prikaz prve stranice dokumenta Heavy hybrid stars from multi-quark interactions
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Heavy hybrid stars from multi-quark interactions
European Physical Journal A: Hadrons and Nuclei, 50 (2014); 111. https://doi.org/10.1140/epja/i2014-14111-1
Benić, Sanjin

Citirajte ovaj rad

Benić, S. (2014). Heavy hybrid stars from multi-quark interactions. European Physical Journal A: Hadrons and Nuclei, 50.. doi: 10.1140/epja/i2014-14111-1

Benić, Sanjin. "Heavy hybrid stars from multi-quark interactions." European Physical Journal A: Hadrons and Nuclei, vol. 50, 2014. https://doi.org/10.1140/epja/i2014-14111-1

Benić, Sanjin. "Heavy hybrid stars from multi-quark interactions." European Physical Journal A: Hadrons and Nuclei 50 (2014). https://doi.org/10.1140/epja/i2014-14111-1

Benić, S. (2014) 'Heavy hybrid stars from multi-quark interactions', European Physical Journal A: Hadrons and Nuclei, 50. doi: 10.1140/epja/i2014-14111-1

Benić S. Heavy hybrid stars from multi-quark interactions. European Physical Journal A: Hadrons and Nuclei [Internet]. 2014. [pristupljeno 16.04.2024.];50. doi: 10.1140/epja/i2014-14111-1

S. Benić, "Heavy hybrid stars from multi-quark interactions", European Physical Journal A: Hadrons and Nuclei, vol. 50, 2014. [Online]. Dostupno na: https://urn.nsk.hr/urn:nbn:hr:217:717602. [Citirano: 16.04.2024.]

Za citiranje koristite ovu mrežnu adresu: https://urn.nsk.hr/urn:nbn:hr:217:717602
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Podaci o radu
Naslov (engleski)Heavy hybrid stars from multi-quark interactions
AutorSanjin Benić
Autorova ustanovaSveučilište u Zagrebu
Prirodoslovno-matematički fakultet
(Fizički odsjek)
Znanstveno / umjetničko
područje, polje i grana		PRIRODNE ZNANOSTI
Fizika
Sažetak (engleski)
We explore the possibility of obtaining heavy hybrid stars within the framework of the two flavor Nambu--Jona-Lasinio model with 8-quark interactions in the scalar and in the vector channel. The main impact of the 8-quark scalar channel is to reduce the onset of quark matter, while the 8-quark vector channel acts to stiff the equation of state at high densities. Within the parameter space where the 4-quark vector channel is small, and the 8-quark vector channel sizeable, stable stars with 2M_sun and above are found to hold quark matter in their cores.
Ključne riječi (engleski)
Jezikengleski
Vrsta publikacijeZnanstveni rad - Izvorni znanstveni rad
Status objaveObjavljen
Vrsta recenzijeRecenziran - međunarodna recenzija
Verzija publikacijeObjavljena verzija rada (izdavačev PDF)
Naslov časopisaEuropean Physical Journal A: Hadrons and Nuclei
Brojčani podacivol. 50, 111
p-ISSN1434-6001
e-ISSN1434-601X
DOIhttps://doi.org/10.1140/epja/i2014-14111-1
URN:NBNurn:nbn:hr:217:717602
Datum objave publikacije2014
ProjektŠifra: 119-0982930-1016
Naziv (hrvatski): Elementarne čestice, teorija polja i kozmologija
Voditelj: Ivica Picek
Pravna nadležnost: Hrvatska
Financijer: MZOS
Linija financiranja: ZP
URL dokumentahttps://link.springer.com/article/10.1140%2Fepja%2Fi2014-14111-1
Vrsta resursaTekst
Prava pristupaOtvoreni pristup
Uvjeti korištenjaIkona licence Imenovanje 4.0 međunarodna (CC BY 4.0)
Javna napomena© The Author(s) 2014. This is an open access article distributed under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. Received: 22 June 2014; Published online: 14 July 2014.
Datum i vrijeme pohrane2019-11-27 21:18:01