prikaz prve stranice dokumenta Jednostavni model neutronskih zvijezda
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undergraduate thesis
Jednostavni model neutronskih zvijezda
2020. urn:nbn:hr:166:524695
Sabljo, Ana-Marija
University of Split
Faculty of Science
Department of Physics

Cite this document

Sabljo, A. M. (2020). Jednostavni model neutronskih zvijezda (Undergraduate thesis). Split: University of Split, Faculty of Science. Retrieved from https://urn.nsk.hr/urn:nbn:hr:166:524695

Sabljo, Ana Marija. "Jednostavni model neutronskih zvijezda." Undergraduate thesis, University of Split, Faculty of Science, 2020. https://urn.nsk.hr/urn:nbn:hr:166:524695

Sabljo, Ana Marija. "Jednostavni model neutronskih zvijezda." Undergraduate thesis, University of Split, Faculty of Science, 2020. https://urn.nsk.hr/urn:nbn:hr:166:524695

Sabljo, A. M. (2020). 'Jednostavni model neutronskih zvijezda', Undergraduate thesis, University of Split, Faculty of Science, accessed 15 November 2024, https://urn.nsk.hr/urn:nbn:hr:166:524695

Sabljo AM. Jednostavni model neutronskih zvijezda [Undergraduate thesis]. Split: University of Split, Faculty of Science; 2020 [cited 2024 November 15] Available at: https://urn.nsk.hr/urn:nbn:hr:166:524695

A. M. Sabljo, "Jednostavni model neutronskih zvijezda", Undergraduate thesis, University of Split, Faculty of Science, Split, 2020. Available at: https://urn.nsk.hr/urn:nbn:hr:166:524695

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Metadata
TitleJednostavni model neutronskih zvijezda
Title (english)Simple model of neutron stars
AuthorAna-Marija Sabljo
MentorMile Dželalija (mentor)
Committee memberMile Dželalija (predsjednik povjerenstva)
Committee memberŽeljana Bonačić Lošić (član povjerenstva)
Committee memberIvana Weber (član povjerenstva)
GranterUniversity of Split
Faculty of Science
(Department of Physics)
Split
Defense date and country2020-09-25, Croatia
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Nuclear Physics
Abstract
Cilj ovog rada je pobliže objasniti kako su nastale neutronske zvijezde, od čega se sastoje te opisati glavna svojstva o kojima ovise. Opisat ću glavne slojeve na jednostavnom modelu neutronske zvijezde, na koji način je došlo do rotacije zvijezde te jak utjecaj gravitacije i magnetskog polja. Gustoća takvih zvijezda izuzetno je visoka i nekoliko puta veća od prosječne gustoće atomskih jezgra. Na kraju su opisane i vrste neutronskih zvijezda koje su izvor elektromagnetskog zračenja koje na Zemlju dolazi u obliku periodičnih impulsa.
Abstract (english)
The aim of this paper is to explain in more detail how neutron stars are formed, what they consist of and to describe the main properties on which it depends. I will describe the main layers on a simple neutron star model, the way the star rotated, and the strong influence of gravity and magnetic field. The density of such stars is extremely high and several times higher than the average density of atomic nuclei. Finally, the types of neutron stars that are a source of electromagnetic radiation that come to Earth in the form of periodic pulses are described.
Keywords
Keywords (english)
Languagecroatian
URN:NBNurn:nbn:hr:166:524695
Study programmeTitle: Physics and Computer Science
Study programme type: university
Study level: undergraduate
Academic / professional title: sveučilišni/a prvostupnik/prvostupnica (baccalaureus/baccalaurea) fizike i informatike (sveučilišni/a prvostupnik/prvostupnica (baccalaureus/baccalaurea) fizike i informatike)
Type of resourceText
File originBorn digital
Access conditionsAccess restricted to students and staff of home institution
Terms of useLicence In copyright icon
Created on2021-01-15 14:43:24