Population synthesis of double neutron stars
Identifieur interne : 006349 ( Main/Curation ); précédent : 006348; suivant : 006350Population synthesis of double neutron stars
Auteurs : S. Osłowski [Australie] ; T. Bulik [Pologne] ; D. Gondek-Rosi Ska [Pologne, France] ; K. Belczy Ski [Pologne, États-Unis]Source :
- Monthly Notices of the Royal Astronomical Society [ 0035-8711 ] ; 2011-05-01.
Descripteurs français
- Pascal (Inist)
English descriptors
- KwdEn :
- Accretion, Accretion rate, Alfv, Angular velocity, Astron, Belczy, Belczynski, Best model, Bhattacharya, Binary, Binary evolution, Binary radio pulsars, Binary stars, Black points, Bmin, Bulik, Chirp, Chirp mass, Chirp masses, Cordes, Death line, Death lines, Dnss, Double neutron stars, Galaxies, Gonthier, Gravitational, Gravitational potential, Gravitational wave, Gravitational waves, Hubble time, Initial masses, Kalogera, Kaspi, Kiel, Konar, Lipunov, Luminosity, Lyne, Magnetic fields, Main sequence, Mass ratio, Mass ratios, Mass scale, Mass transfer, Maximum mass, Merger times, Millisecond pulsars, Mnras, Modelled, Modelling, Models, Monthly notices, Neutron, Neutron star, Neutron star binaries, Neutron stars, Orbital period, Ostriker, Phys, Pmbps, Population synthesis, Probability density, Propeller, Propeller effect, Pulsar, Pulsar evolution, Pulsars, Radio pulsars, Radio selection effects, Radiowave radiation, Recycling, Rudak, Same time, Second pulsar, Selection effect, Selection effects, Semimajor axis, Spatial distribution, Startrack, Startrack code, Stellar, Stellar evolution, Supernova, Urpin, Wave emission, Woosley.
- Teeft :
- Accretion, Accretion rate, Alfv, Angular velocity, Astron, Belczy, Belczynski, Best model, Bhattacharya, Binary, Binary evolution, Binary radio pulsars, Black points, Bmin, Bulik, Chirp, Chirp mass, Chirp masses, Cordes, Death line, Death lines, Dnss, Double neutron stars, Gonthier, Gravitational, Gravitational wave, Gravitational waves, Hubble time, Initial masses, Kalogera, Kaspi, Kiel, Konar, Lipunov, Luminosity, Lyne, Main sequence, Mass ratio, Mass ratios, Mass scale, Mass transfer, Maximum mass, Merger times, Millisecond pulsars, Mnras, Modelled, Modelling, Monthly notices, Neutron, Neutron star, Neutron star binaries, Neutron stars, Orbital period, Ostriker, Phys, Pmbps, Population synthesis, Probability density, Propeller, Propeller effect, Pulsar, Pulsar evolution, Radio pulsars, Radio selection effects, Recycling, Rudak, Same time, Second pulsar, Selection effects, Semimajor axis, Startrack, Startrack code, Stellar, Stellar evolution, Supernova, Urpin, Woosley.
Abstract
Using the StarTrack binary population synthesis code we model the population of double neutron stars in the Galaxy. We include a detailed treatment of the spin evolution of each pulsar due to processes such as spin‐down and spin‐up during accretion events as well as magnetic field decay. We also model the spatial distribution of double neutron stars by including their natal kicks and subsequent propagation in the Galactic gravitational potential. This synthetic pulsar population is compared to the observed sample of double neutron stars taking into account the selection effects of detection in the radio band, to determine the most likely evolutionary parameters. With these parameters we determine the properties of the double neutron star binaries detectable in gravitational waves by the high‐frequency interferometers LIGO and VIRGO. In particular, we discuss the distributions of chirp masses and mass ratios in samples selected by their radio or gravitational wave emission.
