Marco Dall'Amico
Marco Dall'Amico
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Dynamics
Never two without three
Binary black holes stand as one of the principal sources of gravitational waves in the Universe. Emitting ripples in the fabric of spacetime, black holes gradually spiral closer, eventually culminating in a merger. Binary black hole mergers stand out as the most energetic events in the Universe, observable from Earth with laser detectors known as interferometers. The ideal environment for the formation of binary black hole mergers is within star clusters – crowded neighborhoods of stars held together by gravity, where dynamical interactions between celestial bodies occur. In my research, I explore the mechanisms through which these interactions between stars and black holes lead to the formation of binary black hole mergers, with a particular focus on
binary-single encounters
.
May 10, 2024
Video
3-body interaction poster
An outreach poster about 3-body interaction between black holes that I created for the
Best Scientific Images
contest organized by STRUCTURES, Heidelberg. Open
HERE
the HD version of the poster or download
HERE
the pdf version.
Marco Dall'Amico
May 1, 2024
Let's light up a black hole!
An outreach activity I designed for the course
Designing innovative public engagement activities
presented at the astronomy outreach festival in
Castellaro Lagusello back in 2022
. The main idea of this laboratory is to show children how matter accreted by a black hole emits light, and how astronomers manage to ‘see’ the black hole precisely thanks to its accretion disk. If you want to reproduce this experiment, you can find
more info at this link
.
Marco Dall'Amico
May 1, 2024
Eccentric black hole mergers via three-body interactions in young, globular, and nuclear star clusters
Eccentric mergers are a signature of the dynamical formation channel of binary black holes (BBHs) in dense stellar environments and …
Marco Dall'Amico
,
Michela Mapelli
,
Stefano Torniamenti
,
Manuel Arca Sedda
PDF
Dataset
ADS
arXiv
Journal
Stellar mergers and beyond
Not only black holes can merge. Before being black holes, these objects were once massive stars. Stars are forged inside chaotic and crowded environments called young star clusters. There, they can interact with each other and, sometimes, they merge to produce even more massive stars. In my research, I study the history of these stars from their birth up to their death. I simulate their dynamical and stellar evolution and I study how the surrounding environment impacts their life and afterlife when they become massive black holes.
May 27, 2023
GW190521 formation via three-body encounters in young massive star clusters
GW190521 is the most massive binary black hole (BBH) merger observed to date, and its primary component lies in the pair-instability …
Marco Dall'Amico
,
Michela Mapelli
,
Ugo Nicolò Di Carlo
,
Yann Buffanais
,
Sara Rastello
,
Filippo Santoliquido
,
Alessandro Ballone
,
Manuel Arca Sedda
PDF
Video
ADS
arXiv
Journal
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