Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers
TLDR
In this paper, the authors present the first comprehensive study of r-process element nucleosynthesis in the ejecta of compact binary mergers (CBMs) and their relic black hole (BH)-torus systems.Abstract:
We present the first comprehensive study of r-process element nucleosynthesis in the ejecta of compact binary mergers (CBMs) and their relic black hole (BH)–torus systems. The evolution of the BH–accretion tori is simulated for seconds with a Newtonian hydrodynamics code including viscosity effects, pseudo-Newtonian gravity for rotating BHs, and an energy-dependent two-moment closure scheme for the transport of electron neutrinos and antineutrinos. The investigated cases are guided by relativistic double neutron star (NS–NS) and NS–BH merger models, producing ∼3–6 M_⊙ BHs with rotation parameters of A_BH ∼ 0.8 and tori of 0.03–0.3 M_⊙. Our nucleosynthesis analysis includes the dynamical (prompt) ejecta expelled during the CBM phase and the neutrino and viscously driven outflows of the relic BH–torus systems. While typically ∼20–25 per cent of the initial accretion-torus mass are lost by viscously driven outflows, neutrino-powered winds contribute at most another ∼1 per cent, but neutrino heating enhances the viscous ejecta significantly. Since BH–torus ejecta possess a wide distribution of electron fractions (0.1–0.6) and entropies, they produce heavy elements from A ∼ 80 up to the actinides, with relative contributions of A ≳ 130 nuclei being subdominant and sensitively dependent on BH and torus masses and the exact treatment of shear viscosity. The combined ejecta of CBM and BH–torus phases can reproduce the solar abundances amazingly well for A ≳ 90. Varying contributions of the torus ejecta might account for observed variations of lighter elements with 40 ≤ Z ≤ 56 relative to heavier ones, and a considerable reduction of the prompt ejecta compared to the torus ejecta, e.g. in highly asymmetric NS–BH mergers, might explain the composition of heavy-element deficient stars.read more
Citations
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Origin of the heavy elements in binary neutron-star mergers from a gravitational-wave event
TL;DR: The ejected mass and a merger rate inferred from GW170817 imply that such mergers are a dominant mode of r-process production in the Universe.
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The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. II. UV, Optical, and Near-infrared Light Curves and Comparison to Kilonova Models
Philip S. Cowperthwaite,Edo Berger,V. A. Villar,Brian D. Metzger,Matt Nicholl,Ryan Chornock,P. K. Blanchard,Wen-fai Fong,Raffaella Margutti,Marcelle Soares-Santos,Marcelle Soares-Santos,Kate D. Alexander,S. Allam,J. Annis,D. Brout,Duncan A. Brown,R. E. Butler,R. E. Butler,H. S. Chen,H. T. Diehl,Zoheyr Doctor,Maria R. Drout,Tarraneh Eftekhari,Ben Farr,Ben Farr,D. A. Finley,Ryan J. Foley,Joshua A. Frieman,Joshua A. Frieman,Chris L. Fryer,Juan Garcia-Bellido,M. S. S. Gill,James Guillochon,K. Herner,Daniel E. Holz,Daniel E. Holz,Daniel Kasen,Daniel Kasen,Richard Kessler,Richard Kessler,J. P. Marriner,Thomas Matheson,E. H. Neilsen,Eliot Quataert,Antonella Palmese,Armin Rest,Armin Rest,M. Sako,Daniel Scolnic,Nathan Smith,Douglas L. Tucker,Peter K. G. Williams,Eduardo Balbinot,Jeffrey L. Carlin,Edward R. Cook,F. Durret,Tenglin Li,Paulo A. A. Lopes,A. C. C. Lourenço,Jennifer L. Marshall,G. E. Medina,J. Muir,Ricardo R. Muñoz,M. Sauseda,David J. Schlegel,L. F. Secco,A. K. Vivas,W. C. Wester,Alfredo Zenteno,Yanxi Zhang,T. M. C. Abbott,Manda Banerji,Keith