Url:
DOI: 10.1111/j.1365-2966.2010.18147.x
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Gondek-Rosi Ska</name><affiliation wicri:level="1"><country xml:lang="fr">Pologne</country><wicri:regionArea>Nicolaus Copernicus Astronomical Centre, Bartycka 18, 00716 Warszawa</wicri:regionArea><wicri:noRegion>00716 Warszawa</wicri:noRegion></affiliation><affiliation wicri:level="1"><country xml:lang="fr">Pologne</country><wicri:regionArea>Institute of Astronomy, University of Zielona Gòra, Lubuska 2, 65‐265 Zielona Gòra</wicri:regionArea><wicri:noRegion>65‐265 Zielona Gòra</wicri:noRegion></affiliation><affiliation wicri:level="3"><country xml:lang="fr">France</country><wicri:regionArea>LUTH, Observatoire de Paris, Universite Paris 7, Place Jules Janssen, 92195 Meudon Cedex</wicri:regionArea><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Meudon</settlement></placeName></affiliation></author><author><name sortKey="Belczy Ski, K" sort="Belczy Ski, K" uniqKey="Belczy Ski K" first="K." last="Belczy Ski">K. Belczy Ski</name><affiliation wicri:level="1"><country xml:lang="fr">Pologne</country><wicri:regionArea>Astronomical Observatory, University of Warsaw, Aleje Ujazdowskie 4, 00‐478 Warsaw</wicri:regionArea><wicri:noRegion>00‐478 Warsaw</wicri:noRegion></affiliation><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Physics and Astronomy, University of Texas, Brownsville, TX 78520</wicri:regionArea><placeName><region type="state">Texas</region></placeName></affiliation></author></analytic><monogr></monogr><series><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="alt">MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY</title><idno type="ISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><imprint><biblScope unit="vol">413</biblScope><biblScope unit="issue">1</biblScope><biblScope unit="page" from="461">461</biblScope><biblScope unit="page" to="479">479</biblScope><biblScope unit="page-count">19</biblScope><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2011-05-01">2011-05-01</date></imprint><idno type="ISSN">0035-8711</idno></series></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Accretion</term><term>Accretion rate</term><term>Alfv</term><term>Angular velocity</term><term>Astron</term><term>Belczy</term><term>Belczynski</term><term>Best model</term><term>Bhattacharya</term><term>Binary</term><term>Binary evolution</term><term>Binary radio pulsars</term><term>Binary stars</term><term>Black points</term><term>Bmin</term><term>Bulik</term><term>Chirp</term><term>Chirp mass</term><term>Chirp masses</term><term>Cordes</term><term>Death line</term><term>Death lines</term><term>Dnss</term><term>Double neutron stars</term><term>Galaxies</term><term>Gonthier</term><term>Gravitational</term><term>Gravitational potential</term><term>Gravitational wave</term><term>Gravitational waves</term><term>Hubble time</term><term>Initial masses</term><term>Kalogera</term><term>Kaspi</term><term>Kiel</term><term>Konar</term><term>Lipunov</term><term>Luminosity</term><term>Lyne</term><term>Magnetic fields</term><term>Main sequence</term><term>Mass ratio</term><term>Mass ratios</term><term>Mass scale</term><term>Mass transfer</term><term>Maximum mass</term><term>Merger times</term><term>Millisecond pulsars</term><term>Mnras</term><term>Modelled</term><term>Modelling</term><term>Models</term><term>Monthly notices</term><term>Neutron</term><term>Neutron star</term><term>Neutron star binaries</term><term>Neutron stars</term><term>Orbital period</term><term>Ostriker</term><term>Phys</term><term>Pmbps</term><term>Population synthesis</term><term>Probability density</term><term>Propeller</term><term>Propeller effect</term><term>Pulsar</term><term>Pulsar evolution</term><term>Pulsars</term><term>Radio pulsars</term><term>Radio selection effects</term><term>Radiowave radiation</term><term>Recycling</term><term>Rudak</term><term>Same time</term><term>Second pulsar</term><term>Selection