Abstract

In the past, Kundu et al. and Chakraborty et al. used extra scalar fields to cancel the quadratic divergences in the Higgs mass squared and they determined the mass of the required scalar field. In this work, a spin-3/2 particle has been used in the same manner to nullify the power-law divergences, and it is determined that the mass of the spin-3/2 particle resides in the ball park of the GUT scale.

1. Introduction

With the discovery of a resonance at the LHC [1, 2] that seems to be rather consistent with the standard model Higgs boson in light of the ongoing assessment of its properties [311]; the electroweak naturalness [12, 13] is the foremost problem that we should turn our attention to. Even though many new physics theories have been suggested in order to cure the destabilization of the Higgs mass [1419], so far, no signal of these has been observed [2026]. The lack of any new physics particle at the TeV scale casts doubts on the relevance of the idea of naturalness and strengthens the view that the standard model (SM) of electroweak and strong interactions may well be the model of physics at Fermi scale [2730]. However, this situation does not change the fact that SM is an incomplete, effective theory since, for one thing, it is missing the essential dark matter (DM) candidate [3137] and for another, it offers no dynamical principle that generates the masses and couplings of the theory [3841].

Since requiring that the SM be technically natural brings us to a dead end in terms of guidelines to new physics (NP), we explore an orthogonal possibility here and assume that the electroweak scale is stabilized via a mechanism based on the fine-tuning of a sector which is split from the SM. The same line of reasoning has been employed before by Kundu and Raychaudhuri [42] and Chakraborty and Kundu [43] through different models based on singlet scalars. The main motive behind this approach is to cancel the power-law divergences in the Higgs mass squared via the loops of extra fields and fine-tuning the parameters of the specific BSM model that is utilized [44, 45]. Even though this is intrinsically a fine-tuning operation, it brings along valuable advantages such as accommodating viable dark matter candidates [4648]. However, exploiting real scalar fields for this comes with its own drawbacks. Since real singlet scalars with a vacuum expectation value are bound to mixing with the CP—even component of the SM Higgs field itself, an all-encompassing, simultaneous cancellation is not achievable [49].

In the present work, we study the Higgs mass stabilization problem by a hidden spin-3/2 particle high above the electroweak scale and examine the radiative corrections it induces on the Higgs self-energy in an effective field theory approach using cutoff regularization so as to obtain an estimate of the mass of this new particle by demanding that the total one loop corrections to the Higgs mass should cancel. The main advantage of our model over the singlet scalar approaches is that while the latter need auxiliary fields such as vector-like fermions in order to stabilize the NP sector itself, hidden spin-3/2 field is free from such requirements. Due to the unique character of our spin-3/2 interaction with the SM, it is impossible to observe a spin-3/2 particle on mass shell. This means that the BSM sector in our model is a genuinely stable hidden extension of SM. This constitutes a phenomenological advantage, which has important implications not just for the electroweak stabilization but also for the Higgs boson and hidden sector correlation. Another implication is related to the fact that our calculations reveal that this higher spin particle resides in the ball park of the GUT scale. If ongoing searches at the LHC reveal no particles at the TeV scale combined with the fact that the next higher spin particle (spin-3/2) inhabits the GUT scale may strengthen the grand desert notion in the GUTs without TeV scale NP [50].

2. The Hierarchy Problem

Spontaneous breaking of electroweak symmetry is implemented in the SM by postulating the existence of a fundamental scalar, the Higgs field, whose potential is parameterized by a dimensionful mass-squared parameter and a dimensionless Higgs self-coupling . The Higgs field takes on a constant value everywhere in space-time called the vacuum expectation value () which being a dimensionful parameter sets the scale for all the masses of the theory in terms of the Yukawa couplings.

Fundamental scalars are widely considered as unnatural. As opposed to the fermions and gauge bosons whose masses are under control by chiral and gauge symmetries, respectively, masses of fundamental scalars are not protected by any kind of symmetry. This makes them vulnerable to divergent radiative corrections they get from loop diagrams. The technical usage of the term naturalness is related to the quantum corrections that a parameter gets when one makes use of perturbation theory to calculate the properties of a theory.

