The Effect of Non-Thermal Protons on the High Energy Spectra of Black Hole Binaries(Poster)

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概要

• 論文の詳細を見る

• We investigate here the effect on the emitted spectrum of a black hole binary due to the presence of accelerated protons in the inner region of the accretion disk. Our study shows that e^-e^+ pairs and high energy γ-rays created in inelastic p-p collisions contribute mainly in the 1-10 MeV range and produce a broad feature in the spectrum in this energy range which can be verified by INTEGRAL and GLAST observations.

• 理論物理学刊行会の論文
• 2004-11-15

著者

• BHATTACHARYYA S.

  S.D.B.College

• BHATTACHARYYA S.

  Bhabha Atomic Research Centre, Nuclear Research Laboratory

• BHATT N.

  Bhabha Atomic Research Centre, Nuclear Research Laboratory

• MISRA R.

  Inter-University Center for Astronomy and Astrophysics

• KAUL C.

  Bhabha Atomic Research Centre, Nuclear Research Laboratory

• Kaul C.

  Bhabha Atomic Research Centre Nuclear Research Laboratory

• Bhatt N.

  Bhabha Atomic Research Centre Nuclear Research Laboratory

関連論文

• Extended Thomas-Fermi Approach to π^0 Condensation in Neutron Matter
• The Effect of Non-Thermal Protons on the High Energy Spectra of Black Hole Binaries(Poster)
• The Effect of Non-Thermal Protons on the High Energy Spectra of Black Hole Binaries(Poster)

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