Form factor effects in a Higgs portal pionic dark matter...
Transcript of Form factor effects in a Higgs portal pionic dark matter...
Form factor effects in a Higgs portal pionic dark matter model
Shohei Okawa (Nagoya U.)
in collaboration with Masaharu Tanabashi (Nagoya U.)
March 16-20, 2015 Exploring the Dark Sector @ KIAS
Outline!
Introduction
Model
What are form factor effects ?
Our strategy
Results
Summary and Outlook
Higgs portal DM=DM which interacts the SM particles only through the Higgs The nature of the DM is mainly determined by DM mass and the portal interactions to the Higgs !
The simplest case : mDM , λhXX predictive ⇔ severe constrained
λhXX is determined as a function of DM mass
mDM is constrained
Thermal relic density
hSM
SM
DM
DM s = 4m2DM
Direct detection
h
NN
DM DM
s = 0
Collider search
h
SM
SM
DM
DMs = E2
cm
Higgs portal dark matter
h
DM
DM
However, each process occurs at different energies and/or channels !!!!!
It’s significant to consider a case that the portal interactions to the Higgs depend on the energy and/or channels, not just constant
!!!!
Possibilities : Radiative corrections Extra mediator Composite DM … etc.
Motivation
Thermal relic density
hSM
SM
DM
DM s = 4m2DM
Direct detection
h
NN
DM DM
s = 0
Collider search
h
SM
SM
DM
DMs = E2cm
�hXX(s) = h
DM
DMs
Klasen, Yaguna, Ruiz-Alvarez (2013) ; T. Abe and R. Sato (2015) ; Tsai’s talk on Wed.
P. Ko et al. (2007) ; Y. G. Kim et al. (2008), etc.
Jung, et al. (2011) ; Wudka et al. (2013) ; Tuominen et al. (2013) ; J. Kubo et al. (2013), etc.
MotivationComposite DM
MotivationComposite DM
Strong interactions behind the SM
MotivationComposite DM
Strong interactions behind the SM
Scale invariant extension of the Standard Model
Dong-Won Jung’s talk
EW scale can be originated from the strong dynamics
MotivationComposite DM
Strong interactions behind the SM
Scale invariant extension of the Standard Model
EW scale can be originated from the strong dynamics
Form factor effects characteristic of composite particles
Dong-Won Jung’s talk
MotivationComposite DM
Strong interactions behind the SM
EW scale can be originated from the strong dynamics
Form factor effects characteristic of composite particles
Scale invariant extension of the Standard Model
Our work
Dong-Won Jung’s talk
Outline!
Introduction
Model
What are form factor effects ?
Our strategy
Results
Summary and Outlook
Model
A QCD-like SU(3) gauge interaction w/ 2-flavor fermions in the fundamental rep. Q’s are invariant under the SM gauge transf.
Dark pions = DM candidates
Dark-QCD
L = LSM +X
Q=U,D
✓Q̄(i /D �MQ)Q� 1
⇤(H†H)Q̄Q
◆
Higgs portal int.
Dim. 5 op. → EFT Λ : Cut-off scale
Dynamical chiral symmetry breaking (DχSB) +
Dark color confinement
& Higgs portal
Outline!
Introduction
Model
What are form factor effects ?
Our strategy
Results
Summary and Outlook
!!!!!
!For illustration, let us consider a specific case
h⇧a(p0)| Q̄Q |⇧b(p)i = FS(s)�ab, s = (p� p0)2
scalar form factor of the dark pion�h⇧⇧(s) = h
p� p0
⇧a
⇧a
=v
⇤FS(s)
What are form factor effects ?Higgs portal interaction
Decay constant Mass
F⇧ = 103f⇡
M⇧ = 103m⇡
Dark pion’s properties
Typical scale
Dark quark mass MU = 103mu, MD = 103md
⇤dark = 103⇤QCD ⇠ 1 TeV
In this case,
What are form factor effects ?
In this case,
Collider search
s = E2cm
h
SM
SM
⇧a
⇧a
Thermal relic density
hSM
SM
⇧a
⇧a s = 4M2⇧
Direct detection
h
NN
s = 0
⇧a ⇧a
Form factor effects
�h⇧⇧(s = M2⇧) 6= �h⇧⇧(s = 0) 6= �h⇧⇧(s = E2
cm)
What are form factor effects ?
Outline!
Introduction
Model
What are form factor effects ?
Our strategy
Results
Summary and Outlook
!!!!!!!!!!!!!Then, how do we calculate the scalar form factor of the dark pions ?
Chiral Perturbation Theory (χPT)
M⇧, F⇧ : Free parameters
Specific case → General case
Decay constant Mass
F⇧ = 103f⇡
M⇧ = 103m⇡
Specific case General case
?
