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pro vyhledávání: '"Martinez, Miguel A. S."'
Autor:
Prieto, Elena González, Kremer, Kyle, Fragione, Giacomo, Martinez, Miguel A. S., Weatherford, Newlin C., Zevin, Michael, Rasio, Frederic A.
The existence of black holes (BHs) with masses in the range between stellar remnants and supermassive BHs has only recently become unambiguously established. GW190521, a gravitational wave signal detected by the LIGO/Virgo Collaboration, provides the
Externí odkaz:
http://arxiv.org/abs/2208.07881
Observations have shown that the majority of massive stars, progenitors of black holes (BHs), have on average more than one stellar companion. In triple systems, wide inner binaries can be driven to a merger by the third body due to long-term secular
Externí odkaz:
http://arxiv.org/abs/2105.01671
Autor:
Martinez, Miguel A. S., Fragione, Giacomo, Kremer, Kyle, Chatterjee, Sourav, Rodriguez, Carl L., Samsing, Johan, Ye, Claire S., Weatherford, Newlin C., Zevin, Michael, Naoz, Smadar, Rasio, Frederic A.
Hierarchical triples are expected to be produced by the frequent binary-mediated interactions in the cores of globular clusters. In some of these triples, the tertiary companion can drive the inner binary to merger following large eccentricity oscill
Externí odkaz:
http://arxiv.org/abs/2009.08468
Autor:
Fragione, Giacomo, Martinez, Miguel A. S., Kremer, Kyle, Chatterjee, Sourav, Rodriguez, Carl L., Ye, Claire S., Weatherford, Newlin C., Naoz, Smadar, Rasio, Frederic A.
Depending on the stellar type, more than $\sim 50$\% and $\sim 15\%$ of stars in the field have at least one and two stellar companions, respectively. Hierarchical systems can be assembled dynamically in dense star clusters, as a result of few-body e
Externí odkaz:
http://arxiv.org/abs/2007.11605
Autor:
Rodriguez, Carl L., Kremer, Kyle, Grudić, Michael Y., Hafen, Zachary, Chatterjee, Sourav, Fragione, Giacomo, Lamberts, Astrid, Martinez, Miguel A. S., Rasio, Frederic A., Weatherford, Newlin, Ye, Claire S.
We explore the possibility that GW190412, a binary black hole merger with a non-equal-mass ratio and significantly spinning primary, was formed through repeated black hole mergers in a dense super star cluster. Using a combination of semi-analytic pr
Externí odkaz:
http://arxiv.org/abs/2005.04239
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