We propose that the possible 750 GeVdiphoton excess can be explained in the color-octet neutrino mass model extended with a scalar singlet . The model generally contains N s species of color-octet, electroweak doublet scalars S and N f species of color-octet, electroweak triplet χ or singlet ρ fermions. While both scalars and fermions contribute to the production of through gluon fusion, only the charged members induce the diphoton decay of . The diphoton rate can be significantly enhanced due to interference between the scalar and fermion loops. We show that the diphoton cross section can be from 3 to 10 fb for O(TeV) color-octet particles while evading all current LHC limits.
The modelRecently, both ATLAS and CMS have found an excess in the diphoton channel around 750 GeV with a width possibly 45 GeV in the LHC run-II data at √ s = 13 TeV [1,2]. The local significance of the excess is 3.6σ at 747 GeV and 2.6σ at 760 GeV, and the global significance is 2.0σ and 1.2σ for ATLAS [1] and CMS [2], respectively. While CMS previously observed a slight excess ∼ 2σ around 750 GeV at, ATLAS did not go beyond 600 GeV in the same channel [4]. If the excess persists with accumulation of more data in the near future, it will likely point to new physics beyond the standard model (SM). The excess has caused a burst of discussions on its possible origin in various phenomenological frameworks .On the other hand, there is an established piece of evidence for new physics beyond SM, namely the neutrino mass; and a e-mail: dingran@mail.nankai.edu.cn b e-mail: hanzhilong@mail.nankai.edu.cn c e-mail: liaoy@nankai.edu.cn d e-mail: maxid@mail.nankai.edu.cn dark matter whose gravitational evidence is robust may also originate from new particles and physics that are unknown to us so far. It would be desirable if the newly found excess is related to the same physics of the neutrino mass or dark matter. In this work we try to connect the excess with physics that is responsible for neutrino mass. Since the cross section for the excess is large for such a heavy resonance, it seems natural that the resonance is produced and decays through interactions with some new particles that participate in strong and electromagnetic interactions. In this context the color-octet model of the neutrino mass [162] stands out, in which the octet particles generating radiative neutrino mass would also couple to the resonance field resulting in its strong production and electromagnetic decay.Since the nature of the resonance, named below, such as parity and spin is completely unknown, we treat it in the simplest manner from the point of view of effective field theory. Assuming it is an electroweak singlet of spin zero, its relevant effective interaction with color-octet scalars iswhere the octet fields S a r have the same electroweak quantum numbers as the SM Higgs field H with a referring to color and r enumerating N s ≥ 1 such scalars. We note two points in passing. First, the interaction entering radiative neutrino mass is proportional to S a † r H S ...