TU Darmstadt / ULB / TUbiblio

Constraining the onset density of the hadron-quark phase transition with gravitational-wave observations

Blacker, Sebastian ; Bastian, Niels-Uwe F. ; Bauswein, Andreas ; Blaschke, David B. ; Fischer, Tobias ; Oertel, Micaela ; Soultanis, Theodoros ; Typel, Stefan (2020)
Constraining the onset density of the hadron-quark phase transition with gravitational-wave observations.
In: Physical Review D, 102 (12)
doi: 10.1103/PhysRevD.102.123023
Artikel, Bibliographie

Kurzbeschreibung (Abstract)

We study the possible occurrence of the hadron-quark phase transition (PT) during the merging of neutron star binaries by hydrodynamical simulations employing a set of temperature-dependent hybrid equations of state (EOSs). Following previous work, we describe an unambiguous and measurable signature of deconfined quark matter in the gravitational-wave (GW) signal of neutron star binary mergers including equal-mass and unequal-mass systems of different total binary mass. The softening of the EOS by the PT at higher densities, i.e., after merging, leads to a characteristic increase of the dominant postmerger GW frequency fpeak relative to the tidal deformability Λ inferred during the premerger inspiral phase. Hence, measuring such an increase of the postmerger frequency provides evidence for the presence of a strong PT. If the postmerger frequency and the tidal deformability are compatible with results from purely baryonic EOS models yielding very tight relations between fpeak and Λ, a strong PT can be excluded up to a certain density. We find tight correlations of fpeak and Λ with the maximum density during the early postmerger remnant evolution. These GW observables thus inform about the density regime which is probed by the remnant and its GW emission. Exploiting such relations, we devise a directly applicable, concrete procedure to constrain the onset density of the QCD PT from future GW measurements. We point out two interesting scenarios: if no indications for a PT are inferred from a GW detection, our procedure yields a lower limit on the onset density of the hadron-quark PT. On the contrary, if a merger event reveals evidence for the occurrence of deconfined quark matter, the inferred GW parameters set an upper limit on the PT onset density. Both scenarios would thus have strong implications for high-density matter physics, e.g., determining the range of validity of nuclear physics and constraining the properties for quark deconfinement. These prospects demonstrate the importance of simultaneously measuring pre- and postmerger GW signals to exploit the complementarity of the information encoded in both phases. Hence, our work stresses the value added by dedicated high-frequency GW instruments.

Typ des Eintrags: Artikel
Erschienen: 2020
Autor(en): Blacker, Sebastian ; Bastian, Niels-Uwe F. ; Bauswein, Andreas ; Blaschke, David B. ; Fischer, Tobias ; Oertel, Micaela ; Soultanis, Theodoros ; Typel, Stefan
Art des Eintrags: Bibliographie
Titel: Constraining the onset density of the hadron-quark phase transition with gravitational-wave observations
Sprache: Englisch
Publikationsjahr: 22 Dezember 2020
Verlag: APS Physics
Titel der Zeitschrift, Zeitung oder Schriftenreihe: Physical Review D
Jahrgang/Volume einer Zeitschrift: 102
(Heft-)Nummer: 12
DOI: 10.1103/PhysRevD.102.123023
URL / URN: https://journals.aps.org/prd/abstract/10.1103/PhysRevD.102.1...
Kurzbeschreibung (Abstract):

We study the possible occurrence of the hadron-quark phase transition (PT) during the merging of neutron star binaries by hydrodynamical simulations employing a set of temperature-dependent hybrid equations of state (EOSs). Following previous work, we describe an unambiguous and measurable signature of deconfined quark matter in the gravitational-wave (GW) signal of neutron star binary mergers including equal-mass and unequal-mass systems of different total binary mass. The softening of the EOS by the PT at higher densities, i.e., after merging, leads to a characteristic increase of the dominant postmerger GW frequency fpeak relative to the tidal deformability Λ inferred during the premerger inspiral phase. Hence, measuring such an increase of the postmerger frequency provides evidence for the presence of a strong PT. If the postmerger frequency and the tidal deformability are compatible with results from purely baryonic EOS models yielding very tight relations between fpeak and Λ, a strong PT can be excluded up to a certain density. We find tight correlations of fpeak and Λ with the maximum density during the early postmerger remnant evolution. These GW observables thus inform about the density regime which is probed by the remnant and its GW emission. Exploiting such relations, we devise a directly applicable, concrete procedure to constrain the onset density of the QCD PT from future GW measurements. We point out two interesting scenarios: if no indications for a PT are inferred from a GW detection, our procedure yields a lower limit on the onset density of the hadron-quark PT. On the contrary, if a merger event reveals evidence for the occurrence of deconfined quark matter, the inferred GW parameters set an upper limit on the PT onset density. Both scenarios would thus have strong implications for high-density matter physics, e.g., determining the range of validity of nuclear physics and constraining the properties for quark deconfinement. These prospects demonstrate the importance of simultaneously measuring pre- and postmerger GW signals to exploit the complementarity of the information encoded in both phases. Hence, our work stresses the value added by dedicated high-frequency GW instruments.

Zusätzliche Informationen:

Art.No.: 123023

Fachbereich(e)/-gebiet(e): 05 Fachbereich Physik
05 Fachbereich Physik > Institut für Kernphysik
05 Fachbereich Physik > Institut für Kernphysik > Theoretische Kernphysik
05 Fachbereich Physik > Institut für Kernphysik > Theoretische Kernphysik > Kernphysik und Nukleare Astrophysik
05 Fachbereich Physik > Institut für Kernphysik > Theoretische Kernphysik > Kern- und Vielteilchenphysik
05 Fachbereich Physik > Institut für Kernphysik > Theoretische Kernphysik > Theoretische nukleare Astrophysik
TU-Projekte: DFG|SFB1245|Z Schwenk SFB1245
Hinterlegungsdatum: 13 Jul 2022 08:03
Letzte Änderung: 20 Dez 2022 15:18
PPN: 503104221
Export:
Suche nach Titel in: TUfind oder in Google
Frage zum Eintrag Frage zum Eintrag

Optionen (nur für Redakteure)
Redaktionelle Details anzeigen Redaktionelle Details anzeigen