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undergraduate thesis
Bijeli patuljak
2021. urn:nbn:hr:166:970890
Mihovilović, Marko
University of Split
Faculty of Science
Department of Physics

Cite this document

Mihovilović, M. (2021). Bijeli patuljak (Undergraduate thesis). Split: University of Split, Faculty of Science. Retrieved from https://urn.nsk.hr/urn:nbn:hr:166:970890

Mihovilović, Marko. "Bijeli patuljak." Undergraduate thesis, University of Split, Faculty of Science, 2021. https://urn.nsk.hr/urn:nbn:hr:166:970890

Mihovilović, Marko. "Bijeli patuljak." Undergraduate thesis, University of Split, Faculty of Science, 2021. https://urn.nsk.hr/urn:nbn:hr:166:970890

Mihovilović, M. (2021). 'Bijeli patuljak', Undergraduate thesis, University of Split, Faculty of Science, accessed 24 April 2024, https://urn.nsk.hr/urn:nbn:hr:166:970890

Mihovilović M. Bijeli patuljak [Undergraduate thesis]. Split: University of Split, Faculty of Science; 2021 [cited 2024 April 24] Available at: https://urn.nsk.hr/urn:nbn:hr:166:970890

M. Mihovilović, "Bijeli patuljak", Undergraduate thesis, University of Split, Faculty of Science, Split, 2021. Available at: https://urn.nsk.hr/urn:nbn:hr:166:970890

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Metadata
TitleBijeli patuljak
Title (english)White dwarf
AuthorMarko Mihovilović
MentorMarko Kovač (mentor)
Committee memberMarko Kovač (predsjednik povjerenstva)
Committee memberKoraljka Mužić (član povjerenstva)
Committee memberToni Šćulac (član povjerenstva)
GranterUniversity of Split
Faculty of Science
(Department of Physics)
Split
Defense date and country2021-09-28, Croatia
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract
Bijeli patuljak jest završna faza evolucije zvijezde srednje veličine. Na početku je riječ o vrućem objektu, koji se potom postepeno hladi zbog prestanka fuzije. Bijeli patuljak sadržava degeneriranu materiju te tlak degeneriranog plina ima glavnu ulogu u sprječavanju gravitacijskog sažimanja. Kroz raspisivanje niza jednadžbi, došlo se do dvije temeljne diferencijalne jednadžbe uz pomoć kojih je opisana struktura bijelih patuljaka te je ujedno i grafički prikazana.
Abstract (english)
White dwarf is the final phase of the medium sized star evolution. At the beginning, it is a very hot object that gradually losses it’s temperature because of the stoppage of fusion. White dwarf contains degenerate matter and degenerate pressure plays the major role in stopping gravitational collapse. Through a series of equations, we managed to define two main differential equations which helped us in describing the structure of the white dwarfs, and the results are graphically shown.
Keywords
Keywords (english)
Languagecroatian
URN:NBNurn:nbn:hr:166:970890
Study programmeTitle: Physics
Study programme type: university
Study level: undergraduate
Academic / professional title: sveučilišni/a prvostupnik/prvostupnica (baccalaureus/baccalaurea) fizike (sveučilišni/a prvostupnik/prvostupnica (baccalaureus/baccalaurea) fizike)
Type of resourceText
File originBorn digital
Access conditionsOpen access
Terms of useLicence Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0) icon
Created on2021-10-26 10:21:50