Torsion and problems of standard cosmology / Hassan Abdalla Hassan Hamad ; Supervised Mamdouh Ishaac Wanas
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- الألتواء و مشكلات علم الكون القياسى [Added title page title]
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قاعة الرسائل الجامعية - الدور الاول | المكتبة المركزبة الجديدة - جامعة القاهرة | Cai01.12.01.M.Sc.2014.Ha.T (Browse shelf(Opens below)) | Not for loan | 01010110063889000 | ||
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مخـــزن الرســائل الجـــامعية - البدروم | المكتبة المركزبة الجديدة - جامعة القاهرة | Cai01.12.01.M.Sc.2014.Ha.T (Browse shelf(Opens below)) | 63889.CD | Not for loan | 01020110063889000 |
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Cai01.12.01.M.Sc.2014.Am.S Studying the effect of gravitational interaction between galaxies on the symmetry of their morphology and structure / | Cai01.12.01.M.Sc.2014.Em.P Photometric Study of some cD Galaxies / | Cai01.12.01.M.Sc.2014.Em.P Photometric Study of some cD Galaxies / | Cai01.12.01.M.Sc.2014.Ha.T Torsion and problems of standard cosmology / | Cai01.12.01.M.Sc.2014.Ha.T Torsion and problems of standard cosmology / | Cai01.12.01.M.Sc.2014.Ra.A Analysis and interpretation of magnetospheric oscillations / | Cai01.12.01.M.Sc.2014.Ra.A Analysis and interpretation of magnetospheric oscillations / |
Thesis (M.Sc.) - Cairo University - Faculty of Science - Department of Astronomy and Meteorology
The absolute parallelism geometry is used, instead of riemannian geometry, to investigate the effect of torsion on the dynamics of the friedmann {u2013} roberttson {u2013} walker model. We show that the torsion field can solve horizons problem and can be considered as the source of the present cosmic acceleration. Moreover, depending on the possible evolution of the torsion field with time, different world models for accelerating universe, including the dark energy model, can be deduced from our approach
Issued also as CD
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