Absorption Cross Section of Scalar Field in Supergravity Background

TL;DR

This paper calculates the absorption cross section of a massless scalar field by a D3 brane in supergravity, using modified Mathieu functions and low energy expansions to derive analytical results.

Contribution

It introduces a method to compute the scalar absorption rate in supergravity backgrounds using modified Mathieu functions and explores their relation to Dougall coefficients.

Findings

Analytical expressions for absorption cross section obtained.

Connection between Mathieu functions and Dougall coefficients established.

Leading order and logarithmic contributions explicitly derived.

Abstract

It has recently been shown that the equation of motion of a massless scalar field in the background of some specific p branes can be reduced to a modified Mathieu equation. In the following the absorption rate of the scalar by a D3 brane in ten dimensions is calculated in terms of modified Mathieu functions of the first kind, using standard Mathieu coefficients. The relation of the latter to Dougall coefficients (used by others) is investigated. The S-matrix obtained in terms of modified Mathieu functions of the first kind is easily evaluated if known rapidly convergent low energy expansions of these in terms of products of Bessel functions are used. Leading order terms, including the interesting logarithmic contributions, can be obtained analytically.