Zobrazeno 1 - 10
of 14
pro vyhledávání: '"Michele, Lenzi"'
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 79, Iss 11, Pp 1-18 (2019)
Abstract We study equilibrium configurations of a homogenous ball of matter in a bootstrapped description of gravity which includes a gravitational self-interaction term beyond the Newtonian coupling. Both matter density and pressure are accounted fo
Externí odkaz:
https://doaj.org/article/193caec14d234c618364e807c11501db
Autor:
Michele Lenzi, Carlos F. Sopuerta
Publikováno v:
Physical Review D. 107
It has recently been shown that the dynamics of perturbed non-rotating black holes (BHs) admits an infinite number of symmetries that are generated by the flow of the Korteweg-de Vries (KdV) equation. These symmetries lead to an infinite number of co
Autor:
Carlos F. Sopuerta, Michele Lenzi
The dynamics of perturbed non-rotating black holes (BHs) can be described in terms of master equations of the wave type with a potential. In the frequency domain, the master equations become time-independent Schr\"odinger equations with no discrete s
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2f011285508eaf7a321ca488d43064ce
Autor:
Carlos F. Sopuerta, Michele Lenzi
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
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We determine and characterize the full space of master equations describing the dynamics of perturbed Schwarzschild black holes and show that all of them are connected via Darboux transformations. This reveals the presence of a hidden symmetry, Darbo
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::461acb715a0bb1f76f596feda6a2cedb
http://hdl.handle.net/10261/263029
http://hdl.handle.net/10261/263029
Autor:
Michele Lenzi, Carlos F. Sopuerta
Publikováno v:
Digital.CSIC. Repositorio Institucional del CSIC
instname
instname
Perturbation theory of vacuum spherically-symmetric spacetimes is a crucial tool to understand the dynamics of black hole perturbations. Spherical symmetry allows for an expansion of the perturbations in scalar, vector, and tensor harmonics. The resu
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f19ec0ec4afd95b91df70275f9a01d00
We analyse the classical configurations of a bootstrapped Newtonian potential generated by homogeneous spherically symmetric sources in terms of a quantum coherent state. We first compute how the mass and mean wavelength of these solutions scale in t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e2ab8c57ce7215f681f958d392f9b44a
Publikováno v:
European Physical Journal C: Particles and Fields, Vol 79, Iss 11, Pp 1-18 (2019)
European Physical Journal
European Physical Journal
We study equilibrium configurations of a homogenous ball of matter in a bootstrapped description of gravity which includes a gravitational self-interaction term beyond the Newtonian coupling. Both matter density and pressure are accounted for as sour
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::5b952fd90380fc335b7753b67eae196b
A non-linear equation obtained by adding gravitational self-interaction terms to the Poisson equation for Newtonian gravity is here employed in order to analyse a static spherically sym- metric homogeneous compact source of given proper mass and radi
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::af816881657e98f6bc6a81c22c944693
http://hdl.handle.net/11585/649932
http://hdl.handle.net/11585/649932
We provide a (simplified) quantum description of primordial black holes at the time of their formation. Specifically, we employ the horizon quantum mechanics to compute the probability of black hole formation starting from a simple quantum mechanical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::05910766934633d6b4cc782ece32fb04
Publikováno v:
Physical Review D. 96
We study an effective quantum description of the static gravitational potential for spherically symmetric systems up to the first post-Newtonian order. We start by obtaining a Lagrangian for the gravitational potential coupled to a static matter sour