2021
DOI: 10.1103/physrevd.103.106006
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Universal class of type-IIB flux vacua with analytic mass spectrum

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Cited by 12 publications
(23 citation statements)
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“…In our scheme, the mass spectrum clearly depends on the correction K (3) , as one of the fields is only stabilised when they are taken into account. This is also consistent with the results of [45,48], since the parameter ξ that controls their mass spectrum is a simple function of K (3) . Furthermore, we also showed that in one particular case in which the matrix M is not invertible, we recover the residual flat direction found in [47] for the same flux choices.…”
Section: Discussionsupporting
confidence: 90%
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“…In our scheme, the mass spectrum clearly depends on the correction K (3) , as one of the fields is only stabilised when they are taken into account. This is also consistent with the results of [45,48], since the parameter ξ that controls their mass spectrum is a simple function of K (3) . Furthermore, we also showed that in one particular case in which the matrix M is not invertible, we recover the residual flat direction found in [47] for the same flux choices.…”
Section: Discussionsupporting
confidence: 90%
“…Hence, the ansatz m a = (r/q)S abm b implies that C a = C a = 0 in (4.28). Thenm a ∝ t a and S ab ∝ κ ab , as in [48]. Moreover the ratio t a /t 0 is easily fixed at leading order, since (4.28) gives Finally, (4.30) determines the vev for the saxion t 0 .…”
Section: Jhep08(2021)077mentioning
confidence: 88%
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