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Precision Measurements after the Higgs Discovery. M.V. Chizhov Sofia University, Bulgaria and JINR, Russia. July 4, 2012. Is it the Higgs, or isn’t Higgs?. Mean Lifetime and Branching Ratios of the Higgs Boson. M. A. Shifman, A. I. Vainshtein, M . B. Voloshin, and V. I. Zakharov , - PowerPoint PPT Presentation
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Precision Measurementsafter the Higgs Discovery
M.V. ChizhovSofia University, Bulgaria and JINR, Russia
10/06/2014
July 4, 20122
10/06/2014 3
Is it the Higgs, or isn’t Higgs?
2210 s
2310 s
2410 s
2510 s
Mean Lifetime and Branching Ratios of the Higgs Boson
4
g
t
t
tg
g
g
2 32
3
2 2 20
21 2
21
( 2 ) ,128 2
(1 ), 4
2 (1 ) 1 ,
2 3 3 (2 ) .
F Hs
s H
G MH F
F x m M
F x
F x
1arctan , 1
1
1 11ln , 1
2 1 1
x
i
M. A. Shifman, A. I. Vainshtein, M. B. Voloshin, and V. I. Zakharov, Sov. J. Nucl. Phys. 30 (1979) 711
10/06/2014
10/06/2014 5
SM Higgs Production at the LHChttps://twiki.cern.ch/twiki/bin/view/LHCPhysics/CrossSections
LHC in 2012 at record luminosity (7 × 1033 cm-2s-1) and energy (8 TeV) was producing SM Higgs bosons (MH = 125 GeV) at a rate ~ 6𝟓 𝟎/hr
s[pb]
19.27
1.578
0.7046 0.4153
0.1293
125 GeV
10/06/2014
Higgs Boson Signalfrom the Last ATLAS Data
AT
LA
S-C
ON
F-2
013-
014
H
0.50.6
m 125.5 GeV
0.2(stat)
(sys)
6AT
LA
S-C
ON
F-2
013-
108
Phys. Lett. B 726 (2013) 88 (July 4, 2013)
(Nov 28, 2013)
10/06/2014
Higgs Coupling Constantsfrom ATLAS and CMS Results
Hm 125.7 0.3(stat) 0.3(sys) GeV
7
10/06/2014 8
Higgs Spin/Parity at TevatronJ. Ellis, D. S. Hwang, V. Sanz and T. You, JHEP 1211 (2012) 134;
D0 Note 6387-CONF (2013), D0 Note 6406-CONF (2013)
Idea from D. J. Miller, S. Y. Choi, B. Eberle, M. M. Muhlleitner and P. M. Zerwas, Phys. Lett. B505 (2001) 149. Discriminating power is provided by the threshold behaviour of the cross section: s-wave for 0+ s ~ b, p-wave for 0- s ~ b3, d-wave for 2+ s ~ b5.
10/06/2014 9
Results
Phys. Lett. B 726 (2013) 120 Phys. Rev. D 89 (2014) 09207arXiv:1312.5353
10/06/2014 10
Spin and Parity of New Boson:Evidence for 0+ Nature of the Higgs
The orange (blue) band represents the 1σ, 2σ, and 3σ around the median expected value for the SM Higgs boson hypothesis (alternative hypothesis). The black point represents the observed value. The hypotheses of a pseudoscalar and all tested spin-one boson hypotheses are excluded at a 99,9% confidence level or higher. All tested spin-two boson hypotheses are excluded at a 95% confidence level or higher.
Expected (blue triangles/dashed lines) and observed (black circles/solid lines) confidence level CLs for alternative spinparity hypotheses assuming a 0+ signal.
10/06/2014
Universal Fit (LHC+TeVatron)P.P. Giardino, K. Kannike, I. Masina, M. Raidal
and A. Strumia, arXiv:1303.3570 [hep-ph]
/
0.98 0.0 12
0.98 0.07
pm
p
11
2
2
( )
2
( )
2
2
t
t
Z
W
b
b
y
m
g hZZ
M
g hWW
M
y
m
y
m
10/06/2014 12
There is no other Higgs
10/06/2014
„за теоретичното откритие на механизма, допринасящ за разбирането на произхода на масата на субатомните частици и който наскоро беше потвърден чрез откриването на предсказаната фундаментална частица от ATLAS и CMS експериментите на Големия Адронен Колайдер в ЦЕРН“
The Nobel Prize in Physics 2013 was awarded jointly to François Englert and Peter W. Higgs "for the theoretical discovery of a mechanism that contributes to our understanding of the origin of mass of subatomic particles, and which recently was confirmed through the discovery of the predicted fundamental particle, by the ATLAS and CMS experiments at CERN's Large Hadron Collider"
13
10/06/2014 14
10/06/2014
Elementary Particles and Interactions of the Standard Model
2
4 params
| | ( ) 2 params
Y 13 params
SM
i ij j
D F F
D V
L
15
10/06/2014