Bechtol,A. Benoit-Lévy,A. Benoit-Lévy,E. Bertin,E. Buckley-Geer,D. L. Burke,Diego Capozzi,A. Carnero Rosell,M. Carrasco Kind,Francisco J. Castander,Martin Crocce,Carlos E. Cunha,C. B. D'Andrea,L. N. da Costa,C. Davis,Darren L. DePoy,Shantanu Desai,J. P. Dietrich,Alex Drlica-Wagner,Tim Eifler,August E. Evrard,Enrique Fernández,B. Flaugher,Pablo Fosalba,Enrique Gaztanaga,D. W. Gerdes,Tommaso Giannantonio,Tommaso Giannantonio,Daniel A. Goldstein,Daniel A. Goldstein,Daniel Gruen,Robert A. Gruendl,G. Gutierrez,K. Honscheid,Bhuvnesh Jain,David J. James,Tesla E. Jeltema,M. W. G. Johnson,M. D. Johnson,S. Kent,S. Kent,Elisabeth Krause,Richard G. Kron,Richard G. Kron,Kyler Kuehn,N. Nuropatkin,Ofer Lahav,Marcos Lima,Huan Lin,Marcio A. G. Maia,M. March,Paul Martini,Richard G. McMahon,Felipe Menanteau,Christopher J. Miller,Ramon Miquel,Ramon Miquel,Joseph J. Mohr,Joseph J. Mohr,Eric H. Neilsen,Robert C. Nichol,Ricardo L. C. Ogando,A. A. Plazas,Natalie A. Roe,A. K. Romer,A. Roodman,Eli S. Rykoff,E. J. Sanchez,V. Scarpine,R. H. Schindler,Michael Schubnell,I. Sevilla-Noarbe,M. Smith,R. C. Smith,Flavia Sobreira,E. Suchyta,M. E. C. Swanson,G. Tarle,Daniel Thomas,R. C. Thomas,Michael Troxel,Vinu Vikram,Alistair R. Walker,Risa H. Wechsler,Risa H. Wechsler,Jochen Weller,Jochen Weller,Jochen Weller,Brian Yanny,J. Zuntz +161 more
TL;DR: In this article, the Gordon and Betty Moore Foundation (GBMF5076) and the Heising-Simons Foundation (HSPF) have contributed to the creation of the DES-Brazil Consortium.
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First results from the IllustrisTNG simulations: a tale of two elements - chemical evolution of magnesium and europium
Jill Naiman,Annalisa Pillepich,Volker Springel,Enrico Ramirez-Ruiz,Paul Torrey,Mark Vogelsberger,Rüdiger Pakmor,Dylan Nelson,Federico Marinacci,Lars Hernquist,Rainer Weinberger,Shy Genel +11 more
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Journal ArticleDOI
Constraining the Maximum Mass of Neutron Stars from Multi-messenger Observations of GW170817
Ben Margalit,Brian D. Metzger +1 more
TL;DR: In this paper, the authors combine electromagnetic and gravitational wave information on the binary neutron star (NS) merger GW170817 in order to constrain the radii and maximum mass of NSs.
Journal ArticleDOI
The Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars
Nial R. Tanvir,Andrew J. Levan,Carlos González-Fernández,Oleg Korobkin,Ilya Mandel,Stephan Rosswog,Jens Hjorth,P. D'Avanzo,A. S. Fruchter,Chris L. Fryer,Tuomas Kangas,Bo Milvang-Jensen,S. Rosetti,Danny Steeghs,Ryan Wollaeger,Zach Cano,Chris M. Copperwheat,Stefano Covino,Valerio D'Elia,Valerio D'Elia,A. de Ugarte Postigo,A. de Ugarte Postigo,P. A. Evans,Wesley Even,Stephen Fairhurst,R. Figuera Jaimes,Christopher J. Fontes,Yuri I. Fujii,Yuri I. Fujii,Johan P. U. Fynbo,B. P. Gompertz,Jochen Greiner,G. Hodosan,Mike Irwin,Pall Jakobsson,U. G. Jørgensen,David Alexander Kann,J. D. Lyman,D. Malesani,Richard G. McMahon,A. Melandri,P. T. O'Brien,J. P. Osborne,Eliana Palazzi,Daniel A. Perley,Elena Pian,S. Piranomonte,Markus Rabus,E. Rol,Antonia Rowlinson,Antonia Rowlinson,Steve Schulze,Patrick J. Sutton,Christina C. Thöne,Krzysztof Ulaczyk,Darach Watson,Klaas Wiersema,Ralph A. M. J. Wijers +57 more
TL;DR: In this article, the authors reported the discovery and monitoring of the near-infrared counterpart (AT2017gfo) of a binary neutron-star merger event detected as a gravitational wave source by Advanced Laser Interferometer Gravitational-wave Observatory (LIGO)/Virgo (GW170817) and as a short gamma-ray burst by Fermi Gamma-ray Burst Monitor (GBM) and Integral SPI-ACS (GRB 170817A).
