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undergraduate thesis
Razvoj ranog svemira
2016. urn:nbn:hr:160:890084
Pecimotika, Mario
Josip Juraj Strossmayer University of Osijek
Department of Physics
Division of Experimental Physics
Division Chair of Condensed Matter Physics

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Pecimotika, M. (2016). Razvoj ranog svemira (Undergraduate thesis). Osijek: Josip Juraj Strossmayer University of Osijek, Department of Physics. Retrieved from https://urn.nsk.hr/urn:nbn:hr:160:890084

Pecimotika, Mario. "Razvoj ranog svemira." Undergraduate thesis, Josip Juraj Strossmayer University of Osijek, Department of Physics, 2016. https://urn.nsk.hr/urn:nbn:hr:160:890084

Pecimotika, Mario. "Razvoj ranog svemira." Undergraduate thesis, Josip Juraj Strossmayer University of Osijek, Department of Physics, 2016. https://urn.nsk.hr/urn:nbn:hr:160:890084

Pecimotika, M. (2016). 'Razvoj ranog svemira', Undergraduate thesis, Josip Juraj Strossmayer University of Osijek, Department of Physics, accessed 19 April 2024, https://urn.nsk.hr/urn:nbn:hr:160:890084

Pecimotika M. Razvoj ranog svemira [Undergraduate thesis]. Osijek: Josip Juraj Strossmayer University of Osijek, Department of Physics; 2016 [cited 2024 April 19] Available at: https://urn.nsk.hr/urn:nbn:hr:160:890084

M. Pecimotika, "Razvoj ranog svemira", Undergraduate thesis, Josip Juraj Strossmayer University of Osijek, Department of Physics, Osijek, 2016. Available at: https://urn.nsk.hr/urn:nbn:hr:160:890084

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Metadata
TitleRazvoj ranog svemira
Title (english)The evolution of the early universe
AuthorMario Pecimotika
MentorBranko Vuković (mentor)
MentorMaja Varga Pajtler (komentor)
GranterJosip Juraj Strossmayer University of Osijek
Department of Physics
(Division of Experimental Physics)
(Division Chair of Condensed Matter Physics)
Osijek
Defense date and country2016-09-15, Croatia
Scientific / art field,
discipline and subdiscipline		NATURAL SCIENCES
Physics
Astronomy and Astrophysics
Abstract
Fizika ranog svemira nalazi se na granici astronomije i filozofije s obzirom da ne postoji potpuna teorija koja ujedinjuje sve fundamentalne sile prirode u trenutku stvaranja. Osim toga, ne postoji mogućnost povezivanja promatrane fizike ranog svemira s trenutnim fizikalnim teorijama (tj. nije moguće izgraditi drugi svemir). Većinu događaja u evoluciji svemira nakon vremena Planckove epohe (oko 10^−43 sekundi nakon Velikog praska) današnja fizika može objasniti. Medutim, događaji prije tog trenutno su nedefinirani, a posebice ne razumijemo uzrok Velikog praska. U najboljem slučaju, možemo naše napore usredočtiti na ispitivanje i definiranje onoga što ne razumijemo u potpunosti.
Abstract (english)
Physics of the early Universe is at the boundary of astronomy and philosophy since there is no a complete theory that unifies all the fundamental forces at the begining. Furthermore, there is no way of joining observation of early Universe physics to current theories in physics (i.e. it’s not possible to build another Universe) Our physics can explain most of the evolution of the Universe after the Planck time (approximately 10^−43 seconds after the Big Bang). Though, events before this time are still undefined and, in particular, we do not understand the origin of the Big Ban. At best, we can focus our efforts on examining and defining what we do not fully understand.
Keywords
Keywords (english)
Languagecroatian
URN:NBNurn:nbn:hr:160:890084
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 In copyright icon
Created on2016-09-22 06:26:07