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TASI Lectures on D-Branes
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TASI Lectures on D-Branes
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This is an introduction to the properties of D-branes, topological defects in string theory on which string endpoints can live. D-branes provide a simple description of various nonperturbative objects required by string duality, and give new insight into the quantum mechanics of black holes and the nature of spacetime at the shortest distances. The first two thirds of these lectures closely follow the earlier ITP lectures hep-th/9602052, written with S. Chaudhuri and C. Johnson. The final third includes more extensive applications to string duality.
Forward citations
Cited by 6 Pith papers
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Energy-momentum and dark energy in $\boldsymbol{SU(\infty)}$-QGR quantum gravity
SU(∞)-QGR yields an Einstein-like energy-momentum constraint that includes spin-1 gravitons and treats inflation and accelerating expansion as order parameters tracking the evolution of the universe's quantum states u...
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Self-Gravitating Magnetic Monopoles and Dyons in String-Inspired Models: Structure and Stability
Global monopoles plus dilaton/axion/Born-Infeld yield regular self-gravitating magnetic monopoles and dyons with positive ADM mass, finite energy and linear exterior EM stability.
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Self-Gravitating Magnetic Monopoles and Dyons in String-Inspired Models: Structure and Stability
Classical solutions for self-gravitating monopoles and dyons are found in Einstein-Born-Infeld-dilaton-axion theory and shown to be mechanically and linearly stable with positive ADM mass.
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Non-Invertible Symmetries in Compactified Supergravities
Non-invertible symmetry defects from 11D supergravity descend to Type IIA, splitting the Bianchi sector into invertible H[3] and twisted non-invertible F[4] parts with a BF-type auxiliary sector.
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Energy-momentum and dark energy in $\boldsymbol{SU(\infty)}$-QGR quantum gravity
Invariance of the SU(∞)-QGR action under variation of the parameter-space metric produces an Einstein-like energy-momentum constraint, and Hilbert-space fragmentation is argued to classically appear as inflation, rehe...
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Quantum dissipative effects for a real scalar field coupled to a time-dependent Dirichlet surface in d+1 dimensions
Perturbative expressions up to fourth order for pair creation probability in the dynamical Casimir effect are derived for a scalar field with time-dependent Dirichlet boundary in arbitrary dimensions.
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