DiscoverC05005 - Thematic Program on The Geometry of String Theory 2004 - 2005: String Phenomenology
C05005 - Thematic Program on The Geometry of String Theory 2004 - 2005: String Phenomenology
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C05005 - Thematic Program on The Geometry of String Theory 2004 - 2005: String Phenomenology

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String phenomenology is an emerging research area in the rich interdisciplinary boundaries of string theory, particle physics, and cosmology. Although research in string phenomenology is motivated by physical questions, progress often comes from connections to more formal and mathematical aspects of string theory. These connections include:

*How does the Standard Model of particle physics arise from string theory?: Calabi–Yau manifolds, G2 manifolds, brane worlds, orientfolds, intersecting D–branes, warped compactifications, flux compactifications

*Can string theory provide a realistic cosmology?: brane cosmology, tachyon condensation, string field theory, decay of unstable branes, thermodynamics of strings and branes, Hagedorn temperature, models of inflation, time–dependent backgrounds

*What are the experimental signatures of string theory?: brane worlds, extra dimensions, signatures of short distance physics from early universe cosmology, cosmic strings

It is truly an exciting time in cosmology where experiments have produced and are continuing to yield an abundance of precision data. Similarly, collider experiments at Fermilab, SLAC and CERN, as well as precision low–energy experiments, have the potential to make remarkable new discoveries in particle physics in the next five years. Hence string phenomenology is both a timely and exciting topic of a workshop in 2005.
33 Episodes
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LHC Signal (??)

LHC Signal (??)

2005-04-01--:--

Black Box

Black Box

2005-04-0128:49

Shock Therapy

Shock Therapy

2005-04-01--:--

Landscape Attractors

Landscape Attractors

2005-03-3125:41

Landscape Architecture

Landscape Architecture

2005-03-31--:--

LHC

LHC

2005-03-30--:--

By creating a location that is essentially free from radioactive background, sensitive measurements can be performed to test fundamental laws of physics with neutrinos from the Sun, Dark Matter particles left over from the Big Bang and rare forms of radioactivity. The Sudbury Neutrino Observatory (SNO) is a neutrino detector containing 1,000 tonnes of heavy water and situated 2,000 meters underground in INCO's Creighton Mine near Sudbury, Ontario. SNO has observed neutrinos from the core of Sun and has found clear evidence for neutrino flavor change. This requires modification of the Standard Model for elementary particles and confirms solar model calculations with great accuracy. The underground facility is now being expanded to create a long-term international facility for underground science (SNOLAB), where measurements of Dark Matter, Double Beta Decay and Solar Neutrinos will be performed with the lowest radioactive background available anywhere. The results for SNO and the future scientific program for SNO and SNOLAB will be described.
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