A
Alessandro A. Trani
Researcher at University of Tokyo
Publications - 49
Citations - 781
Alessandro A. Trani is an academic researcher from University of Tokyo. The author has contributed to research in topics: Supermassive black hole & Stars. The author has an hindex of 13, co-authored 33 publications receiving 519 citations. Previous affiliations of Alessandro A. Trani include Florida State University College of Arts and Sciences & International School for Advanced Studies.
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Merging black hole binaries with the SEVN code
Mario Spera,Michela Mapelli,Nicola Giacobbo,Nicola Giacobbo,Alessandro A. Trani,Alessandro A. Trani,Alessandro A. Trani,Alessandro Bressan,Alessandro Bressan,Guglielmo Costa +9 more
TL;DR: In this paper, a new version of the SEVN population-synthesis code was proposed to integrate stellar evolution by interpolation over a grid of stellar evolution tracks, and the authors used it to evolve a sample of binary stellar evolution processes.
Journal ArticleDOI
Binary black holes in young star clusters: The impact of metallicity
Ugo N Di Carlo,Ugo N Di Carlo,Michela Mapelli,Michela Mapelli,Nicola Giacobbo,Nicola Giacobbo,Mario Spera,Yann Bouffanais,Sara Rastello,Filippo Santoliquido,Mario Pasquato,Alessandro Ballone,Alessandro A. Trani,Alessandro A. Trani,Stefano Torniamenti,Francesco Haardt +15 more
TL;DR: In this article, the formation of black holes and binary black holes (BBHs) in young star clusters was studied by means of 6000 N-body simulations coupled with binary population synthesis.
Journal ArticleDOI
Merger rate density of Population III binary black holes below, above, and in the pair-instability mass gap
TL;DR: In this article, the authors presented the merger rate density of Population (Pop.) III binary black holes (BHs) by means of a widely-used binary population synthesis code BSE with extensions to very massive and extreme metal-poor stars.
Journal ArticleDOI
Merger Rate Density of Population III Binary Black Holes Below, Above, and in the Pair-instability Mass Gap
TL;DR: In this article, the authors presented the merger rate density of Population (Pop.) III binary black holes (BHs) by means of a widely-used binary population synthesis code BSE with extensions to very massive and extreme metal-poor stars.
Journal ArticleDOI
K2-264: a transiting multiplanet system in the Praesepe open cluster
John H. Livingston,Fei Dai,Fei Dai,Teruyuki Hirano,Davide Gandolfi,Alessandro A. Trani,Grzegorz Nowak,Grzegorz Nowak,William D. Cochran,Michael Endl,Simon Albrecht,Oscar Barragán,J. Cabrera,Sz. Csizmadia,J. P. de Leon,Hans J. Deeg,Hans J. Deeg,Ph. Eigmüller,Ph. Eigmüller,Anders Erikson,Malcolm Fridlund,Malcolm Fridlund,Akihiko Fukui,Akihiko Fukui,Sascha Grziwa,Eike W. Guenther,A. P. Hatzes,Judith Korth,Masayuki Kuzuhara,P. Montañes,P. Montañes,Norio Narita,David Nespral,David Nespral,Enric Palle,Enric Palle,Martin Pätzold,Carina M. Persson,Jorge Prieto-Arranz,Jorge Prieto-Arranz,Heike Rauer,Heike Rauer,Heike Rauer,Motohide Tamura,V. Van Eylen,Joshua N. Winn +45 more
TL;DR: In this paper, the authors presented the discovery of two planets transiting K2-264, an M2 dwarf in the intermediate age (600-800 Myr) Praesepe open cluster (also known as the Beehive Cluster, M44, or NGC 2632), which was observed by K2 during Campaign 16.