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Searching for the existence of unusual nuclear shapes inside neutron starsLi, Chiu-fai., 李朝暉. January 2003 (has links)
published_or_final_version / abstract / toc / Physics / Master / Master of Philosophy
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Anisotropic heat transfer inside rotating neutron starsHui, Chung-yue., 許宗宇. January 2004 (has links)
published_or_final_version / abstract / toc / Physics / Master / Master of Philosophy
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Superfluid inside neutron stars and their signature of existence /Chau, Hoi-fung. January 1900 (has links)
Photocopy of typescript.
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Neutrino driven neutron star formationCernohorsky, Jan. January 1990 (has links)
Thesis (doctoral)--Universiteit van Amsterdam, 1990. / Summary in Dutch. Includes bibliographical references.
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Observations of glitches in PSR 0833-45 and 1641-45Flanagan, Claire Susan January 1996 (has links)
An eleven-year series of radio timing observations of 0833- 45 (Vela) and PSR 1641- 45 is presented. During this time, five large spin-ups ("glitches") were observed in 0833- 45 and one in 1641-45. The stellar response to these events is investigated, and the three relat ively long complete inter-glitch intervals in 0833-45 are modeled. The results are of relevance to studies of the interiors of neutron stars. The initial aim of the project - to obtain good observational coverage of large glitches in the Vela pulsar - was successfully achieved, and high quality observations of the periods between glitches were obtained as a by-product. The results of the analysis presented here provide support for the existence of both linear and non-linear coupling in the Vela pulsar, and put a limit on the former in PSR 1641- 45. The recently observed existence of a rapidly recovering component of part of a glitch in Vela was verified in the subsequent glitch, although there is now evidence to contradict the suggestion that this component involves a particular region of the star that is implicated in every glitch. Observations of a recent glitch in the same pulsar have resolved a small component of the spin-up; such a component has not been reported for any other large glitch.
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A review of pulsar glitch mechanismsMcDonald, Gregory Brett 18 August 2008 (has links)
In this thesis, a review of the most prominent pulsar glitch mechanisms is presented. This includes a discussion of the internal structure of neutron stars and the way in which glitches may be used to describe that structure. Particular attention is paid to the two-component model. This thesis also includes numerous simulations of the two-component model, which are fitted to observational data in order to determine how suitable this mechanism is as a description of pulsar glitches. The results show that this mechanism is in fact still relevant, in spite of its age. / Dr. C.A. Engelbrecht Dr. F.A.M. Frescura
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The evolution of neutron star magnetic fields張承民, Zhang, Chengmin. January 2000 (has links)
published_or_final_version / Physics / Doctoral / Doctor of Philosophy
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Short gamma-ray bursts resulting from phase-induced collapse of neutron starsTian, Xiaolei., 田小磊. January 2008 (has links)
published_or_final_version / Physics / Master / Master of Philosophy
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Properties of neutron stars in the relativistic mean field theory姚昌銓, Yao, Cheong-chuen. January 1996 (has links)
published_or_final_version / abstract / Physics / Master / Master of Philosophy
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Observational constraints on Be/x-ray binary modelsNegueruela, Ignacio January 1997 (has links)
No description available.
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