equation of state;
gravitational waves;
magnetic fields;
stars: magnetars;
stars: neutron;
GAMMA-RAY BURSTS;
EQUATION-OF-STATE;
NEWBORN MAGNETARS;
ENERGY INJECTION;
FIELD MAGNETAR;
EVOLUTION;
RADIATION;
EMISSION;
OUTBURST;
MATTER;
D O I:
10.1088/0004-637X/798/1/25
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Binary neutron star (NS) mergers are among the most promising sources of gravitational waves (GWs), as well as candidate progenitors for short gamma-ray bursts (SGRBs). Depending on the total initial mass of the system and the NS equation of state (EOS), the post-merger phase can be characterized by a prompt collapse to a black hole or by the formation of a supramassive NS, or even a stable NS. In the latter cases of post-merger NS (PMNS) formation, magnetic field amplification during the merger will produce a magnetar and induce a mass quadrupole moment in the newly formed NS. If the timescale for orthogonalization of the magnetic symmetry axis with the spin axis is smaller than the spindown time, the NS will radiate its spin down energy primarily via GWs. Here we study this scenario for the various outcomes of NS formation: we generalize the set of equilibrium states for a twisted torus magnetic configuration to include solutions that, for the same external dipolar field, carry a larger magnetic energy reservoir; we hence compute the magnetic ellipticity for such configurations, and the corresponding strength of the expected GW signal as a function of the relative magnitude of the dipolar and toroidal field components. The relative number of GW detections from PMNSs and from binary NSs is a very strong function of the NS EOS, being higher (similar to 1%) for the stiffest EOSs and negligibly small for the softest ones. For intermediate-stiffness EOSs, such as the n = 4/7 polytrope recently used by Giacomazzo and Perna or the GM1 used by Lasky et al., the relative fraction is 0.3%; correspondingly, we estimate a GW detection rate from stable PMNSs of similar to 0.1-1 yr(-1) with advanced detectors, and of similar to 100-1000 yr(-1) with detectors of third generation such as the Einstein Telescope. Measurement of such GW signals would provide constraints on the NS EOS and, in connection with an SGRB, on the nature of the binary progenitors giving rise to these events.
机构:
Univ Colorado, JILA, Boulder, CO 80309 USA
Natl Inst Stand & Technol, Boulder, CO 80309 USAUniv Colorado, JILA, Boulder, CO 80309 USA
Giacomazzo, Bruno
Perna, Rosalba
论文数: 0引用数: 0
h-index: 0
机构:
Univ Colorado, JILA, Boulder, CO 80309 USA
Univ Colorado, Dept Astrophys & Planetary Sci, Boulder, CO 80309 USAUniv Colorado, JILA, Boulder, CO 80309 USA
机构:
Univ Trento, Dipartimento Fis, Via Sommar 14, I-38123 Trento, Italy
INFN TIFPA, Trento Inst Fundamental Phys & Applicat, Via Sommar 14, I-38123 Trento, ItalyFriedrich Schiller Univ Jena, Theoret Phys Inst, D-07743 Jena, Germany
Camilletti, Alessandro
Prakash, Aviral
论文数: 0引用数: 0
h-index: 0
机构:
Penn State Univ, Inst Gravitat & Cosmos, University Pk, PA 16802 USA
Penn State Univ, Dept Phys, University Pk, PA 16802 USAFriedrich Schiller Univ Jena, Theoret Phys Inst, D-07743 Jena, Germany
机构:
Univ Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USAUniv Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
Foucart, Francois
Haas, Roland
论文数: 0引用数: 0
h-index: 0
机构:
Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, GermanyUniv Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
Haas, Roland
Duez, Matthew D.
论文数: 0引用数: 0
h-index: 0
机构:
Washington State Univ, Dept Phys & Astron, Pullman, WA 99164 USAUniv Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
Duez, Matthew D.
O'Connor, Evan
论文数: 0引用数: 0
h-index: 0
机构:
N Carolina State Univ, Dept Phys, Raleigh, NC 27695 USAUniv Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
O'Connor, Evan
Ott, Christian D.
论文数: 0引用数: 0
h-index: 0
机构:
CALTECH, Walter Burke Inst Theoret Phys, TAPIR, MC 350-17, Pasadena, CA 91125 USAUniv Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
Ott, Christian D.
Roberts, Luke
论文数: 0引用数: 0
h-index: 0
机构:
CALTECH, Walter Burke Inst Theoret Phys, TAPIR, MC 350-17, Pasadena, CA 91125 USAUniv Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
Roberts, Luke
Kidder, Lawrence E.
论文数: 0引用数: 0
h-index: 0
机构:
Cornell Univ, Cornell Ctr Astrophys & Planetary Sci, Ithaca, NY 14853 USAUniv Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
Kidder, Lawrence E.
Lippuner, Jonas
论文数: 0引用数: 0
h-index: 0
机构:
CALTECH, Walter Burke Inst Theoret Phys, TAPIR, MC 350-17, Pasadena, CA 91125 USAUniv Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
Lippuner, Jonas
Pfeiffer, Harald P.
论文数: 0引用数: 0
h-index: 0
机构:
Univ Toronto, Canadian Inst Theoret Astrophys, Toronto, ON M5S 3H8, Canada
Canadian Inst Adv Res, 180 Dundas St West, Toronto, ON M5G 1Z8, CanadaUniv Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
Pfeiffer, Harald P.
Scheel, Mark A.
论文数: 0引用数: 0
h-index: 0
机构:
CALTECH, Walter Burke Inst Theoret Phys, TAPIR, MC 350-17, Pasadena, CA 91125 USAUniv Calif Berkeley, Lawrence Berkeley Natl Lab, 1 Cyclotron Rd, Berkeley, CA 94720 USA
机构:
Max Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, GermanyMax Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany
Dietrich, Tim
Ujevic, Maximiliano
论文数: 0引用数: 0
h-index: 0
机构:
Univ Fed ABC, Ctr Ciencias Nat & Humanas, BR-09210170 Sao Paulo, BrazilMax Planck Inst Gravitat Phys, Albert Einstein Inst, D-14476 Golm, Germany