2025ApJ...982..179M


Query : 2025ApJ...982..179M

2025ApJ...982..179M - Astrophys. J., 982, 179 (2025/April-1)

The Neutron Star Merger Delay-time Distribution, R-process “Knees,” and the Metal Budget of the Galaxy.

MAOZ D. and NAKAR E.

Abstract (from CDS):

For a sample of 18 currently known recycled millisecond pulsars (rMSPs) that are in double neutron star (DNS) systems, and 42 rMSPs with similar properties that are not in DNS pairs, we analyze the distributions of the characteristic age, τc, and the time-until-merger of the double systems, τgw. Based on the τc distribution of non-DNS rMSPs, we argue that τc is a reasonable estimator of true pulsar age and that rMSPs are active as pulsars for a long (≳Hubble) time. Among the DNSs there is an excess of young systems (small τc) with short life expectancy (small τgw) compared to model expectations for the distributions of τc and τgw if, at birth, DNSs have a delay-time distribution (DTD) of the form $\sim {\tau }_{{\rm{gw}}}^{-1}$ (expected generically for close binaries), or for that matter, from expectations from any single power-law DTD. A two-population DNS model solves the problem: the data are best fit by the combination of a “fast” population with DTD going as ${\tau }_{{\rm{gw}}}^{-1.9\pm 0.4}$, and a “slow” population of DNSs, with DTD proportional to ${\tau }_{{\rm{gw}}}^{-1.1\pm 0.15}$. The fast population can be equivalently represented by a shallow power-law DTD with an exponential cutoff beyond τgw ∼ 300 Myr. The fast population completely dominates, by a factor A ≈ 10-100, the numbers of DNSs that merge within a Hubble time, and that presumably lead to short gamma-ray bursts and kilonova explosions. Using a simple, empirically based, chemical-evolution calculation, we show that the fast/steep kilonova DTD, convolved with the measured star formation history of the Milky Way's thick-disk population, naturally reproduces the “knee” structure seen in abundance-ratio diagrams of thick-disk stars, for europium and for two other r-process elements. As a corollary, we show, based again solely on empirical input concerning iron production by supernovae, that the Milky Way is nearly a “closed box” that has retained at least ∼70%-90% of the metals produced over the Galaxy's lifetime.

Abstract Copyright: © 2025. The Author(s). Published by the American Astronomical Society.

Journal keyword(s): Neutron stars - Millisecond pulsars - Gamma-ray bursters - Binary pulsars - Galaxy chemical evolution - R-process

Simbad objects: 22

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Number of rows : 22
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 PSR J0453+1559 Psr 04 53 45.41372 +15 59 21.3000           ~ 92 0
2 PSR J0509+3801 Psr 05 09 31.788 +38 01 18.10           ~ 41 0
3 PSR J0737-3039 Psr 07 37 51.248 -30 39 40.83           ~ 445 1
4 PSR J1018-1523 Psr 10 18 12.72 -15 23 10.2           ~ 10 0
5 PSR J1208-5936 Psr 12 08 27.03010 -59 36 20.3812           ~ 8 0
6 NGC 4933 G 13 04 -11.5   13.18       ~ 10 0
7 NGC 4993 Sy2 13 09 47.6908761600 -23 23 02.314044636   13.34   11.92   ~ 397 0
8 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
9 PSR J1325-6253 Psr 13 25 04.8907 -62 53 39.594           ~ 14 0
10 PSR J1411+2551 Psr 14 11 18.866 +25 51 08.39           ~ 50 0
11 PSR J1518+4904 Psr 15 18 16.832 +49 04 34.19           ~ 201 1
12 PSR B1534+11 Psr 15 37 09.9603 +11 55 55.554           ~ 453 1
13 PSR J1756-2251 Psr 17 56 46.63 -22 51 59.4           ~ 153 1
14 PSR J1757-1854 Psr 17 57 03.78438 -18 54 03.3760           ~ 67 0
15 PSR J1759+5036 Psr 17 59 45.672 +50 36 56.96           ~ 17 0
16 PSR B1809-17.6 Psr 18 11 55.034 -17 36 37.70           ~ 114 1
17 PSR J1829+2456 Psr 18 29 34.6668 +24 56 18.193           ~ 89 1
18 PSR J1906+0749 Psr 19 06 48.67 +07 46 28.6           ~ 172 1
19 PSR J1913+1102 Psr 19 13 29.0542 +11 02 05.741           ~ 64 0
20 PSR J1915+1606 Psr 19 15 27.99999 +16 06 27.4034     22.5     ~ 1032 1
21 PSR J1930-1852 Psr 19 30 29.7156 -18 51 46.270           ~ 54 0
22 PSR J1946+2052 Psr 19 46 14.1438633037 +20 52 24.333605451           ~ 65 0

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