English

On type 0 string theory in solvable RR backgrounds

High Energy Physics - Theory 2022-04-13 v3

Abstract

Motivated by a possibility of solving non-supersymmetric type 0 string theory in AdS5×S5AdS_5 \times S^5 background using integrability, we revisit the construction of type 0 string spectrum in some solvable examples of backgrounds with RR fluxes that are common to type IIB and type 0B theories. The presence of RR fluxes requires the use of a Green-Schwarz description for type 0 string theory. Like in flat space, the spectrum of type 0 theory can be derived from the type II theory spectrum by a (1)F(-1)^F orbifolding, i.e. combining the untwisted sector where GS fermions are periodic with the twisted sector where GS fermions are antiperiodic (and projecting out all spacetime fermionic states). This construction of the type 0 spectrum may also be implemented using a Melvin background that allows to continuously interpolate between the type II and type 0 theories. As an illustration, we discuss the type 0B spectrum in the pp-wave background which is the Penrose limit of AdS5×S5AdS_5 \times S^5 with RR 5-form flux and also in the pp-wave background which is the Penrose limit of AdS3×S3×T4AdS_3 \times S^3 \times T^4 supported by mixed RR and NSNS 3-form fluxes. We show that increasing the strength of the RR flux increases the value of the effective normal ordering constant (which determines the mass of the type 0 tachyon) and thus effectively decreases the momentum-space domain of instability of the ground state. We also comment on the semiclassical sector of states of type 0B theory in AdS5×S5AdS_5 \times S^5.

Keywords

Cite

@article{arxiv.2110.14683,
  title  = {On type 0 string theory in solvable RR backgrounds},
  author = {Torben Skrzypek and Arkady A. Tseytlin},
  journal= {arXiv preprint arXiv:2110.14683},
  year   = {2022}
}

Comments

28 pages, 3 figures; v3: minor comments added

R2 v1 2026-06-24T07:14:44.498Z