Giovanni Camelio

About me

I am a software developer and previously a researcher in astrophysics.

The main topic of my research are neutron stars, studied through numerical and analytical methods.

I am currently based in Gothenburg, Sweden.

Curriculum Vitae

• 2022-now: software developer
• 2020-2022: postdoc at CAMK-PAN Warsaw
• 2017-2020: postdoc at Stockholm University
• 2013-2017: PhD in Physics at University of Rome "Sapienza"
• 2007-2013: Bachelor & Master in Physics at University of Milan

Publications

scientific codes

• Camelio (2022). ASWNS. zenodo. DOI:10.5281/zenodo.6594069.
  nonbarotropic, hot, and differentially rotating neutron stars.
  also on github.
• Camelio (2022). hydro-bulk-1D. zenodo. DOI:10.5281/zenodo.6478022.
  1D general relativistic hydrodynamics with bulk viscosity.
  also on github.

peer-reviewed articles

• Camelio, Gavassino, Antonelli, Bernuzzi & Haskell (2023).
  Simulating bulk viscosity in neutron stars. I. Formalism.
  PRD 107:103031. arXiv:2204.11809.
• Camelio, Gavassino, Antonelli, Bernuzzi & Haskell (2023).
  Simulating bulk viscosity in neutron stars. II. Evolution in spherical symmetry.
  PRD 107:103032. arXiv:2204.11810. code on zenodo and github.
• Benhar, Lovato & Camelio (2022).
  Modeling Neutron Star Matter in the Age of Multimessenger Astrophysics.
  ApJ 939:52. arXiv:2205.11183.
• Camelio, Dietrich, Rosswog & Haskell (2021).
  Axisymmetric models for neutron star merger remnants with realistic thermal and rotational profiles.
  PRD 103:063014. arXiv:2011.10557. dataset on zenodo.
  code based on this paper on zenodo and github.
• Camelio, Dietrich, Marques & Rosswog (2019).
  Rotating neutron stars with nonbarotropic thermal profile.
  PRD 100:123001. arXiv:1908.11258.
  code based on this paper on zenodo and github.
• Camelio, Dietrich & Rosswog (2018).
  Disc formation in the collapse of supramassive neutron stars.
  MNRAS 480:5272. arXiv:1806.07775.
  code based on this paper on zenodo and github.
• Camelio, Lovato, Gualtieri, Benhar, Pons & Ferrari (2017).
  Evolution of a proto-neutron star with a nuclear many-body equation of state: Neutrino luminosity and gravitational wave frequencies.
  PRD 96:043015. arXiv:1704.01923.
• Camelio, Gualtieri, Pons & Ferrari (2016).
  Spin evolution of a proto-neutron star.
  PRD 94:024008. arXiv:1601.02945.
• Camelio & Lombardi (2015).
  On the origin of intrinsic alignment in cosmic shear measurements: an analytic argument.
  A&A 575:A113. arXiv:1501.03014.
• Camelio, Carati & Galgani (2012).
  Classical helium atom with radiation reaction.
  CHAOS 22:023111. arXiv:1111.5794.

thesis

• Camelio (2017). Early evolution of newly born proto-neutron stars.
  Doctoral dissertation. University of Rome "Sapienza". arXiv:1801.01350.

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