effect</term><term>Selection effects</term><term>Semimajor axis</term><term>Spatial distribution</term><term>Startrack</term><term>Startrack code</term><term>Stellar</term><term>Stellar evolution</term><term>Supernova</term><term>Urpin</term><term>Wave emission</term><term>Woosley</term></keywords><keywords scheme="Pascal" xml:lang="fr"><term>Accrétion</term><term>Binaire</term><term>Champ magnétique</term><term>Effet sélection</term><term>Emission onde</term><term>Etoile neutron</term><term>Galaxies</term><term>Modèle</term><term>Onde gravitationnelle</term><term>Onde radio</term><term>Potentiel gravitationnel</term><term>Pulsar</term><term>Rapport masse</term><term>Répartition spatiale</term></keywords><keywords scheme="Teeft" xml:lang="en"><term>Accretion</term><term>Accretion rate</term><term>Alfv</term><term>Angular velocity</term><term>Astron</term><term>Belczy</term><term>Belczynski</term><term>Best model</term><term>Bhattacharya</term><term>Binary</term><term>Binary evolution</term><term>Binary radio pulsars</term><term>Black points</term><term>Bmin</term><term>Bulik</term><term>Chirp</term><term>Chirp mass</term><term>Chirp masses</term><term>Cordes</term><term>Death line</term><term>Death lines</term><term>Dnss</term><term>Double neutron stars</term><term>Gonthier</term><term>Gravitational</term><term>Gravitational wave</term><term>Gravitational waves</term><term>Hubble time</term><term>Initial masses</term><term>Kalogera</term><term>Kaspi</term><term>Kiel</term><term>Konar</term><term>Lipunov</term><term>Luminosity</term><term>Lyne</term><term>Main sequence</term><term>Mass ratio</term><term>Mass ratios</term><term>Mass scale</term><term>Mass transfer</term><term>Maximum mass</term><term>Merger times</term><term>Millisecond pulsars</term><term>Mnras</term><term>Modelled</term><term>Modelling</term><term>Monthly notices</term><term>Neutron</term><term>Neutron star</term><term>Neutron star binaries</term><term>Neutron stars</term><term>Orbital period</term><term>Ostriker</term><term>Phys</term><term>Pmbps</term><term>Population synthesis</term><term>Probability density</term><term>Propeller</term><term>Propeller effect</term><term>Pulsar</term><term>Pulsar evolution</term><term>Radio pulsars</term><term>Radio selection effects</term><term>Recycling</term><term>Rudak</term><term>Same time</term><term>Second pulsar</term><term>Selection effects</term><term>Semimajor axis</term><term>Startrack</term><term>Startrack code</term><term>Stellar</term><term>Stellar evolution</term><term>Supernova</term><term>Urpin</term><term>Woosley</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">Using the StarTrack binary population synthesis code we model the population of double neutron stars in the Galaxy. We include a detailed treatment of the spin evolution of each pulsar due to processes such as spin‐down and spin‐up during accretion events as well as magnetic field decay. We also model the spatial distribution of double neutron stars by including their natal kicks and subsequent propagation in the Galactic gravitational potential. This synthetic pulsar population is compared to the observed sample of double neutron stars taking into account the selection effects of detection in the radio band, to determine the most likely evolutionary parameters. With these parameters we determine the properties of the double neutron star binaries detectable in gravitational waves by the high‐frequency interferometers LIGO and VIRGO. In particular, we discuss the distributions of chirp masses and mass ratios in samples selected by their radio or gravitational wave emission.</div></front></TEI><double idat="0035-8711:2011:Oslowski S:population:synthesis:of"><INIST><TEI><teiHeader><fileDesc><titleStmt><title xml:lang="en" level="a">Population synthesis of double neutron stars</title><author><name sortKey="Oslowski, S" sort="Oslowski, S" uniqKey="Oslowski S" first="S." last="Oslowski">S. Oslowski</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Swinburne University of Technology, Centre for Astrophysics and Supercomputing. Mail H39, PO Box 218</s1><s2>VIC 3122</s2><s3>AUS</s3><sZ>1 aut.