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Acceleration mechanisms for ultra high energy cosmic rays / Ahmed Mohamed Saleh Hassanin ; Supervised Ahmed Abdelhady , Mohamed Tawfik Ghonein , Abdelnasser Mahmoud Tawfik

By: Contributor(s): Material type: TextTextLanguage: English Publication details: Cairo : Ahmed Mohamed Saleh Hassanin , 2012Description: 95P. : plans ; 25cmOther title:
  • آليات تعجيل الأشعة الكونية فائقة الطاقة [Added title page title]
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  • Issued also as CD
Dissertation note: Thesis (M.Sc.) - Cairo University - Faculty of Science - Department of Astronomy and Meteorology Summary: The discovery and detection of ultra high energy cosmic rays ( UHECRs ) of energy up to 10²{u⁰⁰B⁰} eV posed a serious challenge to the astropysicists about their origin as well as the physical acceleration mechanisms . Some theoretical approaches in the past assuming elastic scatterings of cosmic charged particles with magnetic clouds then developed by assuming the presence of shock waves originated from supernova remnant succeeded to explain the existence of energies up to 10¹⁵ eV
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Item type Current library Home library Call number Copy number Status Barcode
Thesis Thesis قاعة الرسائل الجامعية - الدور الاول المكتبة المركزبة الجديدة - جامعة القاهرة Cai01.12.01.M.Sc.2012.Ah.A (Browse shelf(Opens below)) Not for loan 01010110058238000
CD - Rom CD - Rom مخـــزن الرســائل الجـــامعية - البدروم المكتبة المركزبة الجديدة - جامعة القاهرة Cai01.12.01.M.Sc.2012.Ah.A (Browse shelf(Opens below)) 58238.CD Not for loan 01020110058238000

Thesis (M.Sc.) - Cairo University - Faculty of Science - Department of Astronomy and Meteorology

The discovery and detection of ultra high energy cosmic rays ( UHECRs ) of energy up to 10²{u⁰⁰B⁰} eV posed a serious challenge to the astropysicists about their origin as well as the physical acceleration mechanisms . Some theoretical approaches in the past assuming elastic scatterings of cosmic charged particles with magnetic clouds then developed by assuming the presence of shock waves originated from supernova remnant succeeded to explain the existence of energies up to 10¹⁵ eV

Issued also as CD

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