21-23 octubre 2019
Eurostars Palacio de Cristal
Europe/Madrid timezone

A Strong Scalar Weak Gravity Conjecture and Some Implications

21 oct. 2019 15:40
20m
Física Teórica Física Teórica

Ponente

Sr. Eduardo Gonzalo (IFT UAM/CSIC)

Abstract

We propose a new version of the scalar Weak Gravity Conjecture (WGC) which would apply to
any scalar field coupled to quantum gravity. For a single scalar it is given by the differential constraint
$(V'')^2\leq (2V'''^2- V''V'''')M_{\text{p}}^2$,
where $V$ is the scalar potential.
It corresponds to the statement
that self-interactions of a scalar must be stronger than gravity for any value of the scalar field.
We find that the solutions which saturate the bound correspond to towers of extremal states
with mass $m^2(\phi)=m_0^2/((R/m)^2+1/(nR)^2)$, with $R^2=e^\phi$, consistent with the emergence of an extra dimension
at large or small $R$ and the existence of extended objects (strings). These states act as WGC states for the scalar $\phi$.
It is also consistent with the distance swampland conjecture with a built-in duality symmetry.
All of this is remarkable since neither extra dimensions nor string theory are put in the theory from the beginning, but they emerge.
This is quite analogous to how the 11-th dimension appears in M-theory from towers of Type IIA solitonic $D0$-branes.
From this constraint one can derive several swampland conjectures from a single principle. In particular
one finds that an axion potential is only consistent if $f\leq M_{\text{p}}$, recovering a result
already conjectured from other arguments.

            The conjecture has far reaching consequences and applies to several
            interesting physical systems: i) Among chaotic inflation potentials only those asymptotically linear may survive. ii) 
            If applied to the radion of the circle compactification of the Standard Model to 3D with Dirac neutrinos, the
            constraint implies that the 4D cosmological constant scale must be larger than the mass of the lightest neutrino,
            which must be in normal hierarchy. It also puts a constraint on the EW scale, potentially explaining the hierarchy problem.
            This recovers and improves results already obtained by applying the AdS swampland conjecture, but
            in a way which is independent from UV physics.  iii)
            It also constraints simplest moduli fixing string models. The simplest KKLT model is compatible with
            the constraints but the latter may be relevant for some choices of parameters.

Autor primario

Sr. Eduardo Gonzalo (IFT UAM/CSIC)

Materiales de la presentación

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