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pro vyhledávání: '"Higgins, Adam. B."'
Autor:
Kim, Sam, Schulze, Steve, Resmi, Lekshmi, González-López, Jorge, Higgins, Adam. B., Ishwara-Chandra, C. H., Bauer, Franz. E., de Gregorio-Monsalvo, Itziar, De Pasquale, Massimiliano, Postigo, Antonio de Ugarte, Kann, David A., Martín, Sergio, Oates, Samantha R., Starling, Rhaana L. C., Tanvir, Nial. R., Buchner, Johannes, Campana, Sergio, Cano, Zach, Covino, Stefano, Fruchter, Andrew S., Fynbo, Johan P. U., Hartmann, Dieter H., Hjorth, Jens, Jakobsson, Pall P., Levan, Andrew J., Malesani, Daniele, Michałowski, Michal J., Milvang-Jensen, Bo, Misra, Kuntal, O'Brien, Paul T., Sánchez-Ramírez, Rubén, Thöne, Christina C., Watson, Darach J., Wiersema, Klaas
Binary neutron-star mergers (BNSMs) are among the most readily detectable gravitational-wave (GW) sources with LIGO. They are also thought to produce short $\gamma$-ray bursts (SGRBs), and kilonovae that are powered by r-process nuclei. Detecting the
Externí odkaz:
http://arxiv.org/abs/1710.05847
