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Calder, Alan C., Wang, Edward Y. M. (2002) Numerical Models of Binary Neutron Star System Mergers. II. Coalescing Models with Post‐Newtonian Radiation Reaction Forces. The Astrophysical Journal, 570 (1). 303-313 doi:10.1086/339743

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Reference TypeJournal (article/letter/editorial)
TitleNumerical Models of Binary Neutron Star System Mergers. II. Coalescing Models with Post‐Newtonian Radiation Reaction Forces
JournalThe Astrophysical Journal
AuthorsCalder, Alan C.Author
Wang, Edward Y. M.Author
Year2002 (May)Volume570
Issue1
PublisherIOP Publishing
DOIdoi:10.1086/339743Search in ResearchGate
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Mindat Ref. ID3353669Long-form Identifiermindat:1:5:3353669:5
GUID0
Full ReferenceCalder, Alan C., Wang, Edward Y. M. (2002) Numerical Models of Binary Neutron Star System Mergers. II. Coalescing Models with Post‐Newtonian Radiation Reaction Forces. The Astrophysical Journal, 570 (1). 303-313 doi:10.1086/339743
Plain TextCalder, Alan C., Wang, Edward Y. M. (2002) Numerical Models of Binary Neutron Star System Mergers. II. Coalescing Models with Post‐Newtonian Radiation Reaction Forces. The Astrophysical Journal, 570 (1). 303-313 doi:10.1086/339743
In(2002, May) The Astrophysical Journal Vol. 570 (1) IOP Publishing

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Swesty, F. Douglas, Wang, Edward Y. M., Calder, Alan C. (2000) Numerical Models of Binary Neutron Star System Mergers. I. Numerical Methods and Equilibrium Data for Newtonian Models. The Astrophysical Journal, 541 (2). 937-958 doi:10.1086/309460
Bernuzzi, Sebastiano, Thierfelder, Marcus, Brügmann, Bernd (2012) Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms. Physical Review D, 85 (10). doi:10.1103/physrevd.85.104030
Sun, Boyang (2023) Comparison of different models for gravitational and electromagnetic radiation of binary neutron star mergers. Journal of Physics: Conference Series, 2441 (1) 12022 doi:10.1088/1742-6596/2441/1/012022
Titarchuk, Lev, Shaposhnikov, Nickolai (2002) Three Type I X-Ray Bursts from Cygnus X-2: Application of Analytical Models for Neutron Star Mass and Radius Determination. The Astrophysical Journal, 570 (1). doi:10.1086/340834
Wiseman, Alan G. (1992) Coalescing binary systems of compact objects to(post)5/2-Newtonian order. II. Higher-order wave forms and radiation recoil. Physical Review D, 46 (4). 1517-1539 doi:10.1103/physrevd.46.1517
Will, C. M. (1976) A test of post-newtonian conservation laws in the binary system PSR 1913+16. The Astrophysical Journal, 205. 861pp. doi:10.1086/154342
Oohara, K.-i., Nakamura, T. (1992) Gravitational Radiation from Coalescing Binary Neutron Stars. V: Post-Newtonian Calculation. Progress of Theoretical Physics, 88. 307-315 doi:10.1143/ptp/88.2.307
Young, P. (1980) Numerical models of star clusters with a central black hole. I - Adiabatic models. The Astrophysical Journal, 242. 1232pp. doi:10.1086/158553
Kopeikin, S. M., Ozernoy, L. M. (1999) Post‐Newtonian Theory for Precision Doppler Measurements of Binary Star Orbits. The Astrophysical Journal, 523 (2). 771-785 doi:10.1086/307759
Portilla, M., Lapiedra, R. (1984) Long-term post-Newtonian effects in a binary system. The Astrophysical Journal, 286. 633pp. doi:10.1086/162638
Malone, R. C., Johnson, M. B., Bethe, H. A. (1975) Neutron star models with realistic high-density equations of state. The Astrophysical Journal, 199. 741pp. doi:10.1086/153746
 
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