The hierarchy problem we consider here is specifically associated with the quantum corrections to the Higgs mass-squared . A simple statement of the problem can be given as follows. In an effective field theory with a hard ultraviolet cutoff , loop diagrams induce radiative corrections in the Higgs self-energy such that where is the physical Higgs boson mass, is the renormalized gauge couplings of the SM, and the second term signifies the quantum corrections. If the second term in (1) is of the same order or smaller than the measured value of the Higgs mass, it is said that the parameter is natural; however, if the measured value turns out to be much smaller than the radiative correction term, it is said that the theory is unnatural because this hints at a contingent cancellation between the bare mass and the quantum effects so as to produce the measured value of the Higgs boson mass.

Originally put forward by Veltman [51], the SM one-loop corrections to the Higgs boson mass reads where and are the and gauge couplings in the SM, respectively, and is the top quark Yukawa coupling. Only the top quark Yukawa coupling appears in (2) because the contributions of other fermions are considerably small. Veltman stated that the Higgs mass should be stable against loop corrections, and the above criterion is used as a means to estimate the Higgs boson mass; hence, this expression is commonly called the Veltman condition (VC).

The Higgs mass estimated using VC is in conflict with the experimental value today, and we are in a bit of quandary. Considering the fact that the cutoff regulator can get as high as the Planck mass, we are faced with an unnaturalness of 32 orders of magnitude. If we require that the Higgs be technically natural, there should appear new physics around TeV scale and remove the quadratic dependence on the cutoff scale .

People following this motivation have come up with many NP theories, and chief among them is supersymmetry [52, 53]. However, despite all the extensive searches, no compelling evidence in favor of any of these NP theories has been observed during the LHC runs reaching well above the TeV scale.

Having no TeV scale NP to prevent the destabilization of the Higgs boson, new mechanisms have been put forward which involve extensions beyond the SM and general relativity. One such mechanism which makes use of conformal symmetry has been introduced by W. A. Bardeen in 1995 [54] and paved the way for many variants since then. Antigravity effects have also been claimed to be viable in improving the naturalness of electroweak sector [55]. Another interesting possibility is exploiting the coupling between the Higgs boson and the space-time curvature as a means of harmless, soft fine-tuning that was shown to be capable of solving the hierarchy problem [56].

Aside from all these different approaches, a general practice is to invoke a cancellation mechanism which involves fine-tuning of counter-terms that mixes together both low- and high-scale physical degrees of freedom. The scheme that has been followed here in this work is in line with the aforementioned cancellation mechanism approach but it is a completely new model with a unique interaction. The next section is devoted to the description of this model. We first start by a quick review of spin-3/2 and then continue on with the details of the interaction Lagrangian. The interaction is such that, at the renormalizable level, it is only through the neutrino portal that spin-3/2 makes contact with the SM. Due to the special constraints that these fields should obey, they can participate interactions only as virtual particles. Without further ado, let us get to the details in the next section.

3. The Model

Spin-3/2 fields, commonly called vector spinors, , are introduced to the literature for the first time by Rarita and Schwinger [57]. The propagator for the reads and it involves one spin-3/2 and two spin-1/2 components embedded in the projector [58] which exhibit both spinor and vector characteristics. In order to remove the two spin-1/2 components, we impose the two constraints [59, 60] after which satisfies the Dirac equation as expected of an on-shell fermion. The constraints (5) and (6) imply that and both vanish on the physical shell .

Characteristic of singlet fermions, the , at the renormalizable level, makes contact with the SM via in which is the lepton doublet (), and is the Higgs doublet with vacuum expectation value , Higgs boson , and Goldstone bosons , , and (forming the longitudinal components of , , and bosons, respectively).

Because of the constraint in equation (6), effects of the vector spinor are mainly restricted to the loop diagrams. One such diagram is depicted in Figure 1. As a result of this interaction, contributes to the Higgs boson mass correction given in (2).

