Zobrazeno 1 - 10
of 319
pro vyhledávání: '"Šoda, J"'
Autor:
Rogić Vidaković M, Šoda J, Jerković A, Benzon B, Bakrač K, Dužević S, Vujović I, Mihalj M, Pecotić R, Valić M, Mastelić A, Hagelien MV, Zmajević Schőnwald M, Đogaš Z
Publikováno v:
Nature and Science of Sleep, Vol Volume 12, Pp 563-574 (2020)
Maja Rogić Vidaković,1 Joško Šoda,2 Ana Jerković,1 Benjamin Benzon,1 Karla Bakrač,1 Silvia Dužević,1 Igor Vujović,2 Mario Mihalj,3 Renata Pecotić,1,4 Maja Valić,1,4 Angela Mastelić,5 Maximilian Vincent Hagelien,1 Marina Zmajević Schőnwa
Externí odkaz:
https://doaj.org/article/0b7446370bf14a43aed1c53e9d0266ad
The isotropy and homogeneity of the cosmic microwave background (CMB) favors "scalar driven" early Universe inflationary models. Non-scalar fields, and in particular gauge fields, are on the other hand commonplace in all high energy particle physics
Externí odkaz:
http://arxiv.org/abs/1212.2921
Publikováno v:
Materialwissenschaft und Werkstoffechnik; May2024, Vol. 55 Issue 5, p650-655, 6p
Publikováno v:
Mod.Phys.Lett. A16 (2001) 1089-1100
Recently, the self-tuning mechanism of cancellation of vacuum energy has been proposed in which our universe is a flat 3-brane in a 5-dimensional spacetime. In this letter, the self-tuning mechanism of dark energy is proposed by considering the cosmo
Externí odkaz:
http://arxiv.org/abs/hep-th/0008197
Autor:
Taruya, A., Soda, J.
Publikováno v:
Mon.Not.Roy.Astron.Soc. 317 (2000) 873
We discuss the influence of the cosmological background density field on the spherical infall model. The spherical infall model has been used in the Press-Schechter formalism to evaluate the number abundance of clusters of galaxies, as well as to det
Externí odkaz:
http://arxiv.org/abs/astro-ph/9911116
Autor:
Taruya, A., Soda, J.
Publikováno v:
Astrophys.J. 522 (1999) 46-58
It is believed that the biasing of the galaxies plays an important role for understanding the large-scale structure of the universe. In general, the biasing of galaxy formation could be stochastic. Furthermore, the future galaxy survey might allow us
Externí odkaz:
http://arxiv.org/abs/astro-ph/9809204
Publikováno v:
Astrophys.J. 510 (1999) 541
It is generally believed that the spatial distribution of galaxies does not trace that of the total mass. The understanding of the bias effect is therefore necessary to determine the cosmological parameters and the primordial density fluctuation spec
Externí odkaz:
http://arxiv.org/abs/astro-ph/9807005
Autor:
Kustura, L, Bobek, D, Poljičanin, A, Pavelin, S, Šoda, M Buljubašić, Šoda, J, Aksentijević, J, Glavor, K Duka, Knez, N Narančić, Viali, V, Cukrov, A, Laidlaw, I Todorić, Ipavec, N, Vukorepa, D, Stipica, I, Bakrač, K, Bošković, B, Mastelić, A, Mužinić, N Režić, Markotić, A
Publikováno v:
QJM: An International Journal of Medicine; Jan2024, Vol. 117 Issue 1, p38-47, 10p
Publikováno v:
Phys.Rev.D55:3337-3345,1997
We study how the initial inhomogeneities of the spatial curvature affect the onset of inflation in the closed universe. We consider a cosmological model which contains a radiation and a cosmological constant. In order to treat the inhomogeneities in
Externí odkaz:
http://arxiv.org/abs/gr-qc/9606012
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