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Title: Formation of Tidal Captures and Gravitational Wave Inspirals in Binary-single Interactions

Abstract

We perform the first systematic study of how dynamical stellar tides and general relativistic (GR) effects affect the dynamics and outcomes of binary-single interactions. For this, we have constructed an N -body code that includes tides in the affine approximation, where stars are modeled as self-similar ellipsoidal polytropes, and GR corrections using the commonly used post-Newtonian formalism. Using this numerical formalism, we are able resolve the leading effect from tides and GR across several orders of magnitude in both stellar radius and initial target binary separation. We find that the main effect from tides is the formation of two-body tidal captures that form during the chaotic and resonant evolution of the triple system. The two stars undergoing the capture spiral in and merge. The inclusion of tides can thus lead to an increase in the stellar coalescence rate. We also develop an analytical framework for calculating the cross section of tidal inspirals between any pair of objects with similar mass. From our analytical and numerical estimates, we find that the rate of tidal inspirals relative to collisions increases as the initial semimajor axis of the target binary increases and the radius of the interacting tidal objects decreases. The largest effectmore » is therefore found for triple systems hosting white dwarfs and neutron stars (NSs). In this case, we find the rate of highly eccentric white dwarf—NS mergers to likely be dominated by tidal inspirals. While tidal inspirals occur rarely, we note that they can give rise to a plethora of thermonuclear transients, such as Ca-rich transients.« less

Authors:
 [1];  [2];  [3]
  1. Department of Astrophysical Sciences, Princeton University, Peyton Hall, 4 Ivy Lane, Princeton, NJ 08544 (United States)
  2. School of Natural Sciences, Institute for Advanced Study, 1 Einstein Drive, Princeton, NJ 08540 (United States)
  3. Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA 95064 (United States)
Publication Date:
OSTI Identifier:
22663182
Resource Type:
Journal Article
Journal Name:
Astrophysical Journal
Additional Journal Information:
Journal Volume: 846; Journal Issue: 1; Other Information: Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0004-637X
Country of Publication:
United States
Language:
English
Subject:
79 ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; APPROXIMATIONS; CAPTURE; COALESCENCE; COLLISIONS; CORRECTIONS; CROSS SECTIONS; GRAVITATIONAL WAVES; INCLUSIONS; INTERACTIONS; MASS; NEUTRON STARS; RELATIVISTIC RANGE; SIMULATION; STAR EVOLUTION; TRANSIENTS; TWO-BODY PROBLEM; WHITE DWARF STARS

Citation Formats

Samsing, Johan, MacLeod, Morgan, and Ramirez-Ruiz, Enrico. Formation of Tidal Captures and Gravitational Wave Inspirals in Binary-single Interactions. United States: N. p., 2017. Web. doi:10.3847/1538-4357/AA7E32.
Samsing, Johan, MacLeod, Morgan, & Ramirez-Ruiz, Enrico. Formation of Tidal Captures and Gravitational Wave Inspirals in Binary-single Interactions. United States. doi:10.3847/1538-4357/AA7E32.
Samsing, Johan, MacLeod, Morgan, and Ramirez-Ruiz, Enrico. Fri . "Formation of Tidal Captures and Gravitational Wave Inspirals in Binary-single Interactions". United States. doi:10.3847/1538-4357/AA7E32.
@article{osti_22663182,
title = {Formation of Tidal Captures and Gravitational Wave Inspirals in Binary-single Interactions},
author = {Samsing, Johan and MacLeod, Morgan and Ramirez-Ruiz, Enrico},
abstractNote = {We perform the first systematic study of how dynamical stellar tides and general relativistic (GR) effects affect the dynamics and outcomes of binary-single interactions. For this, we have constructed an N -body code that includes tides in the affine approximation, where stars are modeled as self-similar ellipsoidal polytropes, and GR corrections using the commonly used post-Newtonian formalism. Using this numerical formalism, we are able resolve the leading effect from tides and GR across several orders of magnitude in both stellar radius and initial target binary separation. We find that the main effect from tides is the formation of two-body tidal captures that form during the chaotic and resonant evolution of the triple system. The two stars undergoing the capture spiral in and merge. The inclusion of tides can thus lead to an increase in the stellar coalescence rate. We also develop an analytical framework for calculating the cross section of tidal inspirals between any pair of objects with similar mass. From our analytical and numerical estimates, we find that the rate of tidal inspirals relative to collisions increases as the initial semimajor axis of the target binary increases and the radius of the interacting tidal objects decreases. The largest effect is therefore found for triple systems hosting white dwarfs and neutron stars (NSs). In this case, we find the rate of highly eccentric white dwarf—NS mergers to likely be dominated by tidal inspirals. While tidal inspirals occur rarely, we note that they can give rise to a plethora of thermonuclear transients, such as Ca-rich transients.},
doi = {10.3847/1538-4357/AA7E32},
journal = {Astrophysical Journal},
issn = {0004-637X},
number = 1,
volume = 846,
place = {United States},
year = {2017},
month = {9}
}