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H. Ogin,John J. Oh,Seog Oh,Frank Ohme,M. A. Okada,M. Oliver,P. Oppermann,Richard J. Oram,B. O'Reilly,R. G. Ormiston,L. F. Ortega,Richard O'Shaughnessy,S. Ossokine,David J. Ottaway,H. Overmier,Benjamin J. Owen,A. E. Pace,J. Page,M. A. Page,Archana Pai,S. A. Pai,J. R. Palamos,O. V. Palashov,C. Palomba,A. Pal-Singh,Howard Pan,Huang-Wei Pan,B. Pang,P. T. H. Pang,C. Pankow,Francesco Pannarale,B. C. Pant,F. Paoletti,A. Paoli,Maria Alessandra Papa,A. Parida,W. Parker,D. Pascucci,A. Pasqualetti,R. Passaquieti,D. Passuello,Mandar Patil,B. Patricelli,B. L. Pearlstone,M. Pedraza,R. Pedurand,Larne Pekowsky,A. Pele,S. Penn,C. J. Perez,A. Perreca,L. M. Perri,Harald P. Pfeiffer,M. Phelps,O. J. Piccinni,M. Pichot,F. Piergiovanni,Vincenzo Pierro,G. Pillant,L. Pinard,Innocenzo M. Pinto,M. Pirello,Matthew Pitkin,M. Poe,Rosa Poggiani,P. Popolizio,Edward K. Porter,A. Post,Jade Powell,J. Prasad,J. W. W. Pratt,Geraint Pratten,V. Predoi,T. Prestegard,M. Prijatelj,Maria Ilaria Del Principe,S. Privitera,Reinhard Prix,G. A. Prodi,L. G. Prokhorov,O. Puncken,M. Punturo,P. Puppo,M. Pürrer,H. Qi,V. Quetschke,E. A. Quintero,R. Quitzow-James,F. J. Raab,D. S. Rabeling,H. Radkins,P. Raffai,S. Raja,C. Rajan,B. Rajbhandari,M. Rakhmanov,K. E. Ramirez,Antoni Ramos-Buades,P. Rapagnani,Vivien Raymond,M. Razzano,Jocelyn Read,Tania Regimbau,L. Rei,Stuart Reid,D. H. Reitze,W. Ren,Steven Reyes,F. Ricci,Paul M. Ricker,S. Rieger,K. Riles,M. Rizzo,N. A. Robertson,R. Robie,F. Robinet,A. Rocchi,L. Rolland,J. G. Rollins,V. J. Roma,J. D. Romano,Rocco Romano,C. L. Romel,J. H. Romie,D. Rosińska,M. P. Ross,Sheila Rowan,A. Rüdiger,P. Ruggi,G. Rutins,Kris Ryan,Surabhi Sachdev,T. Sadecki,Laleh Sadeghian,Mairi Sakellariadou,L. Salconi,M. Saleem,Francesco Salemi,A. Samajdar,L. Sammut,Laura Sampson,E. J. Sanchez,L. E. Sanchez,Nicolas Sanchis-Gual,V. Sandberg,J. R. Sanders,Benoit Sassolas,Bangalore Suryanarayana Sathyaprakash,Peter R. Saulson,O. E. S. Sauter,R. L. Savage,A. Sawadsky,P. Schale,Mark A. Scheel,Jacob Scheuer,J. Schmidt,Patricia Schmidt,Roman Schnabel,R. M. S. Schofield,A. Schönbeck,E. Schreiber,D. Schuette,B. W. Schulte,Bernard F. Schutz,S. G. Schwalbe,J. Scott,S. M. Scott,Edward Seidel,D. Sellers,A. S. Sengupta,D. Sentenac,V. Sequino,A. M. Sergeev,Daniel A. Shaddock,T. J. Shaffer,A. A. Shah,M. S. Shahriar,M. B. Shaner,Lijing Shao,B. Shapiro,P. Shawhan,A. Sheperd,D. H. Shoemaker,D. M. Shoemaker,K. Siellez,Xavier Siemens,M. Sieniawska,D. Sigg,A. D. Silva,Leo