1,959 research outputs found

    On Sasaki-Einstein manifolds in dimension five

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    We prove the existence of Sasaki-Einstein metrics on certain simply connected 5-manifolds where until now existence was unknown. All of these manifolds have non-trivial torsion classes. On several of these we show that there are a countable infinity of deformation classes of Sasaki-Einstein structures.Comment: 18 pages, Exposition was expanded and a reference adde

    Inflation on Fractional Branes: D--Brane Inflation as D--Term Inflation

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    We describe a D--brane inflation model which consists of two fractional D3 branes separated on a transverse T2×K3T^2 \times K3. Inflation arises due to the resolved orbifold singularity of K3K3 which corresponds to an anomalous D--term on the brane. We show that D--brane inflation in the bulk corresponds to D--term inflation on the brane. The inflaton and the trigger field parametrize the interbrane distances on T2T^2 an K3K3 respectively. After inflation the branes reach a supersymmetric configuration in which they are at the origin of T2T^2 but separated along the K3K3 directions.Comment: 15 pages in phyzzx.tex; minor corrections including all factors of 2\pi; v3: more minor correction

    The Volume of some Non-spherical Horizons and the AdS/CFT Correspondence

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    We calculate the volumes of a large class of Einstein manifolds, namely Sasaki-Einstein manifolds which are the bases of Ricci-flat affine cones described by polynomial embedding relations in C^n. These volumes are important because they allow us to extend and test the AdS/CFT correspondence. We use these volumes to extend the central charge calculation of Gubser (1998) to the generalized conifolds of Gubser, Shatashvili, and Nekrasov (1999). These volumes also allow one to quantize precisely the D-brane flux of the AdS supergravity solution. We end by demonstrating a relationship between the volumes of these Einstein spaces and the number of holomorphic polynomials (which correspond to chiral primary operators in the field theory dual) on the corresponding affine cone.Comment: 25 pp, LaTeX, 1 figure, v2: refs adde

    Campus Vol VI N 4

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    Pierson, Pete. Untitled. Cartoon. 2. Hawk, Pete. The First Big Snow . Prose. 3. Smith, Orlo. A Day In the Life of Miss Campus . Picture. 5. Pierson, Pete. Old Seniors never Die... Cartoon. 8. Cole, Sam H. King . Just a Hobo . Prose. 10. Johnson, C. P. Some Sons Of Denison . Prose. 12. Anonymous. Last Will and Testament of the Senior Class . Prose. 14. Kat, Kitty. Untitled. Prose. 16. Spartan. Untitled. Prose. 16. Shaft. Untitled. Prose. 16. Pointer. Untitled. Prose. 16. Tarnation. Untitled. Prose. 17. Sundial. Untitled. Prose. 17. Pup. Untitled. Prose. 17. Aggrevator. Untitled. Prose. 17. Gander, Green. Untitled. Prose. 17. Mis-A-Sip. Untitled. Prose. 17. Lyke. Untitled. Prose. 17

    Cosmic D--term Strings as Wrapped D3 Branes

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    We describe cosmic D--term strings as D3 branes wrapped on a resolved conifold. The matter content that gives rise to D--term strings is shown to describe the world--volume theory of a space--filling D3 brane transverse to the conifold which itself is a wrapped D5 brane. We show that, in this brane theory, the tension of the wrapped D3 brane mathces that of the D--term string. We argue that there is a new type of cosmic string which arises from fractional D1 branes on the world--volume of a fractional D3 brane.Comment: 13 pages in phyzzx.tex; eq. (17) corrected, other minor corrections; v3: more minor correction

    D-brane dynamics near compactified NS5-branes

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    We examine the dynamics of a DpDp-brane in the background of kk coincident, parallel NSNS5-branes which have had one of their common transverse directions compactified. We find that for small energy, bound orbits can exist at sufficiently large distances where there will be no stringy effects. The orbits are dependent upon the energy density, angular momentum and electric field. The analysis breaks down at radial distances comparable with the compactification radius and we must resort to using a modified form of the harmonic function in this region.Comment: Latex, 20 pages, 6 figs, references adde

    Tuning out vibrational levels in molecular electron energy-loss spectra

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    The phenomenon whereby features associated with certain vibrational levels in molecular states of mixed electronic character disappear under specific scattering conditions in electron energy-loss spectra is investigated. In particular, using a combination of experimental measurements and coupled-channel calculations, anomalous vibrational intensities in the mixed valence-Rydberg 1Π u←X1Σg+ transition of N 2 are explained. A single parameter, i.e., the ratio of the generalized electronic transition moments to the diabatic valence and Rydberg components of the mixed states, dependent on the experimental scattering conditions, is found to be essentially capable of describing all observed relative vibrational intensities, including the near disappearance of the b1Π u(v=5) feature for momentum-transfer-squared values K2 ≈ 0.3 a.u. This result highlights the interesting possibility of experimental control of molecular quantum-interference effects in electron energy-loss spectra, something that is not possible in optical spectra

    A new wrinkle on the enhancon

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    We generalize the basic enhancon solution of Johnson, Peet and Polchinski by constructing solutions without spherical symmetry. A careful consideration of boundary conditions at the enhancon surface indicates that the interior of the supergravity solution is still flat space in the general case. We provide some explicit analytic solutions where the enhancon locus is a prolate or oblate sphere.Comment: 19 pages, no figure

    The Enhancon, Black Holes, and the Second Law

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    We revisit the physics of five-dimensional black holes constructed from D5- and D1-branes and momentum modes in type IIB string theory compactified on K3. Since these black holes incorporate D5-branes wrapped on K3, an enhancon locus appears in the spacetime geometry. With a `small' number of D1-branes, the entropy of a black hole is maximised by including precisely half as many D5-branes as there are D1-branes in the black hole. Any attempts to introduce more D5-branes, and so reduce the entropy, are thwarted by the appearance of the enhancon locus above the horizon, which then prevents their approach. The enhancon mechanism thereby acts to uphold the Second Law of Thermodynamics. This result generalises: For each type of bound state object which can be made of both types of brane, we show that a new type of enhancon exists at successively smaller radii in the geometry, again acting to prevent any reduction of the entropy just when needed. We briefly explore the appearance of the enhancon in the black hole interior.Comment: 22 pages, 2 figures, latex, epsfig (v2: Fixed trivial typos.
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