Quantum Tunneling Beyond Semiclassical Approximation

Hawking radiation as tunneling by Hamilton-Jacobi method beyond semiclassical approximation is analysed. We compute all quantum corrections in the single particle action revealing that these are proportional to the usual semiclassical contribution. We show that a simple choice of the proportionality constants reproduces the one loop back reaction effect in the spacetime, found by conformal field theory methods, which modifies the Hawking temperature of the black hole. Using the law of black hole mechanics we give the corrections to the Bekenstein-Hawking area law following from the modified Hawking temperature. Some examples are explicitly worked out.Comment: LaTex, 17 pages, no figures, Important changes in section 3, new references added, version to appear in JHE

The Interaction of Carbon Dioxide and Hydrogen on Solid Surfaces

Abstract Not Provided

Connecting anomaly and tunneling methods for Hawking effect through chirality

The role of chirality is discussed in unifying the anomaly and the tunneling formalisms for deriving the Hawking effect. Using the chirality condition and starting from the familiar form of the trace anomaly, the chiral (gravitational) anomaly, manifested as a nonconservation of the stress tensor, near the horizon of a black hole, is derived. Solution of this equation yields the stress tensor whose asymptotic infinity limit gives the Hawking flux. Finally, use of the same chirality condition in the tunneling formalism gives the Hawking temperature that is compatible with the flux obtained by anomaly method.Comment: LaTex, 8 pages, no figures, reformulation of tunneling mechanism, to appear in Phys. Rev.

Quantum tunneling and black hole spectroscopy

The entropy-area spectrum of a black hole has been a long-standing and unsolved problem. Based on a recent methodology introduced by two of the authors, for the black hole radiation (Hawking effect) as tunneling effect, we obtain the entropy spectrum of a black hole. In Einstein's gravity, we show that both entropy and area spectrum are evenly spaced. But in more general theories (like Einstein-Gauss-Bonnet gravity), although the entropy spectrum is equispaced, the corresponding area spectrum is not.Comment: 10 pages, LaTeX, no figures; v2: 9 pages, now, title changed, minor changes to match published version in Phys. Lett.

A Note on the Lower Bound of Black Hole Area Change in Tunneling Formalism

In the framework of tunneling mechanism and employing Bekenstein's general expression for the variation of the black hole area, we determine the area quantum up to a constant. Depending on the value of this constant one can get either Bekenstein's lower bound or Hod's one for the change in the black hole area.Comment: 4 pages, LaTeX, no figures; v2: 6 pages, clarifications and references added, no changes in physics and results, to appear in EP