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Fundamental Questions
• What are the most basic building blocks of the universe?
• How do they interact with each other?
원자 가설 (atomic hypothesis)
모든 물질은 원자로 이루어져 있으며 , 이들은 영원히 운동을 계속하는 작은 입자이다 .
John Dalton1766-1844
원자론은 존 돌턴에의해 부활되었다 .그는 모든 물질이 원자로구성되어있다는가정하에 화학반응을성공적으로 설명하였다 .
Richard Phillips Feynman (1918–1988)
다음 세대에 물려줄 과학적 지식을단 한 문장으로 요약해야 한다면 ,그것은 ‘원자가설’일 것이다 .
E. Rutherford
금박실험을 통한 원자핵 발견 (1911)양성자 발견 (1919)
J.J. Thomson
음극선 실험을 통한전자의 발견 (1897)
The Nobel prize in 1906
The Nobel prize in 1908
J. Chadwick
중성자 발견 (1932)
The Nobel prize in 1935“for the discovery of the neutron”
원자핵은 양성자와 중성자로 이루어져 있다
양성자 중성자
그 후 , ‘ 양성자와 중성자는 쿼크로 이루어져 있다’는 것이 밝혀진다
중성미자 (neutrino) 의 발견 (Cowan and Reines, 1956)
Fred ReinesThe Nobel prize in 1995“for the detection of the neutrino”
(observation of inverse beta decay)
God(damn) Particle
• In the Standard Model, particle interactions are dictated by a local gauge symmetry SU(3)c x SU(2)L x U(1)Y.
• Electroweak gauge symmetry is broken spon-taneously by the vacuum value of a scalar (Higgs) field, giving masses to weak gauge bosons and matter particles.
• This implies the existence of a new scalar par-ticle (Higgs particle, aka God particle).
The SM Higgs branching ratio
For mH = 125 GeV,
BR(h bb) ~ 58 %BR(h WW*) ~ 21.6 %BR(h ZZ*) ~ 2.7 %BR(h ττ) ~ 6.4 %BR(h γγ) ~ 0.22 %BR(h gg) ~ 8.5 %
Search Channels for Higgs
For All production mode
For WH/ZH production
Leptons/Photons essential for any search
Global Fit to Higgs data
Best fit converged towardsthe SM; in particular datanow disfavor the solution with c < 0 which appearedin previous fits and gave anenhanced h γ γ
Giardino et al. arXiv:1303.3570
Invisible Higgs Decays
A universal reductionof the rates in all decaychannel
Severely constrained byGlobal fits
Giardino et al. arXiv:1303.3570
Dark Matter Halo
Dark Matter in a galaxy surroundsthe visible matterin a halo.
It might be detectedthrough various ways.
Direct Detection
• Dark Matter particles in the halo might be detected by its elastic scattering with terrestrial nuclear target.
Indirect Detection
• Neutrino Telescopes (e.g IceCube)
High Energy Neutrinos from DM annihilation at the core of SUN can be detected, via ν μ conversion
Indirect Detection
• Search for DM annihilation into gamma rays, antiparticles (antipro-ton, positron)
Positron Excess
• Pulsars remain the best explanation of PAMELA/Fermi excess
• Dark Matter Explanations are tough- Large rates into e+e-- Low rates into antiprotons- But, viable scenarios exist
A Gamma-ray Line
• Positrons are too messy• The observation of gamma-ray line in the
cosmic-ray fluxes would be a smoking-gun signature for dark matter annihilation in the universe
• Weniger found such gamma-ray signatures in the data of Fermi-LAT
A Singlet Scalar DM• Silveira & Zee (85); McDonald (94); Burgess, Pospelov, ter Veldhuis
(00)
- A real scalar S, singlet under the SM gauge group- S -S symmetry, No <S> vacuum expectation value
S stable and neutral- Couplings to all SM fields are controlled by single
parameter λ
Relic Density
DM annihilation cross sectiondepends on λ and ms
Relic density constraint requiresλ ~ O(0.1) and significantlysuppressed near Higgs pole
The connection between λ and ms
derived from the density constraintis very predictive
Direct Detection
DM scattering with nuclei is given by t-channel Higgs exchange
Low DM mass region is ruled outby XENON100 constraint
A region with very light scalar(mS < 10 GeV) still not yet excludedby the precision of XENON100 due to its high threshold
Collider Signatures
