10 October 2017
One of the simplest viable models for dark matter is, next to the standard model, an additional scalar singlet S, permitted by ℤ2 symmetry.
The Lagrangian density L is expressed then as [1]
(1) L = LSM + LS
where LSM is the standard model density Lagrangian and LS is the scalar singlet dark matter density Lagrangian
(2) LS = 1/2 μS² S² + 1/2 λHSS²H*H + 1/4 λSS⁴ + 1/2 ∂μS∂μS.
From left to right, we have the bare S mass, the Higgs-scalar singlet coupling, the S quartic self-coupling, and the S kinetic term.
The singlet mass mS is obtained from
(3) mS² = μS² + 1/2 λHS v²,
where v = 246.22 GeV is the VEV of H, the Higgs field.
If λHS = 0, dark matter has no interaction with ordinary matter except through gravitational field.
We propose a sum rule or a closure relation relating particle masses and v :
(4) mH² + mW² + mZ² + (mS² − µS²) + mt² + mb² + mc² + mτ² + … = v²
Noticing that, in the electroweak standard model, the couplings of all particles to the H field are proportional to 1/v, namely of the form mi/v [3], we get from Eqs. (3) and (4)
(5) 2λ + g²/4 + (g² + g’²)/4 + λHS/2 + (yt² + yb² + yc² + yτ² + …)/2 = 1
In fact, what we propose is that v² is exclusively built on the particles’ masses. v² is a paved parquet exclusively composed of particles’ masses.
Case with λHS = 0 (mS² − µS² = 0) has been considered in Ref. [3].
With
(6) mH = 125.0 – 125.5 GeV (CMS 2017),
(7) mH = 124.7 – 125.3 GeV (ATLAS 2017),
we guess
(8) mH = 125.0 – 125.3 GeV.
Then Eqs. (3) and (4) imply
(9) mt = 173.6 – 173.9 GeV
to be compared with
mt = 172.0 – 172.9 GeV (CMS 2016) (10)
(11) mt = 172.1 – 173.5 GeV (ATLAS 2017)
Now from Eqs. (10) and (11), we guess
(12) mt = 172.1 – 172.9 GeV
With Eqs (3), (4), (8) and (12), we get
(13) mS² − µS² = 1/2 λHS v² = (15 – 25 GeV)²
or
(14) λHS = 0.008 – 0.021
In Refs. [2], [4] and [5], it has been noted that dark matter phenomenology is driven predominantly by mS and λHS, with viable solutions known to exist in a number of regions, in particular where mS is around mH/2 and where coupling λHS is very small (λHS < 0.01). Furthermore the scalar singlet can constitute all the observed dark matter.
In the framework of the scalar singlet dark matter model — assuming Eq.(4) — a more precise value of λHS is dependent on more precise values of mt and mH.
[1] A. Silveira and A. Zee, “Scalar Phantoms”, Phys. Lett. B 161 (1985) 136-170.
[2] For recent updates and references, see : The Gambit Collaboration, “Status of the scalar singlet dark matter model”, Eur. Phys. J. C 77, 568 (2017), https://arxiv.org/abs/1705.07931.
[3] G. López Castro and J. Pestieau, “Relation between masses of particles and the Fermi constant in the electroweak Standard Model” (2013), https://arxiv.org/abs/1305.4208.
[4] J. M. Cline, K. Kainulainen, P. Scott, and C. Weniger, “Update on scalar singlet dark matter”, Phys. Rev. D 88 (2013) 055025, https://arxiv.org/abs/1306.4710.
[5] A. Beniwal, F. Rajec, et. al., “Combined analysis of effective Higgs portal dark matter models”, Phys. Rev. D 93 (2016) 115016, https://arxiv.org/abs/1512.06458.