Fábio Köpp, Jorge Ernesto Horvath, Dimiter Hadjimichef, César A. Zen Vasconcellos
{"title":"Investigating Phase Transitions in Hybrid Stars Using the vMIT Bag Model and the QHD-II Model","authors":"Fábio Köpp, Jorge Ernesto Horvath, Dimiter Hadjimichef, César A. Zen Vasconcellos","doi":"10.1002/asna.20250006","DOIUrl":null,"url":null,"abstract":"<div>\n \n <p>In this contribution, the global properties of hybrid compact stars resulting from a phase transition between hadronic matter and an interior composed of up, down, and strange quarks, based on a Maxwell construction, are studied. For the equation of state of the hadronic matter, we employ a covariant density functional theory within the framework of relativistic mean field theory, specifically the Quantum Hadrodynamics-II (QHD-II) model, with parameters determined using the <span></span><math>\n <semantics>\n <mrow>\n <mi>NL</mi>\n <msup>\n <mn>3</mn>\n <mo>*</mo>\n </msup>\n <mrow>\n <mi>ω</mi>\n <mi>ρ</mi>\n </mrow>\n </mrow>\n <annotation>$$ NL{3}^{\\ast}\\omega \\rho $$</annotation>\n </semantics></math> parametrization. For the quark matter in the stellar core, we use the improved vMIT bag model, which incorporates repulsive interactions mediated by vector mesons, a crucial feature for describing stable and massive hybrid stellar configurations in agreement with recent observations of pulsars with masses above <span></span><math>\n <semantics>\n <mrow>\n <mn>2.0</mn>\n <mspace></mspace>\n <msub>\n <mi>M</mi>\n <mo>⊙</mo>\n </msub>\n </mrow>\n <annotation>$$ 2.0\\kern0.1em {\\mathrm{M}}_{\\odot } $$</annotation>\n </semantics></math>.</p>\n </div>","PeriodicalId":55442,"journal":{"name":"Astronomische Nachrichten","volume":"346 3-4","pages":""},"PeriodicalIF":1.0000,"publicationDate":"2025-01-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Astronomische Nachrichten","FirstCategoryId":"101","ListUrlMain":"https://onlinelibrary.wiley.com/doi/10.1002/asna.20250006","RegionNum":4,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"ASTRONOMY & ASTROPHYSICS","Score":null,"Total":0}
引用次数: 0
Abstract
In this contribution, the global properties of hybrid compact stars resulting from a phase transition between hadronic matter and an interior composed of up, down, and strange quarks, based on a Maxwell construction, are studied. For the equation of state of the hadronic matter, we employ a covariant density functional theory within the framework of relativistic mean field theory, specifically the Quantum Hadrodynamics-II (QHD-II) model, with parameters determined using the parametrization. For the quark matter in the stellar core, we use the improved vMIT bag model, which incorporates repulsive interactions mediated by vector mesons, a crucial feature for describing stable and massive hybrid stellar configurations in agreement with recent observations of pulsars with masses above .
期刊介绍:
Astronomische Nachrichten, founded in 1821 by H. C. Schumacher, is the oldest astronomical journal worldwide still being published. Famous astronomical discoveries and important papers on astronomy and astrophysics published in more than 300 volumes of the journal give an outstanding representation of the progress of astronomical research over the last 180 years. Today, Astronomical Notes/ Astronomische Nachrichten publishes articles in the field of observational and theoretical astrophysics and related topics in solar-system and solar physics. Additional, papers on astronomical instrumentation ground-based and space-based as well as papers about numerical astrophysical techniques and supercomputer modelling are covered. Papers can be completed by short video sequences in the electronic version. Astronomical Notes/ Astronomische Nachrichten also publishes special issues of meeting proceedings.