Abstract

Does the value of the Higgs mass parameter affect the expectation value of local operators in the Standard Model? For essentially all local operators the answer to this question is "no", and this is one of the avatars of the hierarchy problem: nothing is "triggered" when the Higgs mass parameter crosses zero. In this letter, we explore settings in which Higgs mass parameters $can$ act as a "trigger" for some local operators ${\cal O}_T$. In the Standard Model, this happens for ${\cal O}_T = {\rm Tr} (G \tilde G)$. We also introduce a "type-0" two Higgs doublet model, with a $Z_4$ symmetry, for which ${\cal O}_T = H_1 H_2$ is triggered by the Higgs masses, demanding the existence of new Higgs states necessarily comparable to or lighter than the weak scale, with no wiggle room to decouple them whatsoever. Surprisingly, this model is not yet entirely excluded by collider searches, and will be incisively probed by the high-luminosity run of the LHC, as well as future Higgs factories. We also discuss a possibility for using this trigger to explain the origin of the weak scale, invoking a landscape of extremely light, weakly interacting scalars $\phi_i$, with a coupling to ${\cal O}_T$ needed to make it possible to find vacua with small enough cosmological constant. The weak scale trigger links the tuning of the Higgs mass to that of the cosmological constant, while coherent oscillations of the $\phi_i$ can constitute dark matter.

Highlights

  • The apparent failure of naturalness in accounting for the minuscule size of both the cosmological constant and the Higgs mass, is giving us a profound structural clue about the laws of fundamental physics

  • We explore settings in which Higgs mass parameters can act as a “trigger” for some local operators OT

  • We introduce a “type-0” two Higgs doublet model, with a Z4 symmetry, for which OT 1⁄4 H1H2 is triggered by the Higgs masses, demanding the existence of new Higgs states necessarily comparable to or lighter than the weak scale, with no wiggle room to decouple them whatsoever

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Summary

INTRODUCTION

The apparent failure of naturalness in accounting for the minuscule size of both the cosmological constant and the Higgs mass, is giving us a profound structural clue about the laws of fundamental physics. Demanding this Z4 symmetry and requiring that OH is triggered put very tight constraints on the parameters of the model Both Higgses are forced to get a vev, while the Z4 forbids the Bμ term BμH1H2 and so the new Higgses can only be raised in mass via quartic couplings, demanding the existence of new Higgs states necessarily comparable to or lighter than the weak scale, with no wiggle room to decouple them whatsoever. Using the weak scale as a trigger allows us to tie solutions to the cosmological constant and hierarchy problems In this scenario, at least part of the landscape is associated with ultralight fields, which are not frozen to their minima but are oscillating in the Universe today, providing novel possibilities for coherently oscillating dark matter, and mediating (extremely weak) long-range forces

THE WEAK SCALE AS A TRIGGER
The weak scale as a trigger in the type-0 2HDM
Masses and couplings
Experimental constraints
Direct searches
Indirect constraints
WEAK SCALE TRIGGERING LOW ENERGY LANDSCAPE FOR SMALL CC
SM trigger of the landscape
Type-0 2HDM triggering of the landscape
ULTRALIGHT DARK MATTER FROM WEAK SCALE TRIGGERS
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