Paolo Pani
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All software was migrated to our group's GIT repository. You can find useful material for research or even public presentations.  All original codes, notebooks, and data may be used under the terms of the Creative Commons Attribution 3.0 licence. Any further distribution of this work must maintain attribution to the author(s) and cite the relevant references. If you have any question, just drop me a line.
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Reference
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Superradiance in spinning conducting stars
Cardoso, Pani, Yu
[arXiv:1704.06151]
Notebook
​Tidall-deformed, spinning geometry
​Pani, Gualtieri, Maselli, Ferrari
[arXiv:1503.07365]
archive
Advanced Methods in BH Perturbation Theory
@ NRHEP2 Spring School
​Pani, Lecture Notes
[arXiv:1305.6759]
archive
Computation of QNMs with direct integration
[​Chandra & Detweiler PRLSA344, 441 (1975)]
Molina, Pani et al
PRD81, 124021 (2010) 
[arXiv:1004.4007].
Notebook 
​Proca fields on a Kerr BH
Slow-rotation approximation
​Pani,+ PRL (2012), [arXiv:1209.0465].
Pani,+ PRD (2012), [arXiv:1209.0773]
Notebook #1
Notebook #2
​QNMs of Kerr-Newman BHs
Slow-rotation approximation
​Pani, Berti & Gualtieri
[arXiv:1304.1160]
​Notebook
​Massive spin-2 fluctuations
Slow-rotation approximation
Brito, Cardoso & Pani
[arXiv:1304.6725].
​Notebook
Massive scalar unstable
modes of a Kerr black hole through Leaver's continued fraction method.
Brito, Cardoso & Pani
[arXiv:1501.06570]
​Notebook
​Amplification of massless fields
in the Kerr background
​Brito, Cardoso & Pani
[arXiv:1501.06570]
​archive
​Amplification of the superradiant
scattering of a charged wave off a spherically-symmetric or a slowly-rotating black hole with generic metric.
Brito, Cardoso & Pani
[arXiv:1501.06570]
​Notebook
Amplification of the superradiant
scattering of a neutral bosonic wave 
of generic spin off a Kerr BH, obtained
by solving the Teukolsky equations.
Brito, Cardoso & Pani
[arXiv:1501.06570]
​Notebook
Hairy BHs in massive gravity
Brito, Cardoso & Pani
[arXiv:1309.0818]
​Notebook #1
Notebook #2
​Neutron stars in scalar-tensor gravity
Slow-rotation approximation
​Pani & Berti
[arXiv:1405.4547]
​​Notebook
Hartle-Thorne.nb
​​(i) computes and solves Einstein's equations 
for a rotating self-gravitating perfect-fluid 
to second order in the spin. 
(ii) derives in detail the procedure 
to separate the Klein-Gordon equation 
in this background.
Brito, Cardoso & Pani
[arXiv:1501.06570]
​Notebook
Black-hole metric in Dynamical Chern-Simons gravity up to fifth order in the spin
Maselli, Pani, Cotesta, Gualtieri, Ferrari, Stella
​[arXiv:1703.01472]
​Notebook
Lectures on Testing Gravity
@ SIGRAV winter school 2020 (Vietri, IT)
Value
​archive

Other resources:

​GRIT resources
 (maintained by Vitor Cardoso)

OleMiss resources (maintained by Emanuele Berti)

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  • Home
  • News
  • Bio
  • Research
    • Notebooks
    • Workshops & Conferences
  • Teaching
    • Lectures @ Sapienza
    • Master and PhD Theses
    • Schools
  • Press & Outreach
  • Contact