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Annual Report 2005 - Fields Institute - University of Toronto

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Participants<br />

Mariana Grana (Ecole Normale Supérieure-Paris)<br />

Hitchin functionals in supergravity<br />

Sergei Gukov (Harvard)<br />

Heterotic moduli stabilization with fractional Chern-Simons<br />

invariants<br />

Ruben Minasian (École Polytechnique)<br />

On mirror symmetry with fluxes and branes<br />

Michael Schulz (Caltech)<br />

Mapping flux to geometry<br />

Gary Shiu (Wisconsin & Perimeter Inst.)<br />

Building chiral flux vacua<br />

Alessandro Tomasiello (Stanford)<br />

Towards generalized complex mirror symmetry<br />

Workshop on String Phenomenology<br />

March 28–April 1, <strong>2005</strong><br />

Held at Perimeter <strong>Institute</strong><br />

Organizers: Jan Louis (Hamburg), Robert Myers (Perimeter)<br />

and Gary Shiu (Wisconsin)<br />

This workshop was mounted jointly by the <strong>Fields</strong> <strong>Institute</strong><br />

and Perimeter <strong>Institute</strong> (in Waterloo). It ran at Perimeter,<br />

coming immediately after the closely related <strong>Fields</strong> workshop<br />

on N=1 Compactifications.<br />

String phenomenology has emerged as a research area at the<br />

rich interdisciplinary boundaries <strong>of</strong> string theory, particle<br />

physics, and cosmology. Although research in string phenomenology<br />

is motivated by physical questions, progress<br />

T h e m a t i c P r o g r a m s<br />

<strong>of</strong>ten comes from connections to more formal and mathematical<br />

aspects <strong>of</strong> string theory. This meeting brought<br />

together an international array <strong>of</strong> over 80 researchers from<br />

the United States, France, Spain, Italy, Germany, England,<br />

Japan and, <strong>of</strong> course, Canada, representing interest in all<br />

aspects <strong>of</strong> this field.<br />

Traditionally string phenomenology has focused on the<br />

issue <strong>of</strong> how the physics <strong>of</strong> elementary particles and forces,<br />

as observed in laboratory experiments, can arise from<br />

string theory. Hence the workshop included a number <strong>of</strong><br />

technical talks assessing various proposals for how various<br />

features <strong>of</strong> the so-called Standard Model might arise in<br />

stringy constructions. In this domain, an extremely important<br />

question is how to recognize various signatures in the<br />

new collider experiments which will be run over the next<br />

few years. In particular, the largest such experiment, called<br />

the “Large Hadron Collider” (LHC), will turn on at the<br />

CERN laboratory in Geneva in 2007. Hence the workshop<br />

organizers called upon Gordy Kane (Michigan) to organize<br />

an “LHC Stretching Exercise”, in which he presented<br />

mock experimental data and challenged participants to<br />

determine the underlying stringy model. It is expected that<br />

such warm-up exercises will become a common feature for<br />

string phenomenology meetings as 2007 approaches.<br />

A particularly exciting and active area <strong>of</strong> string phenomenology<br />

in recent years has been addressing questions at the<br />

interface between cosmology and string theory. Cosmology<br />

has entered an extraordinary era where experimental data<br />

has fixed the basic parameters describing the evolution <strong>of</strong><br />

the universe and points towards the existence <strong>of</strong> an inflationary<br />

phase <strong>of</strong> accelerated expansion in its very earliest<br />

stages. At the same time, string theory has seen remarkable<br />

progress in the past few years in moving from a stage where<br />

people questioned the compatibility <strong>of</strong> string theory with<br />

cosmological observations to one where people regularly<br />

propose detailed models and compare their predictions<br />

with the experimental data. Hence a good proportion <strong>of</strong> the<br />

workshop was devoted to string cosmology with a variety<br />

<strong>of</strong> talks on topics such as cosmic superstrings, string signatures<br />

in the cosmic microwave background and even the<br />

wave-function <strong>of</strong> the universe.<br />

One <strong>of</strong> the most interesting aspects <strong>of</strong> superstring<br />

cosmology has been the recent realization that rather<br />

than “providing a unique answer”, string theory may<br />

consistently describe a huge number <strong>of</strong> different kinds<br />

<strong>of</strong> universes. This broad array <strong>of</strong> different possible solutions<br />

is known as “the string theory landscape”. At the<br />

<strong>Fields</strong> <strong>Institute</strong> <strong>2005</strong> ANNUAL REPORT 26

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