Rainer Spurzem

Chinese Academy of Sciences — China

Physics and Astronomy · Physical Sciences

43h-index5.1kcitations359works3.32yr avg
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Research Topics

Stellar, planetary, and galactic studies(193), Astronomy and Astrophysical Research(110), Astrophysics and Star Formation Studies(95), Astrophysical Phenomena and Observations(84), Astro and Planetary Science(70)

Publications359 total

Pulsars and Millisecond Pulsars III: Tracing Compact Object Dynamics in Globular Clusters with NBODY6++GPU
Communications of the Byurakan Astrophysical Observatory·2026Open Access
Dynamical evolution of massless particles in star clusters with NBODY6++GPU-MASSLESS
Astronomy and Astrophysics·2026Open Access
The effects of star-gas interactions on binary evolution in open clusters
arXiv (Cornell University)·2026Open Access
The effects of star-gas interactions on binary evolution in open clusters
ArXiv.org·2026Open Access
From Nbody1 to Nbody7: the Growth of Sverres Industry
arXiv (Cornell University)·2025Open Access
From Nbody1 to Nbody7: the Growth of Sverres Industry
ArXiv.org·2025Open Access
Modelling Millisecond Pulsar Populations in Globular Clusters with NBODY6++GPU
arXiv (Cornell University)·2025Open Access
Rapid formation of a very massive star (&gt;50000 M <sub>⊙</sub> ), and subsequently, of an IMBH, from runaway collisions
Astronomy and Astrophysics·2025· 2 citedOpen Access
NbodyCP: A Direct <i>N</i> -body Simulation Code for Composite Stellar Populations of Single and Binary Star Clusters
Research in Astronomy and Astrophysics·2025· 1 citedOpen Access
DRAGON-III simulation: modelling million-body globular and nuclear star clusters
arXiv (Cornell University)·2025Open Access
Pulsars and Millisecond Pulsars II: Deep diving into the Evolutionary Mechanisms
Communications of the Byurakan Astrophysical Observatory·2025· 1 citedOpen Access
Efficient black hole seed formation in low metallicity and dense stellar clusters with implications for JWST sources
arXiv (Cornell University)·2025· 2 citedOpen Access
Formation and Evolution of Compact Binaries Containing Intermediate-mass Black Holes in Dense Star Clusters
The Astrophysical Journal·2025· 5 citedOpen Access
Evolution of star clusters with initial bulk rotation via <i>N</i>-body simulations
Astronomy and Astrophysics·2025· 3 citedOpen Access
Rapid formation of a very massive star &gt;50000 $M_\odot$ and subsequently an IMBH from runaway collisions. Direct N-body and Monte Carlo simulations of dense star clusters
arXiv (Cornell University)·2025Open Access
Formation and Evolution of Compact Binaries Containing Intermediate Mass Black Holes in Dense Star Clusters`
arXiv (Cornell University)·2025Open Access
Pulsars and Millisecond Pulsars I: Advancements, Open Questions and finding Gaps via statistical insights
Communications of the Byurakan Astrophysical Observatory·2024· 2 citedOpen Access
Dynamical evolution of massless particles in star clusters with NBODY6++GPU-MASSLESS
Astronomy and Astrophysics·2024· 2 citedOpen Access
Dynamical evolution of massless particles in star clusters with NBODY6++GPU-MASSLESS: I. Free-floating MLPs
arXiv (Cornell University)·2024Open Access
Influence of planets on debris discs in star clusters – II. The impact of stellar density
Monthly Notices of the Royal Astronomical Society·2024· 2 citedOpen Access
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Frequent Co-authors

Peter Berczik(18), Mirek Giersz(11), Long Wang(7), M. B. N. Kouwenhoven(7), Manuel Arca Sedda(6), A. Just(6), Thorsten Naab(5), David Merritt(4), Abbas Askar(4), Simon Portegies Zwart(4), Maxwell Xu Cai(4), S. J. Aarseth(3), Pau Amaro‐Seoane(3), Shuo Li(3), Francesco Paolo Rizzuto(3), C. Olczak(3), Taras Panamarev(3), Xuefei Gong(2), Yun-Kau Lau(2), Zhoujian Cao(2)