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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Superradiance in spinning conducting stars |
Cardoso, Pani, Yu [arXiv:1704.06151] |
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Tidall-deformed, spinning geometry |
Pani, Gualtieri, Maselli, Ferrari [arXiv:1503.07365] |
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Advanced Methods in BH Perturbation Theory @ NRHEP2 Spring School |
Pani, Lecture Notes [arXiv:1305.6759] |
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Computation of QNMs with direct integration [Chandra & Detweiler PRLSA344, 441 (1975)] |
Molina, Pani et al PRD81, 124021 (2010) [arXiv:1004.4007]. |
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Proca fields on a Kerr BH Slow-rotation approximation |
Pani,+ PRL (2012), [arXiv:1209.0465]. Pani,+ PRD (2012), [arXiv:1209.0773] |
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QNMs of Kerr-Newman BHs Slow-rotation approximation |
Pani, Berti & Gualtieri [arXiv:1304.1160] |
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Massive spin-2 fluctuations Slow-rotation approximation |
Brito, Cardoso & Pani [arXiv:1304.6725]. |
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Massive scalar unstable modes of a Kerr black hole through Leaver's continued fraction method. |
Brito, Cardoso & Pani [arXiv:1501.06570] |
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Amplification of massless fields in the Kerr background |
Brito, Cardoso & Pani [arXiv:1501.06570] |
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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] |
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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] |
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Hairy BHs in massive gravity |
Brito, Cardoso & Pani [arXiv:1309.0818] |
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Neutron stars in scalar-tensor gravity Slow-rotation approximation |
Pani & Berti [arXiv:1405.4547] |
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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] |
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Black-hole metric in Dynamical Chern-Simons gravity up to fifth order in the spin |
Maselli, Pani, Cotesta, Gualtieri, Ferrari, Stella [arXiv:1703.01472] |
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Lectures on Testing Gravity @ SIGRAV winter school 2020 (Vietri, IT) |
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