With existing literature, where such behavior is attributed to the pure gravityĬomponent of the couplings. In particular, we find several examples of $(\mathfrak Project we begin exploring this idea and we give a systematic construction ofĥd generalized ``bifundamental'' SCFTs, building from geometric engineering It is therefore natural to ask whether 5d SCFTs canīe organized in a similar manner, as the outcome of fusions of certainĮlementary building blocks, which we call 5d conformal matter theories. Generalize matter and can be fused together to form all known 6d SCFTs in terms Six-dimensional superconformal field theories (SCFTs) have an atomicĬlassification in terms of elementary building blocks, conformal systems that We also generalize ourįindings to the case of perturbation by several tachyon vertex operatorsĬarrying different momenta, and obtain interesting analytic predictions for theĭisk two-point and annulus one-point functions with ZZ boundary condition. Of string theory in the small $\lambda$ expansion. The matrix model results perfectly match those Parameter $\lambda$, while the matrix model gives results which are Technique is used to compute two orders of the expansion in the SL perturbation Leading and subleading orders in the string coupling expansion. Mechanics and using string theory methods. Matrix model formulation based on a chiral representation of matrix quantum Theory in a non-trivial tachyon background. (SL) theory, which provides a worldsheet description of two-dimensional string We compute instanton corrections to the partition function of sine-Liouville Subjects: High Energy Physics - Theory (hep-th) Have phenomenological implications for BSM physics such as GUTs, suggesting forĮxample a weak or absent gravitational wave signature from the GUT Higgsing If one wants the inflationary scale to lie below the species scale in thisĬase, this bounds the inflationary scale to be $\ll 10^5$ GeV. Violated during inflation is to have a large number of species becoming light. Values of the Higgs in the SM satisfy the bound. Magnitude of the Higgs mass should be heavier than a bound proportional to theĮlectroweak scale (or generally the scale set by the Higgs VEV). For Higgsing of nonabelian gauge fields, I find that the Lente without thermal effects only bounds the confinement scale to be above the Should be higher than a scale proportional to the vacuum energy, while Festina Strengthens the implications of this bound. I consider the Festina Lente Swampland bound and argue taking thermalĮffects, as for instance occur during reheating, into account significantly Subjects: High Energy Physics - Theory (hep-th) Cosmology and Nongalactic Astrophysics (astro-ph.CO) General Relativity and Quantum Cosmology (gr-qc) High Energy Physics - Phenomenology (hep-ph)
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