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Paolo Pani

Researcher at Sapienza University of Rome

Publications -  337
Citations -  19007

Paolo Pani is an academic researcher from Sapienza University of Rome. The author has contributed to research in topics: Black hole & General relativity. The author has an hindex of 66, co-authored 302 publications receiving 14022 citations. Previous affiliations of Paolo Pani include Harvard University & Federal University of Pará.

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Instability of hyper-compact Kerr-like objects

TL;DR: In this article, a detailed investigation of wormholes and superspinars is presented, using plausible models and mirror boundary conditions at the surface, showing that these objects are unstable with very short instability timescales.
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Exotic compact objects with soft hair

TL;DR: In this article, the Hartle-Thorne formalism is extended to include deformations induced by multipole moments higher than the spin, thus constructing the most general, axisymmetric quasi-Schwarzschild solution to Einstein's vacuum equations.
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Probing the Nature of Black Holes: Deep in the mHz Gravitational-Wave Sky

TL;DR: Precision tests of black hole spacetimes with mHz-band gravitational-wave detectors will probe general relativity and fundamental physics in previously inaccessible regimes, and allow us to address some of these fundamental issues in the current understanding of nature.
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Enhancement of cholesterol synthesis and pentose phosphate pathway activity in proliferating hepatocyte nodules

TL;DR: Hepatocyte nodules showed a striking increase in their capacity for synthesizing cholesterol, in comparison to surrounding and control tissues, and an enhancement in the activity of the pentose phosphate pathway, as indicated by increased activity of glucose-6-ph phosphate dehydrogenase and of 6-phosphogluconate dehydrogensase, and a concomitant decrease of glucose -6- phosphatase.
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Partially massless gravitons do not destroy general relativity black holes

TL;DR: In this article, it was shown that general relativity black holes are stable in this limit and that the spectrum of massive gravitational perturbations is isospectral, where the mass of the graviton is fixed in terms of the cosmological constant.