000			02167cam a2200337 a 4500
003			EG-GiCUC
005			20250223032516.0
008			200119s2019 ua d f m 000 0 eng d
040			_aEG-GiCUC _beng _cEG-GiCUC
041	0		_aeng
049			_aDeposite
097			_aM.Sc
099			_aCai01.12.20.M.Sc.2019.Ah.T
100	0		_aAhmed Imsaeri Omar Imsaeri
245	1	0	_aTheoretical studies of mechanical properties for infinite nuclear matter / _cAhmed Imsaeri Omar Imsaeri ; Supervised Sayed Saleh Abdelaziz Saleh , Magdi Mohamed Hamed Elgogary , Mohammed Hasan Mohammed Soleiman
246	1	5	_aدراسات نظرية للخواص الميكانيكية للمادة النووية اللامنتهية
260			_aCairo : _bAhmed Imsaeri Omar Imsaeri , _c2019
300			_a82 P. : _bcharts , facsimile ; _c25cm
502			_aThesis (M.Sc.) - Cairo University - Faculty of Science - Department of Physics
520			_aMechanical properties of infinite nuclear matter are important in determining the type of the equation of state of the nuclear matter. Stress {u2013} strain of the infinite nuclear matter making up a pulsar included in binary compact neutron star system is studied for sources PSR B 1913+16 (Discovered in 1974). Bulk modulus (or the compressibility) of the infinite nuclear matter is investigated through two theoretical treatments.That is, deriving the compressibility from the polytropic equation of state and by modeling the tidal deformation of a pulsar included in a binary system. The compressibility is found as a function of total energy density in first approach, and the magnitude of the deformation is estimated in the second approach, as the eccentricity is found to be of 10⁻⁵ order and the elongation is of the order 10⁻⁹ km
530			_aIssued also as CD
653		4	_aBulk Modulus
653		4	_aInfinite Nuclear Matter
653		4	_aNeutron Star
700	0		_aMagdi Mohamed Hamed Elgogary , _eSupervisor
700	0		_aSayed Saleh Abdelaziz Saleh , _eSupervisor
856			_uhttp://172.23.153.220/th.pdf
905			_aNazla _eRevisor
905			_aShimaa _eCataloger
942			_2ddc _cTH
999			_c76384 _d76384