Quasinormal modes of near extremal black branes
By A. Starinets. 2002
216 citations recorded by the source corpus.
We investigate a method to evaluate quasinormal modes of D3-brane black holes by wave interpretation of fields on a D3-brane based on Feynman’s spacetime approach. We perturbatively solve the wave equation which describes propagation of a dilaton wave in a bulk space and its interaction with the D3-brane. The condition obtained for the quasinormal modes is qualitatively equivalent to that evaluated in the usual scattering of the dilaton in the black three-brane spacetime in the corresponding supergravity description.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/ae874b27d8c77e289c5fc309fde9955c587725fa
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Citations in the corpus
- An Analytical computation of asymptotic Schwarzschild quasinormal frequencies (2002, background): “In [29], the continued fractions play an important role.”
- Holographic Quantum Matter (2016, methodology): “These include the use of truncated high order power series expansions [385] and a method using continued fractions [686].”
- The complex life of hydrodynamic modes (2019, background): “The equations of motion describing fluctuations of the gravitational background dual to finite-temperature N = 4 SYM theory are of the Heun type [55], and the exact analytic solution for the spectral curve similar to eq.”
- Quarks in an External Electric Field in Finite Temperature Large N Gauge Theory (2007, background): “The equation of motion for this ansatz has one intriguing difference from similar fluctuation calculations done elsewhere [19, 20, 21, 16]: Because of the presence of the current, there exists a term proportional to ∂t̃Φ × ∂ũΦ.”
- Quasinormal modes and holography (2005, methodology): “Quasinormal spectrum of fluctuations obeying incoming wave boundary condition at the horizon and Dirichlet condition Z3(u=0) = 0 at the boundary was numerically computed in [11, 26].”
- AdS / CFT correspondence, quasinormal modes, and thermal correlators in N=4 SYM (2003, methodology): “These checks give us confidence that the values of quasinormal frequencies reported in [25] and in this paper are determined correctly(7).”
- Numerical solution of gravitational dynamics in asymptotically anti-de Sitter spacetimes (2013, background): “departures from equilibrium [13, 14], specifically those of ` = 2 metric perturbations whose linearized dynamics around the AdS-Schwarzschild black brane solution coincides with fluctuations of a minimally coupled scalar field.”
- Gauge-gravity duality and thermalization of a boost-invariant perfect fluid (2006, background): “ons linearized around the background geometry. In particular the calculation of the QNM’s corresponding to a scalar excitation canonically coupled to the metric in the gravitational dual configuration [4, 5, 6, 7] may give an evaluation of the thermalization time of the dual gauge field-theoretic stro”
- Holographic meson melting (2006, unknown): “Contents”