</sZ></inist:fA14><country>Australie</country><wicri:noRegion>VIC 3122</wicri:noRegion></affiliation><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>CSIRO Astronomy and Space Sciences, Australia Telescope National Facility, PO Box 76</s1><s2>Epping, NSW 1710</s2><s3>AUS</s3><sZ>1 aut.</sZ></inist:fA14><country>Australie</country><wicri:noRegion>Epping, NSW 1710</wicri:noRegion></affiliation></author><author><name sortKey="Bulik, T" sort="Bulik, T" uniqKey="Bulik T" first="T." last="Bulik">T. Bulik</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>Astronomical Observatory, University of Warsaw, Aleje Ujazdowskie 4</s1><s2>00-478 Warsaw</s2><s3>POL</s3><sZ>2 aut.</sZ><sZ>4 aut.</sZ></inist:fA14><country>Pologne</country><wicri:noRegion>00-478 Warsaw</wicri:noRegion></affiliation><affiliation wicri:level="1"><inist:fA14 i1="04"><s1>Nicolaus Copernicus Astronomical Centre, Bartvcka 18</s1><s2>00716 Warszawa</s2><s3>POL</s3><sZ>2 aut.</sZ><sZ>3 aut.</sZ></inist:fA14><country>Pologne</country><wicri:noRegion>00716 Warszawa</wicri:noRegion></affiliation></author><author><name sortKey="Gondek Rosinska, D" sort="Gondek Rosinska, D" uniqKey="Gondek Rosinska D" first="D." last="Gondek-Rosinska">D. Gondek-Rosinska</name><affiliation wicri:level="1"><inist:fA14 i1="04"><s1>Nicolaus Copernicus Astronomical Centre, Bartvcka 18</s1><s2>00716 Warszawa</s2><s3>POL</s3><sZ>2 aut.</sZ><sZ>3 aut.</sZ></inist:fA14><country>Pologne</country><wicri:noRegion>00716 Warszawa</wicri:noRegion></affiliation><affiliation wicri:level="1"><inist:fA14 i1="05"><s1>Institute of Astronomy, University of Zielona Gòra, Lubuska 2</s1><s2>65-265 Zielona Gòra</s2><s3>POL</s3><sZ>3 aut.</sZ></inist:fA14><country>Pologne</country><wicri:noRegion>65-265 Zielona Gòra</wicri:noRegion></affiliation><affiliation wicri:level="1"><inist:fA14 i1="06"><s1>LUTH, Observatoire de Paris, Universite Paris 7, Place Jules Janssen</s1><s2>92195 Meudon</s2><s3>FRA</s3><sZ>3 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>92195 Meudon</wicri:noRegion><wicri:noRegion>Place Jules Janssen</wicri:noRegion><wicri:noRegion>92195 Meudon</wicri:noRegion></affiliation></author><author><name sortKey="Belczynski, K" sort="Belczynski, K" uniqKey="Belczynski K" first="K." last="Belczynski">K. Belczynski</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>Astronomical Observatory, University of Warsaw, Aleje Ujazdowskie 4</s1><s2>00-478 Warsaw</s2><s3>POL</s3><sZ>2 aut.</sZ><sZ>4 aut.</sZ></inist:fA14><country>Pologne</country><wicri:noRegion>00-478 Warsaw</wicri:noRegion></affiliation><affiliation wicri:level="1"><inist:fA14 i1="07"><s1>Department of Physics and Astronomy, University of Texas</s1><s2>Brownsville, TX 78520</s2><s3>USA</s3><sZ>4 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>Brownsville, TX 78520</wicri:noRegion></affiliation></author></titleStmt><publicationStmt><idno type="wicri:source">INIST</idno><idno type="inist">11-0208604</idno><date when="2011">2011</date><idno type="stanalyst">PASCAL 11-0208604 INIST</idno><idno type="RBID">Pascal:11-0208604</idno><idno type="wicri:Area/PascalFrancis/Corpus">001E16</idno><idno type="wicri:Area/PascalFrancis/Curation">004124</idno><idno type="wicri:Area/PascalFrancis/Checkpoint">001777</idno><idno type="wicri:explorRef" wicri:stream="PascalFrancis" wicri:step="Checkpoint">001777</idno><idno type="wicri:doubleKey">0035-8711:2011:Oslowski S:population:synthesis:of</idno><idno type="wicri:Area/Main/Merge">006C28</idno></publicationStmt><sourceDesc><biblStruct><analytic><title xml:lang="en" level="a">Population synthesis of double neutron stars</title><author><name sortKey="Oslowski, S" sort="Oslowski, S" uniqKey="Oslowski S" first="S." last="Oslowski">S. Oslowski</name><affiliation wicri:level="1"><inist:fA14 i1="01"><s1>Swinburne University of Technology, Centre for Astrophysics and Supercomputing. Mail H39, PO Box 218</s1><s2>VIC 3122</s2><s3>AUS</s3><sZ>1 aut.