnetic Fields: Their Generation, Evolution and Observation (2013, methodology): “Here nEBL(ǫ) is the number density of EBL photons, nEBL ≃ ρEBL/ǫ, σγγ(ǫ) is the pair production cross-section which reaches it maximum σγγ ≃ 10 cm(2) at aout 4 times the threshold energy (Aharonian 2004) and we have to insert the value of ρEBL at this maximum, ǫmax ≃ 4m(2)e/Eγ . The mean free path o”
• NEUTRAL PION EMISSION FROM ACCELERATED PROTONS IN THE SUPERNOVA REMNANT W44 (2011, background): “Moreover, Abdo et al. (2010a) excluded the presence of a pulsation in the γ -ray signal.”
• Cosmic ray protons in the inner Galaxy and the Galactic Center gamma-ray excess (2014, methodology): “[28], which describes the temporal evolution of the spectrum of a cosmic-rays which are accelerated inside a molecular cloud, where large gas densities and magnetic fields can trap low-energy protons on timescales of 10(5) yr.”