Lucio Mayer

University of Zurich

Switzerland

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Articles (11)

Year:

2024

Year:

2024

Year:

2024

Year:

2024

Year:

2023

Year:

2023

Year:

2023

Year:

2023

Year:

2023

Year:

2023

Year:

2022

Collaborators (11)

Seoyoung Lyla Jung

University of Oxford

UNITED KINGDOM

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Ross Church

Lund University

SWEDEN

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Emanuele Berti

Professor

Johns Hopkins University

UNITED STATES

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Enrico Barausse

Associate professor

Scuola Internazionale Superiore di Studi Avanzati

ITALY

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Johan Richard

Université Claude Bernard Lyon 1

FRANCE

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Peter Johansson

University of Helsinki

FINLAND

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Tiziana DiMatteo

Director/Professor

Carnegie Mellon University

UNITED STATES

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Michael Tremmel

Lecturer

University College Cork

IRELAND

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Arif Babul

University Distinguished Professor

University of Victoria

CANADA

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Christopher Berry

University of Glasgow

UNITED KINGDOM

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Jessie Runnoe

Adjunct Professor of Physics

Fisk University

UNITED STATES

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Lucio Mayer

Research Interests

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Articles (11)

Direct Formation of Massive Black Holes via Dynamical Collapse in Metal-enriched Merging Galaxies at z ∼ 10: Fully Cosmological Simulations

High resolution modelling of [CII], [CI], [OIII], and CO line emission from the interstellar medium and circumgalactic medium of a star-forming galaxy at z ∼ 6.5

Stellar cluster formation in a Milky Way-sized galaxy at z > 4 – II. A hybrid formation scenario for the nuclear star cluster and its connection to the nuclear stellar ring

The minimum measurable eccentricity from gravitational waves of LISA massive black hole binaries

Astrophysics with the Laser Interferometer Space Antenna

Molecular gas cloud properties at z ≃ 1 revealed by the superb angular resolution achieved with ALMA and gravitational lensing

Characterizing fragmentation and sub-Jovian clump properties in magnetized young protoplanetary discs

Cool and gusty, with a chance of rain: dynamics of multiphase CGM around massive galaxies in the Romulus simulations

Direct collapse of exceptionally heavy black holes in the merger-driven scenario

In situ extreme mass ratio inspirals via subparsec formation and migration of stars in thin, gravitationally unstable AGN discs

The imprint of gas on gravitational waves from LISA intermediate-mass black hole binaries

Collaborators (11)

Seoyoung Lyla Jung

Ross Church

Emanuele Berti

Enrico Barausse

Johan Richard

Peter Johansson

Tiziana DiMatteo

Michael Tremmel

Arif Babul

Christopher Berry

Jessie Runnoe

Make your next move.

Lucio Mayer

Research Interests

Explore related searches

Contact this professor

Articles (11)

Direct Formation of Massive Black Holes via Dynamical Collapse in Metal-enriched Merging Galaxies at z ∼ 10: Fully Cosmological Simulations

High resolution modelling of [CII], [CI], [OIII], and CO line emission from the interstellar medium and circumgalactic medium of a star-forming galaxy at z ∼ 6.5

Stellar cluster formation in a Milky Way-sized galaxy at z &gt; 4 – II. A hybrid formation scenario for the nuclear star cluster and its connection to the nuclear stellar ring

The minimum measurable eccentricity from gravitational waves of LISA massive black hole binaries

Astrophysics with the Laser Interferometer Space Antenna

Molecular gas cloud properties at z ≃ 1 revealed by the superb angular resolution achieved with ALMA and gravitational lensing

Characterizing fragmentation and sub-Jovian clump properties in magnetized young protoplanetary discs

Cool and gusty, with a chance of rain: dynamics of multiphase CGM around massive galaxies in the Romulus simulations

Direct collapse of exceptionally heavy black holes in the merger-driven scenario

In situ extreme mass ratio inspirals via subparsec formation and migration of stars in thin, gravitationally unstable AGN discs

The imprint of gas on gravitational waves from LISA intermediate-mass black hole binaries

Collaborators (11)

Seoyoung Lyla Jung

Ross Church

Emanuele Berti

Enrico Barausse

Johan Richard

Peter Johansson

Tiziana DiMatteo

Michael Tremmel

Arif Babul

Christopher Berry

Jessie Runnoe

Make your next move.

Stellar cluster formation in a Milky Way-sized galaxy at z > 4 – II. A hybrid formation scenario for the nuclear star cluster and its connection to the nuclear stellar ring