</sZ></inist:fA14><country>Australie</country><wicri:noRegion>VIC 3122</wicri:noRegion></affiliation><affiliation wicri:level="1"><inist:fA14 i1="02"><s1>CSIRO Astronomy and Space Sciences, Australia Telescope National Facility, PO Box 76</s1><s2>Epping, NSW 1710</s2><s3>AUS</s3><sZ>1 aut.</sZ></inist:fA14><country>Australie</country><wicri:noRegion>Epping, NSW 1710</wicri:noRegion></affiliation></author><author><name sortKey="Bulik, T" sort="Bulik, T" uniqKey="Bulik T" first="T." last="Bulik">T. Bulik</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>Astronomical Observatory, University of Warsaw, Aleje Ujazdowskie 4</s1><s2>00-478 Warsaw</s2><s3>POL</s3><sZ>2 aut.</sZ><sZ>4 aut.</sZ></inist:fA14><country>Pologne</country><wicri:noRegion>00-478 Warsaw</wicri:noRegion></affiliation><affiliation wicri:level="1"><inist:fA14 i1="04"><s1>Nicolaus Copernicus Astronomical Centre, Bartvcka 18</s1><s2>00716 Warszawa</s2><s3>POL</s3><sZ>2 aut.</sZ><sZ>3 aut.</sZ></inist:fA14><country>Pologne</country><wicri:noRegion>00716 Warszawa</wicri:noRegion></affiliation></author><author><name sortKey="Gondek Rosinska, D" sort="Gondek Rosinska, D" uniqKey="Gondek Rosinska D" first="D." last="Gondek-Rosinska">D. Gondek-Rosinska</name><affiliation wicri:level="1"><inist:fA14 i1="04"><s1>Nicolaus Copernicus Astronomical Centre, Bartvcka 18</s1><s2>00716 Warszawa</s2><s3>POL</s3><sZ>2 aut.</sZ><sZ>3 aut.</sZ></inist:fA14><country>Pologne</country><wicri:noRegion>00716 Warszawa</wicri:noRegion></affiliation><affiliation wicri:level="1"><inist:fA14 i1="05"><s1>Institute of Astronomy, University of Zielona Gòra, Lubuska 2</s1><s2>65-265 Zielona Gòra</s2><s3>POL</s3><sZ>3 aut.</sZ></inist:fA14><country>Pologne</country><wicri:noRegion>65-265 Zielona Gòra</wicri:noRegion></affiliation><affiliation wicri:level="1"><inist:fA14 i1="06"><s1>LUTH, Observatoire de Paris, Universite Paris 7, Place Jules Janssen</s1><s2>92195 Meudon</s2><s3>FRA</s3><sZ>3 aut.</sZ></inist:fA14><country>France</country><wicri:noRegion>92195 Meudon</wicri:noRegion><wicri:noRegion>Place Jules Janssen</wicri:noRegion><wicri:noRegion>92195 Meudon</wicri:noRegion></affiliation></author><author><name sortKey="Belczynski, K" sort="Belczynski, K" uniqKey="Belczynski K" first="K." last="Belczynski">K. Belczynski</name><affiliation wicri:level="1"><inist:fA14 i1="03"><s1>Astronomical Observatory, University of Warsaw, Aleje Ujazdowskie 4</s1><s2>00-478 Warsaw</s2><s3>POL</s3><sZ>2 aut.</sZ><sZ>4 aut.</sZ></inist:fA14><country>Pologne</country><wicri:noRegion>00-478 Warsaw</wicri:noRegion></affiliation><affiliation wicri:level="1"><inist:fA14 i1="07"><s1>Department of Physics and Astronomy, University of Texas</s1><s2>Brownsville, TX 78520</s2><s3>USA</s3><sZ>4 aut.</sZ></inist:fA14><country>États-Unis</country><wicri:noRegion>Brownsville, TX 78520</wicri:noRegion></affiliation></author></analytic><series><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="abbreviated">Mon. Not. R. Astron. Soc.</title><idno type="ISSN">0035-8711</idno><imprint><date when="2011">2011</date></imprint></series></biblStruct></sourceDesc><seriesStmt><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="abbreviated">Mon. Not. R. Astron. Soc.