In the SM QCD, χPT is successful calculation method in describing the mesonic interactions at low energy !!!!!!!!!!!!!O(p2) χPT corresponds to the simplest case → No form factor effect O(p6) χPT can explain the experimental behavior quite well up to ~400 MeV
O(p2)
O(p4)
O(p6)
Experiment
Bijnens et al. , JHEP 9805 (1998)
χPT estimate of form factor
Outline!
Introduction
Model
What are form factor effects ?
Our strategy
Results
Summary and Outlook
Thermal relic density
hSM
SM
⇧a
⇧a s = 4M2⇧
h
NN
s = 0
⇧a ⇧a
Direct detection
h
s = m2h
⇧a
⇧a
Higgs invisible decay
Measurements we use
(PDG 2014)
LUXXENON100
Spin-independent (SI) cross section
Br(h ! inv) = 0.51
(arXiv:1404.1344 CMS)
(2014)
(2012)
⌦CDMh2 = 0.1198± 0.0026
O(p2) χPT (no form factor effect)
2M⇧ ⇠ mh, 200 GeV . M⇧Kanemura et al. (2010) ; CMS collaboration (2014), etc.
DM thermal relic
Higgs invisible decay
XENON100
LUX
Resonance region
O(p6) χPT (FΠ = 50 GeV)
2M⇧ ⇠ mh, 100 GeV . M⇧2M⇧ ⇠ mh, 200 GeV . M⇧
O(p2) χPT O(p6) χPT (FΠ = 50 GeV)
DM thermal relic
Higgs invisible decay
XENON100
LUX
Varying FΠ continuously, we can obtain the figure below
+ Resonance regionF⇧ [GeV]
M⇧[G
eV]
Excluded region
Lower bound in O(p2) χPT
non-reliable region of the calculation in χPT
O(p2) χPT O(p6) χPT
200 GeV . M⇧ 80 GeV . M⇧
Results
Outline!
Introduction
Model
What are form factor effects ?
Our strategy
Results
Summary and Outlook
Summary and OutlookSummary When we consider a QCD-like strong interaction in the hidden sector, the pNGBs resulting from DχSB, which we call the dark pions, can be Higgs portal dark matters !Form factor effects on the portal interaction between the Higgs and the dark pions tend to relax the constraint on the dark pion mass !
Outlook Since the non-reliable region of the calculation in χPT isn’t equal to the excluded region, thus we want to reduce that region
Modified Omnès representation
Back UP
O(p4) chiral Lagrangian !!!!!!!We determined the LECs as follows,
Low energy constants (LECs) in Dark-QCD
LO(p4)chiral = L1
�tr[(@µU)(@µU†)]
�2+ L2 tr[(@µU)(@⌫U
†)(@µU)(@⌫U †)]
+ L3 tr[(@µU)(@µU†)(@⌫U)(@⌫U †)]
+ L4 tr[(@µU)(@µU†)] tr[�U† + U�†] + L5 tr[(@µU)(@µU†)(�U† + U�†)]
+ L6
�tr[�U† + U�†]
�2+ L7
�tr[�U† � U�†]
�2
+ L8 tr[�U†�U† + U�†U�†]
Lr5(µ = 770 MeV)⇥ 103 = 1.21± 0.08
Lr5(µ = 770 GeV)⇥ 103 = 1.21± 0.08
SM QCD
Dark-QCD
( f⇡ = 93 MeV )
( F⇧ = 93 GeV )
!!!!!!Generally, scalar form factor in χPT can be divided into two parts
Explicit expression of scalar form factor
N = 16⇡2
PS(s) 3s
M2⇧
,
✓s
M2⇧
◆2
US(s) 3 lns
M2⇧
,s
M2⇧
lns
M2⇧
,
✓s
M2⇧
◆2
lns
M2⇧
, · · ·
Polynomial term
Dispersive term
FS(s) = FS(0)
⇢1 +
M2⇧
F 2⇧
✓s
M2⇧
� 1
2
◆J(s) +
s
M2⇧
✓lr4 � L� 1
N
◆�+
M4⇧
F 4⇧
(PS(s) + US(s))
�
L =1
Nln
M2⇧
µ2
s
M2⇧
✓lr4 � L� 1
N
◆
J(s) ⇠ lns
M2⇧
!!! is necessary ? → Yes !
�h⇧⇧(s = 0)
v=
2M2⇧
v2F(M⇧/F⇧)
⇠ 2M2⇧
v2(M⇧/F⇧ . 3)
F⇧ = 50 GeV
Necessity of dark quark mass
L = LSM +X
Q=U,D
✓Q̄(i /D �MQ)Q� 1
⇤(H†H)Q̄Q
◆