2 research outputs found
The Eikonal Approximation and the Gravitational Dynamics of Binary Systems
PhD ThesisIn this thesis we study the conservative gravitational dynamics of binary systems using
the eikonal approximation; allowing us to use scattering amplitude techniques to
calculate dynamical quantities in classical gravity. This has implications for the study
of binary black hole systems and their resulting gravitational waves.
In the rst three chapters we introduce some of the basic concepts and results that
we will use in the rest of the thesis. In the rst chapter an overview of the topic is
discussed and the academic context is introduced. The second chapter includes a basic
discussion of gravity as a quantum eld theory, the post-Newtonian (PN) and post-
Minkowskian (PM) expansions and the eikonal approximation. In the third chapter we
consider various Feynman integrals that are used extensively in subsequent chapters.
Speci cally, we give a recipe for expanding the relevant integrands in a so-called high
energy expansion and then calculating the resulting integrals.
The fourth chapter involves the study of massless states scattering o of a stack of
Dp-branes in N = 8 supergravity. The setup we consider provides an ideal scenario to
study inelastic contributions to the scattering process and their impact on the formulation
of the eikonal approximation. These results will give us a better understanding
of the eikonal approximation presented in the second chapter. The fth chapter involves
studying the eikonal and corresponding dynamical quantities in a Kaluza-Klein
theory of gravity providing further interesting insight into the eikonal approximation
and allowing us to compare with various known results.
The sixth and seventh chapter apply the concepts developed in this thesis to the
problem of binary Schwarzschild black holes in D spacetime dimensions. This allows us
to apply the framework exposed in previous chapters to a physically realistic scenario
giving us a better understanding of how to extract the relevant dynamical information
from scattering amplitudes. The results derived in chapter six also have an impact on
our understanding at higher orders in the PM expansion beyond the ones considered
in this text. In the seventh chapter we present the Hamiltonian for a system of binary
Schwarzschild black holes and show how to extract the Hamiltonian from other
dynamical quantities calculated using the eikonal.
In the last chapter we provide some concluding remarks and a brief outlook
The subleading eikonal in supergravity theories
In this paper we study the subleading contributions to eikonal scattering in
(super)gravity theories with particular emphasis on the role of both elastic
and inelastic scattering processes. For concreteness we focus on the scattering
of various massless particles off a stack of D-branes in type II
supergravity in the limit of large impact parameter . We analyse the
relevant field theory Feynman diagrams which naturally give rise to both
elastic and inelastic processes. We show that in the case analysed the leading
and subleading eikonal only depend on elastic processes, while inelastic
processes are captured by a pre-factor multiplying the exponentiated leading
and subleading eikonal phase. In addition to the traditional Feynman diagram
computations mentioned above, we also present a novel method for computing the
amplitudes contributing to the leading and subleading eikonal phases, which, in
the large limit, only involves knowledge of the onshell three and
four-point vertices. The two methods are shown to give the same results.
Furthermore we derive these results in yet another way, by computing various
one-point amplitudes which allow us to extract the classical solution of the
gravitational back reaction of the target D-branes. Finally we show how our
expressions for the leading and subleading eikonal agree with the calculation
of the metric and corresponding deflection angle for massless states moving
along geodesics in the relevant curved geometry.Comment: 40 pages, 5 figure