</title><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Accretion</term><term>Binary stars</term><term>Galaxies</term><term>Gravitational potential</term><term>Gravitational waves</term><term>Magnetic fields</term><term>Mass ratio</term><term>Models</term><term>Neutron stars</term><term>Pulsars</term><term>Radiowave radiation</term><term>Selection effect</term><term>Spatial distribution</term><term>Wave emission</term></keywords><keywords scheme="Pascal" xml:lang="fr"><term>Etoile neutron</term><term>Modèle</term><term>Galaxies</term><term>Pulsar</term><term>Accrétion</term><term>Champ magnétique</term><term>Répartition spatiale</term><term>Potentiel gravitationnel</term><term>Effet sélection</term><term>Binaire</term><term>Onde gravitationnelle</term><term>Rapport masse</term><term>Onde radio</term><term>Emission onde</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">Using the STARTRACK binary population synthesis code we model the population of double neutron stars in the Galaxy. We include a detailed treatment of the spin evolution of each pulsar due to processes such as spin-down and spin-up during accretion events as well as magnetic field decay. We also model the spatial distribution of double neutron stars by including their natal kicks and subsequent propagation in the Galactic gravitational potential. This synthetic pulsar population is compared to the observed sample of double neutron stars taking into account the selection effects of detection in the radio band, to determine the most likely evolutionary parameters. With these parameters we determine the properties of the double neutron star binaries detectable in gravitational waves by the high-frequency interferometers LIGO and VIRGO. In particular, we discuss the distributions of chirp masses and mass ratios in samples selected by their radio or gravitational wave emission.</div></front></TEI></INIST><ISTEX><TEI wicri:istexFullTextTei="biblStruct"><teiHeader><fileDesc><titleStmt><title xml:lang="en">Population synthesis of double neutron stars</title><author><name sortKey="Oslowski, S" sort="Oslowski, S" uniqKey="Oslowski S" first="S." last="Osłowski">S. Osłowski</name></author><author><name sortKey="Bulik, T" sort="Bulik, T" uniqKey="Bulik T" first="T." last="Bulik">T. Bulik</name></author><author><name sortKey="Gondek Osi Ska, D" sort="Gondek Osi Ska, D" uniqKey="Gondek Osi Ska D" first="D." last="Gondek-Rosi Ska">D. Gondek-Rosi Ska</name></author><author><name sortKey="Belczy Ski, K" sort="Belczy Ski, K" uniqKey="Belczy Ski K" first="K." last="Belczy Ski">K. Belczy Ski</name></author></titleStmt><publicationStmt><idno type="wicri:source">ISTEX</idno><idno type="RBID">ISTEX:E8C7E49999427051D03B060835809228F3213FDC</idno><date when="2011" year="2011">2011</date><idno type="doi">10.1111/j.1365-2966.2010.18147.x</idno><idno type="url">https://api.istex.fr/document/E8C7E49999427051D03B060835809228F3213FDC/fulltext/pdf</idno><idno type="wicri:Area/Istex/Corpus">002B84</idno><idno type="wicri:explorRef" wicri:stream="Istex" wicri:step="Corpus" wicri:corpus="ISTEX">002B84</idno><idno type="wicri:Area/Istex/Curation">002B84</idno><idno type="wicri:Area/Istex/Checkpoint">000768</idno><idno type="wicri:explorRef" wicri:stream="Istex" wicri:step="Checkpoint">000768</idno><idno type="wicri:doubleKey">0035-8711:2011:Oslowski S:population:synthesis:of</idno><idno type="wicri:Area/Main/Merge">006725</idno></publicationStmt><sourceDesc><biblStruct><analytic><title level="a" type="main">Population synthesis of double neutron stars</title><author><name sortKey="Oslowski, S" sort="Oslowski, S" uniqKey="Oslowski S" first="S." last="Osłowski">S. Osłowski</name><affiliation wicri:level="1"><country xml:lang="fr">Australie</country><wicri:regionArea>Swinburne University of Technology, Centre for Astrophysics and Supercomputing, Mail H39, PO Box 218, VIC 3122</wicri:regionArea><wicri:noRegion>VIC 3122</wicri:noRegion></affiliation><affiliation wicri:level="1"><country xml:lang="fr">Australie</country><wicri:regionArea>CSIRO Astronomy and Space Sciences, Australia Telescope National Facility, PO Box 76, Epping, NSW 1710</wicri:regionArea><wicri:noRegion>NSW 1710</wicri:noRegion></affiliation><affiliation wicri:level="1"><country wicri:rule="url">Australie</country></affiliation></author><author><name sortKey="Bulik, T" sort="Bulik, T" uniqKey="Bulik T" first="T." last="Bulik">T. Bulik</name><affiliation