Black hole spin and mass function in gaseous proto-clusters

Project Information

ProtoBH

Grant agreement ID: 101149270

DOI

10.3030/101149270

Project closed

EC signature date 8 April 2024

Start date 1 September 2024

End date 31 August 2026

Funded under

• Marie Skłodowska-Curie Actions (MSCA)

Total cost

No data

EU contribution

€ 188 590,08

Coordinated by

UNIVERSITA' DEGLI STUDI DI MILANO-BICOCCA
Italy

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Links to deliverables and publications from FP7 projects, as well as links to some specific result types such as dataset and software, are dynamically retrieved from OpenAIRE .

Deliverables

Documents, reports (1)

Communication, Dissemination & Exploitation Plan

The plan describes the planned measures to maximize the impact ofthe project, including the dissemination and exploitation measures that are planned, and the target group(s) addressed. Regarding communication measuresand public engagement strategy, the aim is to inform and reach out to society andshow the activities performed, and the use and the benefits the project will have forcitizens.

Data Management Plan (1)

Data Management Plan

The Data Management Plan describes the data management life cyclefor all data sets that will be collected, processed or generated by the action. It is adocument describing what data will be collected, processed or generated andfollowing what methodology and standards, whether and how this data will beshared and/or made open, and how it will be curated and preserved.

Publications

Peer reviewed articles (7)

Black hole spin-mass correlation and vector resonant relaxation in gaseous star clusters: The origin of GW231123?

Author(s): Zacharias Roupas
Published in: Astronomy & Astrophysics, Issue 714, 2026, ISSN 0004-6361
Publisher: EDP Sciences
DOI: 10.48550/ARXIV.2607.17869

Spin-up and spin distribution of stellar black holes grown by gas accretion in proto-stellar clusters

Author(s): Zacharias Roupas
Published in: Astronomy & Astrophysics, Issue 709, 2026, ISSN 0004-6361
Publisher: EDP Sciences
DOI: 10.1051/0004-6361/202558435

Massive Black Hole Formation in Proto-Stellar Clusters via Early Gas Accretion

Author(s): Zacharias Roupas
Published in: Particles, Issue 9, 2026, ISSN 2571-712X
Publisher: MDPI AG
DOI: 10.3390/PARTICLES9010018

Radical reform is needed to combat power abuses in academia

Author(s): Zacharias Roupas
Published in: Nature Human Behaviour, Issue 424, 2025, ISSN 2397-3374
Publisher: Springer Nature
DOI: 10.1038/S41562-025-02127-3

Black hole spin-mass correlation and vector resonant relaxation in gaseous star clusters: the origin for GW231123?

Author(s): Zacharias Roupas
Published in: Astronomy & Astrophysics, 2026, ISSN 0004-6361
Publisher: EDP Sciences
DOI: 10.1051/0004-6361/202662023

Black hole mass function shift in proto-stellar clusters driven by gas accretion

Author(s): Zacharias Roupas
Published in: Astronomy & Astrophysics, Issue 702, 2025, ISSN 0004-6361
Publisher: EDP Sciences
DOI: 10.1051/0004-6361/202556434

Self-gravitating isothermal sphere in an expanding background

Author(s): Zacharias Roupas
Published in: Physical Review D, Issue 110, 2024, ISSN 2470-0010
Publisher: American Physical Society (APS)
DOI: 10.48550/ARXIV.2411.05393