BPS Bound States Of D0-D6 And D0-D8 Systems In A B-Field
By E. Witten. 2000
152 citations recorded by the source corpus.
The D0-D6 system, which is not supersymmetric in the absence of a Neveu-Schwarz B-field, becomes supersymmetric if a suitable constant B-field is turned on. On one side of the supersymmetric locus, this system has a BPS bound state, and on the other side it does not. After compactification on Bbb T6, this gives a simple example in which the number of 1/8 BPS states jumps as the moduli of the compactification are changed. The D0-D8 system in a B-field has two different supersymmetric loci, only one of which is continuously connected to the familiar supersymmetric D0-D8 system without a B-field. In a certain range, the D0-D8 system also has a BPS bound state. In the limit in which the B-field goes to infinity, supersymmetric D0-D6 and D0-D8 systems and their bound states can be studied using non-commutative Yang-Mills theory.
Subfields: Geometry and Topology, Nuclear and High Energy Physics, Statistical and Nonlinear Physics
View Paper: https://www.semanticscholar.org/paper/548be41959c6fc09e0d8b162ea5a96f6727b6a9e
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In Geometry and Topology
- Ashoke Sen
- Ralph Blumenhagen
- B. Pioline
- D. Lust
- Gary Shiu
- F. Marchesano
- G. Moore
- Vijay Balasubramanian
In Nuclear and High Energy Physics
In Statistical and Nonlinear Physics
Citations in the corpus
- SUSY Quivers, Intersecting Branes and the Modest Hierarchy Problem (2002, background): “For a T-dual description of this phenomenon see [38].”
- Supersymmetric Intersecting Branes on the Type IIA T6/Bbb Z4 Orientifold (2002, background): “When the two D-branes only preserve N = 1 supersymmetry and support a massless chiral supermultiplet Φ on the intersection [60,61], the situation gets a little bit more involved.”
- Four dimensional black hole microstates: from D-branes to spacetime foam (2006, methodology): “The SU(Np) equations take the form, written using the generators t α (α = 1 . . . N 2 p − 1) [ 57 ]:”
- Split states, entropy enigmas, holes and halos (2007, background): “However this can change when the B-field is sufficiently large [83, 84, 85], or equivalently when a sufficiently large U(1) flux is turned on on the D6.”
- Moduli stabilization in chiral type IIB orientifold models with fluxes (2003, background): “where ρ(M) denotes the rotation matrix by the angles ψ a in the spinor representation [58,59].”
- Wall crossing from Boltzmann black hole halos (2010, background): “It is known that for infinite volume and small B-field, a configuration of r ≥ 1 D6-branes and n ≥ 1 D0 branes do not form any bound state [52].”
- Getting just the standard model at intersecting branes (2001, background): “As we have mentioned above other properties as the presence or absence of tachyons, the supersymmetries preserved [25, 26, 27] by the system of D-branes, the massive spectrum, etc.”
- Precision Counting of Small Black Holes (2005, background): “At finite R and sufficiently large ~q or B-field, BPS states with nonzero q1 may appear [90–93].”
- Building MSSM flux vacua (2004, background): “, is no longer a ‘factorisable’ D-brane but a BPS bound state of two of them [63].”