wicri:level="1"><country xml:lang="fr">Pologne</country><wicri:regionArea>Astronomical Observatory, University of Warsaw, Aleje Ujazdowskie 4, 00‐478 Warsaw</wicri:regionArea><wicri:noRegion>00‐478 Warsaw</wicri:noRegion></affiliation><affiliation wicri:level="1"><country xml:lang="fr">Pologne</country><wicri:regionArea>Nicolaus Copernicus Astronomical Centre, Bartycka 18, 00716 Warszawa</wicri:regionArea><wicri:noRegion>00716 Warszawa</wicri:noRegion></affiliation></author><author><name sortKey="Gondek Osi Ska, D" sort="Gondek Osi Ska, D" uniqKey="Gondek Osi Ska D" first="D." last="Gondek-Rosi Ska">D. Gondek-Rosi Ska</name><affiliation wicri:level="1"><country xml:lang="fr">Pologne</country><wicri:regionArea>Nicolaus Copernicus Astronomical Centre, Bartycka 18, 00716 Warszawa</wicri:regionArea><wicri:noRegion>00716 Warszawa</wicri:noRegion></affiliation><affiliation wicri:level="1"><country xml:lang="fr">Pologne</country><wicri:regionArea>Institute of Astronomy, University of Zielona Gòra, Lubuska 2, 65‐265 Zielona Gòra</wicri:regionArea><wicri:noRegion>65‐265 Zielona Gòra</wicri:noRegion></affiliation><affiliation wicri:level="3"><country xml:lang="fr">France</country><wicri:regionArea>LUTH, Observatoire de Paris, Universite Paris 7, Place Jules Janssen, 92195 Meudon Cedex</wicri:regionArea><placeName><region type="region" nuts="2">Île-de-France</region><settlement type="city">Meudon</settlement></placeName></affiliation></author><author><name sortKey="Belczy Ski, K" sort="Belczy Ski, K" uniqKey="Belczy Ski K" first="K." last="Belczy Ski">K. Belczy Ski</name><affiliation wicri:level="1"><country xml:lang="fr">Pologne</country><wicri:regionArea>Astronomical Observatory, University of Warsaw, Aleje Ujazdowskie 4, 00‐478 Warsaw</wicri:regionArea><wicri:noRegion>00‐478 Warsaw</wicri:noRegion></affiliation><affiliation wicri:level="2"><country xml:lang="fr">États-Unis</country><wicri:regionArea>Department of Physics and Astronomy, University of Texas, Brownsville, TX 78520</wicri:regionArea><placeName><region type="state">Texas</region></placeName></affiliation></author></analytic><monogr></monogr><series><title level="j" type="main">Monthly Notices of the Royal Astronomical Society</title><title level="j" type="alt">MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY</title><idno type="ISSN">0035-8711</idno><idno type="eISSN">1365-2966</idno><imprint><biblScope unit="vol">413</biblScope><biblScope unit="issue">1</biblScope><biblScope unit="page" from="461">461</biblScope><biblScope unit="page" to="479">479</biblScope><biblScope unit="page-count">19</biblScope><publisher>Blackwell Publishing Ltd</publisher><pubPlace>Oxford, UK</pubPlace><date type="published" when="2011-05-01">2011-05-01</date></imprint><idno type="ISSN">0035-8711</idno></series></biblStruct></sourceDesc><seriesStmt><idno type="ISSN">0035-8711</idno></seriesStmt></fileDesc><profileDesc><textClass><keywords scheme="KwdEn" xml:lang="en"><term>Accretion</term><term>Accretion rate</term><term>Alfv</term><term>Angular velocity</term><term>Astron</term><term>Belczy</term><term>Belczynski</term><term>Best model</term><term>Bhattacharya</term><term>Binary</term><term>Binary evolution</term><term>Binary radio pulsars</term><term>Black points</term><term>Bmin</term><term>Bulik</term><term>Chirp</term><term>Chirp mass</term><term>Chirp masses</term><term>Cordes</term><term>Death line</term><term>Death lines</term><term>Dnss</term><term>Double neutron stars</term><term>Gonthier</term><term>Gravitational</term><term>Gravitational wave</term><term>Gravitational waves</term><term>Hubble time</term><term>Initial masses</term><term>Kalogera</term><term>Kaspi</term><term>Kiel</term><term>Konar</term><term>Lipunov</term><term>Luminosity</term><term>Lyne</term><term>Main sequence</term><term>Mass ratio</term><term>Mass ratios</term><term>Mass scale</term><term>Mass transfer</term><term>Maximum mass</term><term>Merger