R =
Over most of parameter space λ ~ O(0.1)
Higgs production might frequently be associated with S production, potentially leading to strong missing energy signals
A region with very light scalar (mS < 10 GeV) corresponds tovery large invisible branching ratio
A Singlet Scalar DM
• Provide definite predictions for DM-proton scattering cross section and invisible Higgs decay rates, when thermal DM relic den-sity constraint imposed
• Low DM mass region (mS <100 GeV) is dis-favored by XENON100 experiment and LHC discovery of SM-like Higgs, except Higgs pole region
A Singlet Fermionic DM
• YGK & Lee (07); YGK, Lee & Shin (08); Baek, Ko & Park (11); Lopez-Honorez, Schwetz & Zupan (12)
Hidden sector
Connection between hiddenand SM sectors
A Singlet Fermionic DM• The scalar (Higgs) potential develops nontrivial vacuum ex-
pectation values for SM Higgs and singlet scalar
• The neutral scalar fields h and s are mixed, and the corre-sponding mass eigenstates h1 and h2 are given by
• Mixing between h and s makes the physical Higgs boson h1 and h2 have reduced couplings with the SM fermions and the SM weak gauge bosons
Direct Detection
mh1 = 120 GeVmh2 = 500 GeV
If mΨ < mh2,Direct detectionconstraint excludesmost of parameterspace, except Higgspole region
YGK, Lee & Shin (2008)
Direct Detection
mh1 = 120 GeVmh2 = 100 GeV
If mΨ~mh2 (or mΨ>mh2)large parameter spaces,which gives small DM-proton scattering crosssection below XENON100 limit, are allowed
YGK, Lee & Shin (2008)
Secluded DM
• If singlet-like Higgs mass mh2 is less than or simi-lar to DM mass, dominant contribution for DM an-nihilation arises from the following process
Singlet-like Higgs doesn’t decayto DM pair since it’s not kinematicallyallowed, but it decays entirely to SMparticles
This fixes essentially the coupling gs,while leaving the Higgs mixing angle θUnconstrained
Since the direct detection cross sectionis proportional to sin2(2θ), essentially any value below the XENON boundcan be obtained
Direct Detection (mh2 < mΨ)
Parameter choices giving rise toa relic density in the WMAP rangein the Higgs portal model withmh1 = 125 GeV.
Green and red points correspondto mh2 < mΨ with a more (r1 >0.9)or less (r1 < 0.9) SM Higgs-like h1,respectively.
The r1 > 0.9 requirement tends tokeep the scattering cross sectionbelow the XENON100 limit.
(signal strength reduction factor)
Lopez-Honorez, Schwetz & Zupan(2012)
Conclusions• Identified two simple ways to make thermal ferminonic DM consistent
with a SM-like Higgs at 125 GeV and XENON100 bounds
- Resonant Higgs portal. If the DM mass is close to half of the Higgs mass, then the annihilation cross section is enhanced by an s-channel resonance, allowing small couplings and a suppressed direct detec-tion cross section.
- Indirect Higgs portal. If the mediator Ф is lighter than the DM, the relic density can be obtained by ΨΨ→ФФ annihilation, where the diagrams are independent of the Higgs portal strength. The Higgs portal only acts indirectly to provide thermal contact between the dark and the visible sector thermal baths.
• In all cases it is possible to have a SM-like Higgs, with an LHC signal strength modifier r1 > 0.9 (where r1 =1 corresponds to the SM Higgs).
God(damn) Particle
• In the Standard Model, particle interactions are dictated by a local gauge symmetry SU(3)c x SU(2)L x U(1)Y.
• Electroweak gauge symmetry is broken spon-taneously by the vacuum value of a scalar (Higgs) field, giving masses to weak gauge bosons and matter particles.
• This implies the existence of a new scalar par-ticle (Higgs particle, aka God particle).