Singer,A. P. Singh,A. Singhal,Alicia M. Sintes,B. J. J. Slagmolen,Beverly J. Smith,J. R. Smith,Rory Smith,Surendra Nadh Somala,E. J. Son,J. A. Sonnenberg,B. Sorazu,Fiodor Sorrentino,Tarun Souradeep,A. P. Spencer,A. K. Srivastava,Kai Staats,A. Staley,M. Steinke,Jessica Steinlechner,Sebastian Steinlechner,D. Steinmeyer,S. P. Stevenson,Robert Stone,D. J. Stops,Kenneth A. Strain,G. Stratta,S. E. Strigin,A. Strunk,Riccardo Sturani,A. L. Stuver,T. Summerscales,L. Sun,S. Sunil,J. Suresh,P. J. Sutton,B. L. Swinkels,Marek Szczepanczyk,M. Tacca,S. C. Tait,Colm Talbot,D. Talukder,David B. Tanner,Márton Tápai,Andrea Taracchini,Jay D. Tasson,J. A. Taylor,R. Taylor,Sumanta Tewari,T. Theeg,F. Thies,E. G. Thomas,M. Thomas,P. Thomas,K. A. Thorne,Kip S. Thorne,Eric Thrane,S. N. Tiwari,V. Tiwari,K. V. Tokmakov,K. Toland,M. Tonelli,Z. Tornasi,Alejandro Torres-Forné,C. I. Torrie,D. Töyrä,F. Travasso,G. Traylor,J. Trinastic,M. C. Tringali,L. Trozzo,K. W. Tsang,Maggie Tse,R. Tso,Leo Tsukada,Daichi Tsuna,D. Tuyenbayev,K. Ueno,D. Ugolini,C. S. Unnikrishnan,A. L. Urban,S. A. Usman,H. Vahlbruch,G. Vajente,G. Valdes,Michele Vallisneri,N. van Bakel,M. van Beuzekom,J. F. J. van den Brand,C. Van Den Broeck,D. C. Vander-Hyde,L. van der Schaaf,J. V. van Heijningen,A. A. van Veggel,M. Vardaro,Vijay Varma,S. Vass,M. Vasúth,Alberto Vecchio,G. Vedovato,John Veitch,P. J. Veitch,K. Venkateswara,G. Venugopalan,D. Verkindt,F. Vetrano,A. Viceré,Aaron Viets,Serena Vinciguerra,D. J. Vine,J-Y. Vinet,Salvatore Vitale,T. Vo,H. Vocca,C. Vorvick,Sergey P. Vyatchanin,A. R. Wade,L. E. Wade,Madeline Wade,R. C. Walet,Michelle E. Walker,L. Wallace,S. Walsh,G. Wang,Haiyan Wang,J. Z. Wang,W. H. Wang,Y. F. Wang,R. L. Ward,J. Warner,M. Was,Jennifer Watchi,B. A. Weaver,L.-W. Wei,M. Weinert,A. J. Weinstein,Rainer Weiss,Linqing Wen,E. K. Wessel,P. Weßels,J. Westerweck,Tobias Westphal,K. Wette,James Whelan,S. E. Whitcomb,B. F. Whiting,C. Whittle,D. M. Wilken,David A. Williams,Roy Williams,A. R. Williamson,J. L. Willis,Benno Willke,M. H. Wimmer,Walter Winkler,C. C. Wipf,H. Wittel,Graham Woan,J. Woehler,J. K. Wofford,K. W. K. Wong,John Worden,J. L. Wright,D. S. Wu,Daniel Wysocki,S. Xiao,H. Yamamoto,C. C. Yancey,Lili Yang,M. J. Yap,Maher Yazback,Hang Yu,Haocun Yu,M. Yvert,A. K. Zadrożny,Michele Zanolin,T. Zelenova,J. P. Zendri,M. Zevin,L. Zhang,Mi Zhang,T. Zhang,Yanxi Zhang,Chunnong Zhao,Minchuan Zhou,Zifan Zhou,Sylvia J. Zhu,Xing-Jiang Zhu,Aaron Zimmerman,Michael E Zucker,J. Zweizig +1134 more