times</term><term>Millisecond pulsars</term><term>Mnras</term><term>Modelled</term><term>Modelling</term><term>Monthly notices</term><term>Neutron</term><term>Neutron star</term><term>Neutron star binaries</term><term>Neutron stars</term><term>Orbital period</term><term>Ostriker</term><term>Phys</term><term>Pmbps</term><term>Population synthesis</term><term>Probability density</term><term>Propeller</term><term>Propeller effect</term><term>Pulsar</term><term>Pulsar evolution</term><term>Radio pulsars</term><term>Radio selection effects</term><term>Recycling</term><term>Rudak</term><term>Same time</term><term>Second pulsar</term><term>Selection effects</term><term>Semimajor axis</term><term>Startrack</term><term>Startrack code</term><term>Stellar</term><term>Stellar evolution</term><term>Supernova</term><term>Urpin</term><term>Woosley</term></keywords><keywords scheme="Teeft" xml:lang="en"><term>Accretion</term><term>Accretion rate</term><term>Alfv</term><term>Angular velocity</term><term>Astron</term><term>Belczy</term><term>Belczynski</term><term>Best model</term><term>Bhattacharya</term><term>Binary</term><term>Binary evolution</term><term>Binary radio pulsars</term><term>Black points</term><term>Bmin</term><term>Bulik</term><term>Chirp</term><term>Chirp mass</term><term>Chirp masses</term><term>Cordes</term><term>Death line</term><term>Death lines</term><term>Dnss</term><term>Double neutron stars</term><term>Gonthier</term><term>Gravitational</term><term>Gravitational wave</term><term>Gravitational waves</term><term>Hubble time</term><term>Initial masses</term><term>Kalogera</term><term>Kaspi</term><term>Kiel</term><term>Konar</term><term>Lipunov</term><term>Luminosity</term><term>Lyne</term><term>Main sequence</term><term>Mass ratio</term><term>Mass ratios</term><term>Mass scale</term><term>Mass transfer</term><term>Maximum mass</term><term>Merger times</term><term>Millisecond pulsars</term><term>Mnras</term><term>Modelled</term><term>Modelling</term><term>Monthly notices</term><term>Neutron</term><term>Neutron star</term><term>Neutron star binaries</term><term>Neutron stars</term><term>Orbital period</term><term>Ostriker</term><term>Phys</term><term>Pmbps</term><term>Population synthesis</term><term>Probability density</term><term>Propeller</term><term>Propeller effect</term><term>Pulsar</term><term>Pulsar evolution</term><term>Radio pulsars</term><term>Radio selection effects</term><term>Recycling</term><term>Rudak</term><term>Same time</term><term>Second pulsar</term><term>Selection effects</term><term>Semimajor axis</term><term>Startrack</term><term>Startrack code</term><term>Stellar</term><term>Stellar evolution</term><term>Supernova</term><term>Urpin</term><term>Woosley</term></keywords></textClass></profileDesc></teiHeader><front><div type="abstract" xml:lang="en">Using the StarTrack binary population synthesis code we model the population of double neutron stars in the Galaxy. We include a detailed treatment of the spin evolution of each pulsar due to processes such as spin‐down and spin‐up during accretion events as well as magnetic field decay. We also model the spatial distribution of double neutron stars by including their natal kicks and subsequent propagation in the Galactic gravitational potential. This synthetic pulsar population is compared to the observed sample of double neutron stars taking into account the selection effects of detection in the radio band, to determine the most likely evolutionary parameters. With these parameters we determine the properties of the double neutron star binaries detectable in gravitational waves by the high‐frequency interferometers LIGO and VIRGO. In particular, we discuss the distributions of chirp masses and mass ratios in samples selected by their radio or gravitational wave emission.</div></front></TEI></ISTEX></double></record>Pour manipuler ce document sous Unix (Dilib)
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