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Scotoseesaw mechanism from a $$Z_3$$ symmetry of matter
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Abstract
We show that the neutrino mass generation and the dark matter stability can be governed by the center of the QCD group, which is a
$$Z_3$$
Z
3
group. Three right-handed neutrinos
$$N_{1,2,3R}$$
N
1
,
2
,
3
R
transform under
$$Z_3$$
Z
3
as
$$1,w,w^2$$
1
,
w
,
w
2
, where
$$w=e^{i2\pi /3}$$
w
=
e
i
2
π
/
3
is the cube root of unity, and they couple to usual lepton doublets via the usual Higgs doublet H and two new scalar doublets
$$\eta ,\chi $$
η
,
χ
, which transform under
$$Z_3$$
Z
3
as
$$1,w^2,w$$
1
,
w
2
,
w
, respectively. This leads to a scotoseesaw mechanism in which the seesaw and scotogenic neutrino mass generations are induced by the Majorana
$$N_{1R}$$
N
1
R
mass and the Dirac
$$N_{2,3R}$$
N
2
,
3
R
mass, respectively. Although the lightest of the
$$Z_3$$
Z
3
fields is stabilized, responsible for dark matter, the model lacks an explanation for relic density and/or direct detection. The issue can be solved in a
$$U(1)_{B-L}$$
U
(
1
)
B
-
L
gauge completion of the model, for which the center of the QCD group is isomorphic to
$$Z_3=\{1,T,T^2\}$$
Z
3
=
{
1
,
T
,
T
2
}
for
$$T=w^{3(B-L)}$$
T
=
w
3
(
B
-
L
)
.
Springer Science and Business Media LLC
Title: Scotoseesaw mechanism from a $$Z_3$$ symmetry of matter
Description:
Abstract
We show that the neutrino mass generation and the dark matter stability can be governed by the center of the QCD group, which is a
$$Z_3$$
Z
3
group.
Three right-handed neutrinos
$$N_{1,2,3R}$$
N
1
,
2
,
3
R
transform under
$$Z_3$$
Z
3
as
$$1,w,w^2$$
1
,
w
,
w
2
, where
$$w=e^{i2\pi /3}$$
w
=
e
i
2
π
/
3
is the cube root of unity, and they couple to usual lepton doublets via the usual Higgs doublet H and two new scalar doublets
$$\eta ,\chi $$
η
,
χ
, which transform under
$$Z_3$$
Z
3
as
$$1,w^2,w$$
1
,
w
2
,
w
, respectively.
This leads to a scotoseesaw mechanism in which the seesaw and scotogenic neutrino mass generations are induced by the Majorana
$$N_{1R}$$
N
1
R
mass and the Dirac
$$N_{2,3R}$$
N
2
,
3
R
mass, respectively.
Although the lightest of the
$$Z_3$$
Z
3
fields is stabilized, responsible for dark matter, the model lacks an explanation for relic density and/or direct detection.
The issue can be solved in a
$$U(1)_{B-L}$$
U
(
1
)
B
-
L
gauge completion of the model, for which the center of the QCD group is isomorphic to
$$Z_3=\{1,T,T^2\}$$
Z
3
=
{
1
,
T
,
T
2
}
for
$$T=w^{3(B-L)}$$
T
=
w
3
(
B
-
L
)
.
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