On some results about the variational theory of complex rays used close to the high frequency regime

2016 ◽  
Vol 124 ◽  
pp. 30-43 ◽  
Author(s):  
Hervé Riou
2021 ◽  
Vol 98 ◽  
pp. 239-253
Author(s):  
Niall Bootland ◽  
Victorita Dolean ◽  
Pierre Jolivet ◽  
Pierre-Henri Tournier

2012 ◽  
pp. 334-374
Author(s):  
C. J. Joachain ◽  
N. J. Kylstra ◽  
R. M. Potvliege

2009 ◽  
Vol 06 (02) ◽  
pp. 343-360 ◽  
Author(s):  
AHMED JELLAL ◽  
RACHID HOUÇA

We propose an approach based on a generalized quantum mechanics to deal with the basic features of the intrinsic spin Hall effect. This can be done by considering two decoupled harmonic oscillators on the noncommutative plane and evaluating the spin Hall conductivity. Focusing on the high frequency regime, we obtain a diagonalized Hamiltonian. After getting the corresponding spectrum, we show that there is a Hall conductivity without an external magnetic field, which is noncommutativity parameter θ-dependent. This allows us to make contact with the spin Hall effect and also give different interpretations. Fixing θ, one can recover three different approaches dealing with the phenomenon.


Universe ◽  
2018 ◽  
Vol 4 (9) ◽  
pp. 93 ◽  
Author(s):  
Finnian Gray ◽  
Matt Visser

In earlier work concerning the sparsity of the Hawking flux, we found it necessary to re-examine what is known regarding the greybody factors of black holes, with a view to extending and expanding on some old results from the 1970s. Focusing specifically on Schwarzschild black holes, we have re-calculated and re-assessed the greybody factors using a path-ordered-exponential approach, a technique which has the virtue of providing a pedagogically useful semi-explicit formula for the relevant Bogoliubov coefficients. These path-ordered-exponentials, being based on a variant of the “transfer matrix” formalism, are closely related to so-called “product integrals”, leading to quite straightforward and direct numerical evaluation, while side-stepping any need for numerically solving the relevant ordinary differential equations. Furthermore, while considerable analytic information is already available regarding both the high-frequency and low-frequency asymptotics of these greybody factors, numerical approaches seem better adapted to finding suitable “global models” for these greybody factors in the intermediate frequency regime, where most of the Hawking flux is actually concentrated. Working in a more general context, these path-ordered-exponential techniques are also likely to be of interest for generic barrier-penetration problems.


2013 ◽  
Vol 127 (4) ◽  
pp. 641-683
Author(s):  
Youness Noumir ◽  
François Dubois ◽  
Olivier Lafitte

2017 ◽  
Vol 59 (6) ◽  
pp. 909-918 ◽  
Author(s):  
Hao Li ◽  
Pierre Ladeveze ◽  
Hervé Riou

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