  Compactifying the Standard Model (SM) on a circle may lead to AdS 3D vacua,
depending on the character (Majorana or Dirac) and the mass of the lightest
neutrino. It has been shown that, imposing the Ooguri-Vafa conjecture that no
stable non-SUSY AdS vacua are consistent with Quantum Gravity, one can obtain
conditions on the mass of the lightest neutrino. This result has the
shortcoming that it is in general sensitive to the UV structure of the theory.
In the present paper we show that two other independent swampland conditions
may yield constraints very similar to those. These other two conditions come
from the AdS swampland distance conjecture and the dS conjecture as applied to
AdS vacua by Lust, Palti and Vafa. Unlike the non-SUSY AdS constraints, for
these conjectures the results require only local IR information of the radion
potential. We consider both the case of an explicit cosmological 4D constant
and the alternative of a simple quintessence 4D potential. Cosmological data in
the next decade may falsify the results, giving us information on the
constraints of particle physics from Quantum Gravity.
