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Identification

Personal identification

Full name
Marco Calza

Citation names

  • Calza, Marco

Author identifiers

Ciência ID
681E-D88D-DD99

Addresses

  • Rua Miguel Torga B12 cv esq, 3030-165, Coimbra, Coimbra, Portugal (Personal)

Knowledge fields

  • Exact Sciences - Physical Sciences - Particles and Fields Physics

Languages

Language Speaking Reading Writing Listening Peer-review
Italian (Mother tongue)
English Advanced (C1) Advanced (C1) Advanced (C1) Proficiency (C2) Advanced (C1)
Spanish; Castilian Advanced (C1) Advanced (C1) Upper intermediate (B2) Advanced (C1) Upper intermediate (B2)
Portuguese Upper intermediate (B2) Upper intermediate (B2) Intermediate (B1) Upper intermediate (B2)
German Elementary (A2) Elementary (A2) Elementary (A2) Elementary (A2) Beginner (A1)
Russian Beginner (A1) Beginner (A1) Beginner (A1) Elementary (A2) Beginner (A1)
Education
Degree Classification
2020/01/01 - 2024/01/01
Ongoing
PhD in Physics (Doutoramento)
Universidade de Coimbra, Portugal
2018/03/20
Concluded
Master degree in Theoretical and Computational Physics (Laurea Magistrale)
Università degli Studi di Trento, Italy
"A special class of vacuum solutions in f(R)-gravity" (THESIS/DISSERTATION)
110/110
2013/03/26
Concluded
Standard Physics bachelor degree (Laurea)
Università degli Studi di Trento, Italy
"Review of the S-factor evaluation in the p-p chain reactions occurring in the Sun" (THESIS/DISSERTATION)
87/110
Affiliation

Others

Category
Host institution
Employer
2019/11/29 - Current PhD student Universidade de Coimbra, Portugal
2018/04/01 - 2018/11/01 Collaborator Università degli Studi di Trento, Italy
Projects

Grant

Designation Funders
2020/01/01 - Current Primordial black hole superradiant instabilities
SFRH/BD/146700/2019
PhD Student Fellow
Universidade de Coimbra, Portugal

Universidade de Coimbra Centro de Física, Portugal
Fundação para a Ciência e a Tecnologia
Ongoing
Outputs

Publications

Journal article
  1. Calza, Marco; João Pedro Trancoso Gomes Rosa. "Evaporating Kerr black holes as probes of new physics". PRL (2023): https://inspirehep.net/literature/2737620.
  2. Calza, Marco; João Pedro Trancoso Gomes Rosa. "Determining the spin of light primordial black holes with Hawking radiation II: high spin regime". JHEP (2023): https://inspirehep.net/literature/2725479.
    Submitted
  3. Calza, Marco; Lorenzo Sebastiani. "A class of static spherically symmetric solutions in f(T)-gravity". Eur.Phys.J.C (2023): https://inspirehep.net/literature/2696232.
    Under revision
  4. Calza, Marco; João Pedro Trancoso Gomes Rosa ; Filipe Serrano. "Primordial black hole superradiance and evaporation in the string axiverse". JHEP (2023):
    Under revision
  5. Calza, Marco; João Pedro Trancoso Gomes Rosa. "Determining the spin of light primordial black holes with Hawking radiation". JHEP 12 (2022) 090 (2022): https://inspirehep.net/literature/2165208.
    Published
  6. Calza, Marco; Lorenzo Sebastiani. "A class of static spherically symmetric solutions in f(Q)-gravity". Eur.Phys.J.C 83 (2023) 3, 247 (2022): https://inspirehep.net/literature/2142650.
    Published
  7. Calza, Marco. "Evaporation of a Kerr-black-bounce by emission of scalar particles". Phys.Rev.D 107 (2023) 4, 044067 (2022): https://inspirehep.net/literature/2120633.
    Published
  8. Calza, Marco; Lorenzo Sebastiani; Alessandro Casalino. "Local solutions of general relativity in the presence of the trace anomaly". Phys.Dark Univ. 37 (2022) 101066 (2022): https://inspirehep.net/literature/2078104.
    Published
  9. Calza, Marco; João Pedro Trancoso Gomes Rosa ; March-Russell, John. "Evaporating primordial black holes, the string axiverse, and hot dark radiation". PRL (2021): https://inspirehep.net/literature/1952327.
    Under revision
  10. Calza, Marco; Lorenzo Sebastiani; Alessandro Casalino; Orlando Luongo. "Kinematic reconstructions of extended theories of gravity at small and intermediate redshifts". Eur.Phys.J.Plus 135 (2020) 1, 1 (2020): https://inspirehep.net/literature/1758491.
    Published
  11. Calza, Marco; Lorenzo Sebastiani; Massimiliano Rinaldi. "A special class of solutions in F(R)-gravity". Eur.Phys.J.C 78 (2018) 3, 178 (2018): https://inspirehep.net/literature/1651797.
    Published
Activities

Oral presentation

Presentation title Event name
Host (Event location)
2023/06/20 Primordial Black Holes as Laboratories for Physics Beyond the Standard Scenarios NEHOP
Napoli
2023/05/03 Primordial Black Holes as Laboratories for Physics Beyond the standard scenarios Dark matter and Stars International Conference, (part of the LOC)
IST, Lisbon
2023/04/04 Primordial Black Holes as laboratories for Physics beyond the standard scenarios IberiCOS 2023
Ponte de Lima
2022/10/18 Primordial Black Holes as laboratories for Physics beyond the standard scenarios invited seminar at CENTRA
IST, Lisbon
2022/10/06 The Quantum and Gravity invited seminar at the 4th I.N.F.N. FLAG meeting
University of Trento
2022/07/26 Evaporating primordial black holes, the string axiverse, and hot dark radiation 27th PASCOS conference
Max Planck Institute, Heidelberg
2022/05/05 PBHs evaporating in the string axiverse IberiCOS2022
University of Barcelona
2021/12/21 Evaporating primordial black holes, the string axiverse, and hot dark radiation XVI Black Holes Workshop
University of Aveiro
2021/12/10 Evaporating primordial black holes, the string axiverse, and hot dark radiation
University of Trento, TIFPA
2021/10/07 Local solutions in f(r)-gravity adopting an ad hoc ansatz Journal Club of Physics Department
University of Coimbra, CFisUC (Coimbra, Portugal)
2021/03/30 Kinematic reconstructions of extended theories of gravity at small and intermediate redshifts. IberiCOS 2021 – 15th Iberian Cosmology Meeting
University of Coimbra (Coimbra, Portugal)
2018/12/18 Invited seminars of TIFPA: Reconstructions of f(R, G) and f(R) scenarios at small redshifts through kinematics Invited seminars of TIFPA
University of Trento (Trento, Italy)

Consulting

Activity description Institution / Organization
2018/04/01 - 2018/11/01 We focused our attention on two classes of extended theories of gravity, f(R) and f(R, G), on three different Hubble rate parametrizations, XCDM, CPL and WP, and the constraint on their parameters set by Planck mission data. By computationally solve the modified Friedmann equations we are able to obtain the shape of the functions f(R) or f(R,G) for each parametrization within the experimental allowed range. Università degli Studi di Trento, Italy