A hybrid SPH/N-body method for star cluster simulations
We present a new hybrid smoothed particle hydrodynamics (SPH)/N-body method for modelling the collisional stellar dynamics of young clusters in a live gas background. By deriving the equations of motion from Lagrangian mechanics we obtain a formally conservative combined SPH-N-body scheme. The SPH g...
Gespeichert in:
| Hauptverfasser: | , , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
11 April 2013
|
| In: |
Monthly notices of the Royal Astronomical Society
Year: 2013, Jahrgang: 430, Heft: 3, Pages: 1599-1616 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sts694 |
| Online-Zugang: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/sts694 |
| Verfasserangaben: | D.A. Hubber, R.J. Allison, R. Smith, S.P. Goodwin |
MARC
| LEADER | 00000caa a2200000 c 4500 | ||
|---|---|---|---|
| 001 | 178482559X | ||
| 003 | DE-627 | ||
| 005 | 20220921120849.0 | ||
| 007 | cr uuu---uuuuu | ||
| 008 | 220105s2013 xx |||||o 00| ||eng c | ||
| 024 | 7 | |a 10.1093/mnras/sts694 |2 doi | |
| 035 | |a (DE-627)178482559X | ||
| 035 | |a (DE-599)KXP178482559X | ||
| 035 | |a (OCoLC)1341436572 | ||
| 040 | |a DE-627 |b ger |c DE-627 |e rda | ||
| 041 | |a eng | ||
| 084 | |a 29 |2 sdnb | ||
| 100 | 1 | |a Hubber, David A. |e VerfasserIn |0 (DE-588)1248791983 |0 (DE-627)1784826383 |4 aut | |
| 245 | 1 | 2 | |a A hybrid SPH/N-body method for star cluster simulations |c D.A. Hubber, R.J. Allison, R. Smith, S.P. Goodwin |
| 264 | 1 | |c 11 April 2013 | |
| 336 | |a Text |b txt |2 rdacontent | ||
| 337 | |a Computermedien |b c |2 rdamedia | ||
| 338 | |a Online-Ressource |b cr |2 rdacarrier | ||
| 500 | |a Gesehen am 05.01.2022 | ||
| 520 | |a We present a new hybrid smoothed particle hydrodynamics (SPH)/N-body method for modelling the collisional stellar dynamics of young clusters in a live gas background. By deriving the equations of motion from Lagrangian mechanics we obtain a formally conservative combined SPH-N-body scheme. The SPH gas particles are integrated with a second-order Leapfrog, and the stars with a fourth-order Hermite scheme. Our new approach is intended to bridge the divide between the detailed, but expensive, full hydrodynamical simulations of star formation and pure N-body simulations of gas-free star clusters. We have implemented this hybrid approach in the SPH code seren and perform a series of simple tests to demonstrate the fidelity of the algorithm and its conservation properties. We investigate and present resolution criteria to adequately resolve the density field and to prevent strong numerical scattering effects. Future developments will include a more sophisticated treatment of binaries. | ||
| 700 | 1 | |a Allison, Richard James |e VerfasserIn |0 (DE-588)1058404636 |0 (DE-627)796848351 |0 (DE-576)41456040X |4 aut | |
| 700 | 1 | |a Smith, R. |e VerfasserIn |4 aut | |
| 700 | 1 | |a Goodwin, Simon |e VerfasserIn |0 (DE-588)1268556122 |0 (DE-627)1817207652 |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |a Royal Astronomical Society |t Monthly notices of the Royal Astronomical Society |d Oxford : Oxford Univ. Press, 1827 |g 430(2013), 3, Seite 1599-1616 |h Online-Ressource |w (DE-627)314059164 |w (DE-600)2016084-7 |w (DE-576)090955420 |x 1365-2966 |7 nnas |
| 773 | 1 | 8 | |g volume:430 |g year:2013 |g number:3 |g pages:1599-1616 |a A hybrid SPH/N-body method for star cluster simulations |
| 856 | 4 | 0 | |u https://doi.org/10.1093/mnras/sts694 |x Verlag |x Resolving-System |z lizenzpflichtig |3 Volltext |
| 951 | |a AR | ||
| 992 | |a 20220105 | ||
| 993 | |a Article | ||
| 994 | |a 2013 | ||
| 998 | |g 1058404636 |a Allison, Richard James |m 1058404636:Allison, Richard James |d 700000 |d 714000 |d 714200 |e 700000PA1058404636 |e 714000PA1058404636 |e 714200PA1058404636 |k 0/700000/ |k 1/700000/714000/ |k 2/700000/714000/714200/ |p 1 |x j | ||
| 999 | |a KXP-PPN178482559X |e 4030221963 | ||
| BIB | |a Y | ||
| SER | |a journal | ||
| JSO | |a {"language":["eng"],"relHost":[{"origin":[{"publisherPlace":"Oxford ; Oxford [u.a.] ; Oxford [u.a.]","dateIssuedKey":"1827","publisher":"Oxford Univ. Press ; Blackwell ; Wiley-Blackwell","dateIssuedDisp":"1827-"}],"id":{"doi":["10.1111/(ISSN)1365-2966"],"eki":["314059164"],"zdb":["2016084-7"],"issn":["1365-2966"]},"physDesc":[{"extent":"Online-Ressource"}],"title":[{"title_sort":"Monthly notices of the Royal Astronomical Society","title":"Monthly notices of the Royal Astronomical Society"}],"note":["Gesehen am 15.01.2018"],"type":{"bibl":"periodical","media":"Online-Ressource"},"disp":"Royal Astronomical SocietyMonthly notices of the Royal Astronomical Society","language":["eng"],"corporate":[{"role":"aut","display":"Royal Astronomical Society","roleDisplay":"VerfasserIn"}],"recId":"314059164","pubHistory":["1.1827 -"],"part":{"volume":"430","text":"430(2013), 3, Seite 1599-1616","pages":"1599-1616","issue":"3","year":"2013"}}],"recId":"178482559X","note":["Gesehen am 05.01.2022"],"type":{"media":"Online-Ressource","bibl":"article-journal"},"id":{"doi":["10.1093/mnras/sts694"],"eki":["178482559X"]},"origin":[{"dateIssuedDisp":"11 April 2013","dateIssuedKey":"2013"}],"title":[{"title_sort":"hybrid SPH/N-body method for star cluster simulations","title":"A hybrid SPH/N-body method for star cluster simulations"}],"person":[{"role":"aut","roleDisplay":"VerfasserIn","display":"Hubber, David A.","given":"David A.","family":"Hubber"},{"display":"Allison, Richard James","roleDisplay":"VerfasserIn","role":"aut","family":"Allison","given":"Richard James"},{"family":"Smith","given":"R.","roleDisplay":"VerfasserIn","display":"Smith, R.","role":"aut"},{"role":"aut","roleDisplay":"VerfasserIn","display":"Goodwin, Simon","given":"Simon","family":"Goodwin"}],"name":{"displayForm":["D.A. Hubber, R.J. Allison, R. Smith, S.P. Goodwin"]}} | ||
| SRT | |a HUBBERDAVIHYBRIDSPHN1120 | ||