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master's thesis
Kvazinormalni modovi crnih rupa
Zagreb: University of Zagreb, Faculty of Science, 2022. urn:nbn:hr:217:019333
Dulibić, Lovro
University of Zagreb
Faculty of Science
Department of Physics

Institutional repository: Repository of the Faculty of Science

Cite this document

Dulibić, L. (2022). Kvazinormalni modovi crnih rupa (Master's thesis). Zagreb: University of Zagreb, Faculty of Science. Retrieved from https://urn.nsk.hr/urn:nbn:hr:217:019333

Dulibić, Lovro. "Kvazinormalni modovi crnih rupa." Master's thesis, University of Zagreb, Faculty of Science, 2022. https://urn.nsk.hr/urn:nbn:hr:217:019333

Dulibić, Lovro. "Kvazinormalni modovi crnih rupa." Master's thesis, University of Zagreb, Faculty of Science, 2022. https://urn.nsk.hr/urn:nbn:hr:217:019333

Dulibić, L. (2022). 'Kvazinormalni modovi crnih rupa', Master's thesis, University of Zagreb, Faculty of Science, accessed 26 November 2024, https://urn.nsk.hr/urn:nbn:hr:217:019333

Dulibić L. Kvazinormalni modovi crnih rupa [Master's thesis]. Zagreb: University of Zagreb, Faculty of Science; 2022 [cited 2024 November 26] Available at: https://urn.nsk.hr/urn:nbn:hr:217:019333

L. Dulibić, "Kvazinormalni modovi crnih rupa", Master's thesis, University of Zagreb, Faculty of Science, Zagreb, 2022. Available at: https://urn.nsk.hr/urn:nbn:hr:217:019333

Metadata
TitleKvazinormalni modovi crnih rupa
Title (english)Quasinormal modes of black holes
AuthorLovro Dulibić
MentorIvica Smolić (mentor)
Committee memberIvica Smolić (predsjednik povjerenstva)
Committee memberMaro Cvitan (član povjerenstva)
Committee memberVernesa Smolčić (član povjerenstva)
Committee memberSanjin Benić (član povjerenstva)
Committee memberKrešimir Pavlovski (član povjerenstva)
GranterUniversity of Zagreb
Faculty of Science
(Department of Physics)
Zagreb
Defense date and country2022-09-23, Croatia
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Abstract
Prostorvremena crnih rupa stabilna su rješenja Einsteinove jednadžbe. Uslijed neke perturbacije one će se vratiti u prvobitno stanje prilikom čega će izgubiti dio energije zračenjem gravitacijskih valova. Svojstveni načini titranja disipativnih sustava, stoga i crnih rupa, nazivaju se kvazinormalni modovi. U ovome radu dan je teorijski pregled kvazinormalnih modova kroz teoriju perturbacija crnih rupa. U prvom ne iščezavajućem redu promotrena je dinamika perturbacije prostorvremena te dinamika skalarnih i vektorskih polja uronjenih u pozadinsko prostorvrijeme Schwarzschildove crne rupe. Proučeno je nekoliko poznatih, aproksimativnih i egzaktnih, metoda računanja kvazinormalnih modova te su njihovi rezultati također i reproducirani.
Abstract (english)
Black hole spacetimes are stable solutions to Einstein’s equations. After a perturbation they will return to their equilibrium state during which they will lose energy through gravitational radiation. Eigenmodes of dissipative systems, including black holes, are called quasinormal modes. In this thesis, a theoretical overview of quasinormal modes is given through black hole perturbation theory. The dynamics of spacetime perturbations, as well as scalar and vector field dynamics in Schwarzschild spacetime is analysed in leading order of perturbation theory. A couple of well-known, approximative and exact, methods of calculating quasinormal modes is given and their results are reproduced.
Keywords
Keywords (english)
Languagecroatian
URN:NBNurn:nbn:hr:217:019333
Study programmeTitle: Physics; specializations in: Research
Course: Research
Study programme type: university
Study level: integrated undergraduate and graduate
Academic / professional title: magistar/magistra fizike (magistar/magistra fizike)
Type of resourceText
File originBorn digital
Access conditionsOpen access
Terms of useLicence In copyright icon
Created on2022-10-19 08:56:45