The contribution of the Feynman diagram in Figure 1 is given by

The term in the square brackets is the propagator of , where is the projector as a function of the loop momentum of , the explicit form of which is

The leftmost vertex is designated by and the other by ; hence, the two vertex factors are respectively.

After taking the integral over the loop momentum of the neutrino , the expression takes the form

There are five traces that should be evaluated, and they are denoted by , , , , and in the following:

Equation (15) in terms of the five traces can be written as

After replacing the values of the traces, the term in the square brackets in equation (17) becomes

Plugging equation (18) into equation (17), it is possible to split the integral over into two halves

Denoting the first integral by and the second by , equation (19) takes the form

Using cutoff regularization, the two integrals and are evaluated to be where designates the cutoff scale.

After inserting equations (21) and (22) into (20), the mass correction to the Higgs mass due to the spin-3/2 particle becomes

It is interesting to note that the mass correction in (23) is of positive sign and purely quartic (no quadratic correction arises due to spin-3/2), although one would expect it to have the opposite sign since this is a fermion that we are dealing with. The crucial point is that the origin of this quartic contribution can be traced back to the last term in the propagator of the spin-3/2, to wit, the term in equation (4), and that tells us that the longitudinal component of the propagator overrides the fermionic character at high energy.

After this remark, now, let us get back to the calculation. Recall that the SM one-loop correction to the Higgs mass reads

The total correction to the Higgs mass is the sum of SM part plus the spin-3/2 contribution; to wit

If we allow the possibility that the hidden sector is finely tuned such that the total quantum correction to vanishes, i.e., we have a clear constraint on the mass scale of the quanta of the spin-3/2 field

If we take the cutoff scale to be the Planck mass and the coupling constant of the spin-3/2, , of order unity, this gives us as the mass scale of the spin-3/2 quanta.

4. Summary

In this work, we have taken up the hierarchy problem from a different angle. Contrary to the general acceptance that electroweak scale should be technically natural, we have allowed the possibility that fine-tuning may well be the option that nature favors. The rationale behind this choice is the nonexistence of any experimental proof of the natural theories of BSM that predict TeV scale NP so as to stabilize the Higgs boson.

We have assumed that the Higgs boson stays stable via a finely tuned hidden sector which involves a spin-3/2 field that is split from the SM and whose sole contact with it at the renormalizable level is through the neutrino portal. The interaction Lagrangian of our model is given by equation (8) along with the two constraints (equations (5) and (6)) that these fields should obey so as to satisfy the Dirac equation. The distinctive feature of this model is that the spin-3/2 field is enforced to be inherently off-shell due to the constraint (equation (6)). As such, this field is hidden from the SM and the effects of it are mainly expected to be visible through the loop diagrams.

One such diagram that one can witness the effects of is the loop given in Figure 1 which designates the contribution of the spin-3/2 to the Higgs self-energy. As such, this diagram plays an important role in the hierarchy problem.

The loop diagram that we have depicted in Figure 1 induces a quartic radiative correction in the Higgs mass. However, contrary to the general expectation that fermions should have negative radiative power law corrections to the Higgs mass, what we observe here is that the spin-3/2 field has a positive contribution. This strange phenomenon can be traced back to the longitudinal terms in the propagator of and reveals that the fermionic character is washed out at high energy.

After making the pivotal assumption that the Higgs mass stays stable via a mechanism that involves a finely tuned hidden sector, we have used the total mass correction to the Higgs mass as a constraint to calculate the mass scale of the spin-3/2 field. This calculation has revealed that the spin-3/2 field is indeed split from the SM because it resides well above the SM with a mass around which is in the ball park of GUT scale. Even though there is no phenomenological possibility so far to prove the correctness of the theory which extends to the GUT scale, this finding offers a plausible support for the notion called the grand desert in the GUTs without TeV scale NP.

Data Availability

No data were used to support this study.

Conflicts of Interest

The author declares that he has no conflicts of interest.

Acknowledgments

The author is grateful to Durmuş Ali Demir for fruitful discussions.