Bayesian Analysis for Extracting Properties of the Nuclear Equation of State from Observational Data Including Tidal Deformability from GW170817
We develop a Bayesian analysis method for selecting the most probable equation of state under a set of constraints from compact star physics, which now include the tidal deformability from GW170817. We apply this method for the first time to a two-parameter family of hybrid equations of state that i...
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doaj-d0024faccae44589bb7e2d11fad43fad2020-11-25T02:16:02ZengMDPI AGUniverse2218-19972019-02-01526110.3390/universe5020061universe5020061Bayesian Analysis for Extracting Properties of the Nuclear Equation of State from Observational Data Including Tidal Deformability from GW170817Alexander Ayriyan0David Alvarez-Castillo1David Blaschke2Hovik Grigorian3Laboratory for Information Technologies, Joint Institute for Nuclear Research, Joliot-Curie Street 6, Dubna 141980, RussiaBogoliubov Laboratory for Theoretical Physics, Joint Institute for Nuclear Research, Joliot-Curie Street 6, Dubna 141980, RussiaBogoliubov Laboratory for Theoretical Physics, Joint Institute for Nuclear Research, Joliot-Curie Street 6, Dubna 141980, RussiaLaboratory for Information Technologies, Joint Institute for Nuclear Research, Joliot-Curie Street 6, Dubna 141980, RussiaWe develop a Bayesian analysis method for selecting the most probable equation of state under a set of constraints from compact star physics, which now include the tidal deformability from GW170817. We apply this method for the first time to a two-parameter family of hybrid equations of state that is based on realistic models for the hadronic phase (KVORcut02) and the quark matter phase (SFM<inline-formula> <math display="inline"> <semantics> <mi>α</mi> </semantics> </math> </inline-formula>) which produce a third family of hybrid stars in the mass⁻radius diagram. One parameter (<inline-formula> <math display="inline"> <semantics> <mi>α</mi> </semantics> </math> </inline-formula>) characterizes the screening of the string tension in the string-flip model of quark matter while the other (<inline-formula> <math display="inline"> <semantics> <msub> <mo>Δ</mo> <mi>P</mi> </msub> </semantics> </math> </inline-formula>) belongs to the mixed phase construction that mimics the thermodynamics of pasta phases and includes the Maxwell construction as a limiting case for <inline-formula> <math display="inline"> <semantics> <mrow> <msub> <mo>Δ</mo> <mi>P</mi> </msub> <mo>=</mo> <mn>0</mn> </mrow> </semantics> </math> </inline-formula>. We present the corresponding results for compact star properties like mass, radius and tidal deformabilities and use empirical data for them in the newly developed Bayesian analysis method to obtain the probabilities for the model parameters within their considered range.https://www.mdpi.com/2218-1997/5/2/61bayesian analysisquark–hadron phase transitionpasta phaseshybrid compact starsmass–radius relationGW170817tidal deformability |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Alexander Ayriyan David Alvarez-Castillo David Blaschke Hovik Grigorian |
spellingShingle |
Alexander Ayriyan David Alvarez-Castillo David Blaschke Hovik Grigorian Bayesian Analysis for Extracting Properties of the Nuclear Equation of State from Observational Data Including Tidal Deformability from GW170817 Universe bayesian analysis quark–hadron phase transition pasta phases hybrid compact stars mass–radius relation GW170817 tidal deformability |
author_facet |
Alexander Ayriyan David Alvarez-Castillo David Blaschke Hovik Grigorian |
author_sort |
Alexander Ayriyan |
title |
Bayesian Analysis for Extracting Properties of the Nuclear Equation of State from Observational Data Including Tidal Deformability from GW170817 |
title_short |
Bayesian Analysis for Extracting Properties of the Nuclear Equation of State from Observational Data Including Tidal Deformability from GW170817 |
title_full |
Bayesian Analysis for Extracting Properties of the Nuclear Equation of State from Observational Data Including Tidal Deformability from GW170817 |
title_fullStr |
Bayesian Analysis for Extracting Properties of the Nuclear Equation of State from Observational Data Including Tidal Deformability from GW170817 |
title_full_unstemmed |
Bayesian Analysis for Extracting Properties of the Nuclear Equation of State from Observational Data Including Tidal Deformability from GW170817 |
title_sort |
bayesian analysis for extracting properties of the nuclear equation of state from observational data including tidal deformability from gw170817 |
publisher |
MDPI AG |
series |
Universe |
issn |
2218-1997 |
publishDate |
2019-02-01 |
description |
We develop a Bayesian analysis method for selecting the most probable equation of state under a set of constraints from compact star physics, which now include the tidal deformability from GW170817. We apply this method for the first time to a two-parameter family of hybrid equations of state that is based on realistic models for the hadronic phase (KVORcut02) and the quark matter phase (SFM<inline-formula> <math display="inline"> <semantics> <mi>α</mi> </semantics> </math> </inline-formula>) which produce a third family of hybrid stars in the mass⁻radius diagram. One parameter (<inline-formula> <math display="inline"> <semantics> <mi>α</mi> </semantics> </math> </inline-formula>) characterizes the screening of the string tension in the string-flip model of quark matter while the other (<inline-formula> <math display="inline"> <semantics> <msub> <mo>Δ</mo> <mi>P</mi> </msub> </semantics> </math> </inline-formula>) belongs to the mixed phase construction that mimics the thermodynamics of pasta phases and includes the Maxwell construction as a limiting case for <inline-formula> <math display="inline"> <semantics> <mrow> <msub> <mo>Δ</mo> <mi>P</mi> </msub> <mo>=</mo> <mn>0</mn> </mrow> </semantics> </math> </inline-formula>. We present the corresponding results for compact star properties like mass, radius and tidal deformabilities and use empirical data for them in the newly developed Bayesian analysis method to obtain the probabilities for the model parameters within their considered range. |
topic |
bayesian analysis quark–hadron phase transition pasta phases hybrid compact stars mass–radius relation GW170817 tidal deformability |
url |
https://www.mdpi.com/2218-1997/5/2/61 |
work_keys_str_mv |
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