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The evolution of binary neutron star orbits due to the emission of gravitational waves / (Record no. 64029)

MARC details
000 -LEADER
fixed length control field 02281cam a2200325 a 4500
003 - CONTROL NUMBER IDENTIFIER
control field EG-GiCUC
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION
fixed length control field 171216s2017 ua do f m 000 0 eng d
040 ## - CATALOGING SOURCE
Original cataloging agency EG-GiCUC
Language of cataloging eng
Transcribing agency EG-GiCUC
041 0# - LANGUAGE CODE
Language code of text/sound track or separate title eng
049 ## - LOCAL HOLDINGS (OCLC)
Holding library Deposite
097 ## - Thesis Degree
Thesis Level M.Sc
099 ## - LOCAL FREE-TEXT CALL NUMBER (OCLC)
Classification number Cai01.12.01.M.Sc.2017.Ze.E
100 0# - MAIN ENTRY--PERSONAL NAME
Personal name Zeinab Ahmed Mabrouk
245 14 - TITLE STATEMENT
Title The evolution of binary neutron star orbits due to the emission of gravitational waves /
Statement of responsibility, etc. Zeinab Ahmed Mabrouk ; Supervised Mustafa Kamal Mahmoud Ahmed , Shahinaz Mostafa Ali Yousef , Walied Ali Ahmed Hassan Rahoma
246 15 - VARYING FORM OF TITLE
Title proper/short title تطور مدارات النجوم النيوترونية المزدوجة نتيجة إنبعاث موجات التثاقل
260 ## - PUBLICATION, DISTRIBUTION, ETC.
Place of publication, distribution, etc. Cairo :
Name of publisher, distributor, etc. Zeinab Ahmed Mabrouk ,
Date of publication, distribution, etc. 2017
300 ## - PHYSICAL DESCRIPTION
Extent 74 P. :
Other physical details charts , photographs ;
Dimensions 25cm
502 ## - DISSERTATION NOTE
Dissertation note Thesis (M.Sc.) - Cairo University - Faculty of Science - Department of Astronomy and Meteorology
520 ## - SUMMARY, ETC.
Summary, etc. We have applied the method derived by (imshennik and popov) of determination the elliptical orbits evolution due to gravitational wave emission on two different systems. The first is the Pre-supernova SN1987A, it was the same system that Imshennik and popov used. With the aid of mathematica programme, we got the same curves and conclusions; however we added some curves in order to ensure the gotten results. The second system was PSR1913+16 system. Our results for this system are highly comparable with the latest analysis for that system based on published timing observations from 1974 through 2006 (weisberg, nice and taylor, 2010). The most important results from our study are: Both our studied elliptical orbits shrink in size and become near circular at their late stages of evolution while the circular orbits don{u2019}t change its shape; and most of the energy is lost at high eccentricities near the periastron position
530 ## - ADDITIONAL PHYSICAL FORM AVAILABLE NOTE
Additional physical form available note Issued also as CD
653 #4 - INDEX TERM--UNCONTROLLED
Uncontrolled term Evolution of neutron star orbits
653 #4 - INDEX TERM--UNCONTROLLED
Uncontrolled term Gravitational waves
653 #4 - INDEX TERM--UNCONTROLLED
Uncontrolled term PSR 1913+16
700 0# - ADDED ENTRY--PERSONAL NAME
Personal name Mustafa Kamal Mahmoud Ahmed ,
Relator term
700 0# - ADDED ENTRY--PERSONAL NAME
Personal name Shahinaz Mostafa Ali Yousef ,
Relator term
700 0# - ADDED ENTRY--PERSONAL NAME
Personal name Walied Ali Ahmed Hassan Rahoma ,
Relator term
905 ## - LOCAL DATA ELEMENT E, LDE (RLIN)
Cataloger Nazla
Reviser Revisor
905 ## - LOCAL DATA ELEMENT E, LDE (RLIN)
Cataloger Samia
Reviser Cataloger
942 ## - ADDED ENTRY ELEMENTS (KOHA)
Source of classification or shelving scheme Dewey Decimal Classification
Koha item type Thesis
Holdings
Source of classification or shelving scheme Not for loan Home library Current library Date acquired Full call number Barcode Date last seen Koha item type Copy number
Dewey Decimal Classification   المكتبة المركزبة الجديدة - جامعة القاهرة قاعة الرسائل الجامعية - الدور الاول 11.02.2024 Cai01.12.01.M.Sc.2017.Ze.E 01010110073716000 22.09.2023 Thesis  
Dewey Decimal Classification   المكتبة المركزبة الجديدة - جامعة القاهرة مخـــزن الرســائل الجـــامعية - البدروم 11.02.2024 Cai01.12.01.M.Sc.2017.Ze.E 01020110073716000 22.09.2023 CD - Rom 73716.CD