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Master theses

For thesis availability contact andrea.maselli@gssi.it

2024-2025

Serafino Bruscia @ University of Pisa
(co-advisor with L. Gualtieri)
Scalar fields and Extreme Mass Ratio Inspirals: where do we look with LISA

2025-2026

Giorgio Monti @ University Of Milano Bicocca
(co-advisor with F. Longo, M. Branchesi & S. Ansoldi)
Eccentricity evolution of Extreme Mass Ratio Inspirals in dense environments

2024

Elisabet Keppler @ Trieste University
(co-advisor with F. Longo, M. Branchesi & S. Ansoldi)
A Multimessenger approach to Tidal Disruption Events

2024

Niccolo' D'onofrio @ Sapienza University of Rome
(co-advisor with S. Barsanti)
Scalar fields and Extreme Mass Ratio Inspirals: where do we look with LISA

2024

Chiara Anselmo @ Sapienza University of Rome
Ringdown tests of General Relativity with future
space gravitational wave detectors

2023 - 2024

Alessandro Agapito @ Sapienza University of Rome

(co-advisor with P. Pani)
GWs inspiral tests of General Relativity in the framework of the Einstein Telescope

2023

Laura Pezzella @ Sapienza University of Rome
Quasi Normal Mode of dirty Black Holes embeeded by dark matter halos

2021 - 2022

Lavinia Paiella @ Sapienza University of Rome
Anatomy of a binary neutron star merger

2021 - 2022

Matteo della Rocca @ Sapienza University of Rome
(co-advisor with L. Gualtieri)
Scalar Flux from an EMRI: inclined circular orbits around Kerr Black holes

2020 - 2021

Viola De Renzis @ Sapienza University of Rome
Distinguishing Black Holes from Exotic Compact objects with gravitational observations

2020 - 2021

Tommaso Garbin @ Sapienza University of Rome
(co-advisor with L. Gualtieri)
Black holes in Einstein-scalar-Gauss-Bonnet gravity:
numerical analysis and analytical approximation for the numerical solutions

2019 - 2020

Irene Fabbri @ Sapienza University of Rome
Constraining the neutron star composition with QPO observations

2020

Susanna Barsanti @ Sapienza University of Rome
Scalar fields around Kerr black holes in extreme mass ratio inspirals

2020

Giulio Danella @ Sapienza University of Rome
Multi-band analysis of the neutron star EoS with future gravitational wave and electromagnetic observatories

2019-2020

Vania Vellucci @ Sapienza University of Rome
(co-advisor with P. Pani & L. Gualtieri)

Black-hole spectroscopy with multiple event:
A data-analysis framework

2017-2018

Goncalo Castro @ Instituto Superior Tecnico [Lisbon]
(co-advisor with V. Cardoso)

Gravitational waves and massive gravitons

2017-2018

Giuseppe Gnocchi @ Sapienza University of Rome

(co-advisor with V. Ferrari)
Prospects for testing General Relativity with multiband gravitational wave detections

PhD theses

2025 - on

 @ GSSI [L'Aquila]

TBA

2024 - on

Manule Gonçalo Oliveira Mariano @ University of Aveiro
(co-advisor with C. Herdeiro)

TBA

2024 - on

Laura Pezzella @ GSSI [L'Aquila]

Ringdown modelling for asymmetric mass ratio mergers 

2023 - on

Sara Gliorio @ GSSI [L'Aquila]

Asymmetric Binaries as fundamental physics probes

​2022 - on

Anjali Kugarajh @ GSSI [L'Aquila]
(co-advisor with S. Matarrese & A. Ricciardone)

Scalar Induced GWs in the multimessenger era: from fundamental physics in the early universe to PBH evolution

​2020 - 2023

Susanna Barsanti @ Sapienza University of Rome
(co-advisor with L. Gualtieri)

Testing fundamental physics with extreme mass ratio binaries

2019 - 2022

Andrea Sabatucci @ Sapienza University of Rome
(co-advisor with O. Benhar)
Nuclear dynamics in modeling Neutron Star structure and its
implications in Gravitational Waves phenomenology

2019 - 2022

Massimo Vaglio @ Sapienza University of Rome
(co-advisor with P. Pani)
Modelling and phenomenology of boson stars as gravitational

sources for future ground and space based interferometers

2018 - 2022

Gabriel Piovano @ Sapienza University of Rome
(co-advisor with P. Pani)
Gravitational waves from exotic compact objects in extreme mass ratio inspirals

2017 - 2020

Margherita Fasano @ Sapienza University of Rome
(co-advisor with V. Ferrari)
Constraining the equation of  state of neutron stars with astrophysical and GWs observations

© 2017 by Andrea Maselli. Created with Wix.com

When you have eliminated the impossible, whatever remains, however improbable,

must be the truth (S.H.)

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