Standard Model Extrapolationto the Planck Energy
D. Buttazzo, G. Degrassi, P.P. Giardino, G.F. Giudicе, F. Sala, A. Salvio, A. StrumiaarXiv:1307.3536 [hep-ph]
Figure from Giardino’s slides
16
10/06/2014 17
MW and mt precise measurements
CDF and D0 Collaborations,Phys. Rev. D 88 (2013) 052018 (arXiv:1307.7627)
ATLAS, CDF, CMS and D0 CollaborationsarXiv:1403.4427 [hep-ex]
See, however, CMS-PAS-TOP-14-001:mtop = 172.22 ± 0.73 GeV
10/06/2014 18
SM predictions versus measurementsEffect of Higgs Mass Knowledge
http://gfitter.desy.de
10/06/2014 19
The Latest Measurementsof the Higgs Properties
No yet combination of CMS and ATLAS results with the full run 1 dataset: scheduled for Fall 2014
10/06/2014 20
Tight Higgs Width Constraint!CMS: arXiv:1405.3455
Impossible directly due to experimental resolution, but using idea byFabrizio Caola and Kirill Melnikov, Phys. Rev. D 88 (2013) 054024
2 2resonance (on-shell) production:
( ) ( ) in H f H in H f
H H
g gin H BR H f
2 2off-shell production: ( ) H in H fin f g g
Assuming presence of the SM interactions only:SM5.4 22 MeVH H
10/06/2014 21
No evidence yetfor H bb decay
Tevatron combination: Phys. Rev. D 88, 052014 (2013)
m = 1.6 ± 0.7
ATLAS-CONF-2013-079 CMS PAS HIG-13-012
10/06/2014 22
No H Zg decay signal yet
10/06/2014 23
No H mm decay signal yetATLAS-CONF-2013-010 CMS PAS HIG-13-007
CMS also has Upper Limiton Br(H→ee) < 0.0017(SM prediction is ~ 5*10-9)
stat syst
H
m 125.7 0.3 0.3 GeVm 0.6 GeVH
10/06/2014 24
Precise Higgs-Boson Mass Measurements
stat sys
stat sy
stat syst
H stat sys
t
st
t
m( ) 125.98 0.42 0.28 Gem 125.36 0.37 0.18 GeV
Vm( 4 ) 124.51 0.52 0.04 GeV
m 1.47 0.67 0.28 GeVH
HH
Considerable reduction of systematic uncertainties on individual measurements
Shown at LHCP last week for first time; paper to be submitted shortly
stat syst
H stat syst
m 125.55 0.31 0.23 GeVm 0.2 0.6 0.6 GeV
my estimation!
H
CMS-PAS-HIG-13-005
CMS-PAS-HIG-13-001 (March 2013)
CMS: Phys. Rev. D 89 (2014) 09207stat systm( 4 ) 125.6 0.4 0.2 GeVH
stat systm( ) 125.4 0.5 0.6 GeVH
25
Higgs Couplings Measurements ATLAS-CONF-2014-009 CMS-PAS-HIG-13-005
0.170.15
1.15 0.18
0.99
V
F
0.89 0.08
0.91 0.20V
F
0.150.13
0.150.12
1.08
1.19
g
0.84 0.11
0.97 0.18
g
10/06/2014
10/06/2014 26
Top-Pair Production at LHC
Strong collaboration between theoretical and experimental researchers10/06/2014 27
10/06/2014 28
Single Top Production at Tevatron
CDF: 0.96 0.09(stat+syst) 0.05(theory)
0.78 at 95% C.L.
D0:
0.79 at 95% C.L
tb
tb
tb
V
V
V
.
10/06/2014 29
Single-Top Production at LHC
t-channel s-channeltW
10/06/2014 30
10/06/2014 31Victor E. Bazterra
10/06/2014 32Victor E. Bazterra
10/06/2014 33
FR = -0.009 ± 0.006(stat.) ± 0.020(syst.),
10/06/2014 34
35
“Stairway to Heaven”
10/06/2014 36
Heavy Flavour Physicswill be discussed in Augusto Ceccucci talk
10/06/2014 37
Precision measurement of tau lepton mass by BESIII
arXiv:1405.1076 [hep-ex]
BESIII 0.100.131776.91 0.12 MeV [96 ppm]m
PDG 2012
0.510 998 928(11) MeV [21.5 ppb]
10 5.658 3715(35) MeV [33.1 ppb]
1776.82(16) MeV [90 ppm]
em
m
m
2
3
? ?
5( )( )
192
( ) ( ) ( )
F
F F F
G e mBr e
G e G e G
10/06/2014 38
MEG + → e + Phys. Rev. Lett. 110 (2013) 201801; arXiv:1303.0754
[hep-ex]
BR(+ → e+ ) < 5.7 10-13
*
* *2
2
2 221
2
2 3 1
5
3
2
34
5
3BR( )
32
3
32
(2.4 3.7) 10
i
i ei
e
W
e
i
W
U U
U
eM
M
m
m mU U U
MEG 2013
10/06/2014
Peculiarity of Neutrino Physics
t
c
u
b
s
d
tm
e
?n†
D h.c.jL
ij iRjL
y
L
TM
s2
eesaw
h.c.ij iR jRC
ym
+L
39
Mixing matrices in quark and lepton sectors
Cabibbo-Kobayashi-Maskawa
Pontecorvo-Maki-Nakagawa-Sakata
3 i
2
3 i 2
1 e
1
(1 e ) 1
ud us ub
CKM cd cs cb
td ts tb
d s b
u V V V
V c V V V
t V V V
'
'
'CKM
d d
s V s
b b
1
2
3
e
PMNSU
i
1 2 3
1 2 3 i i
1 2 3
1 2 3 i i
i i2 2
i i2 2
i i2 2
2 1 e
3 3 2
1 e 1 e 2 1
6 3 2
1
e e
e
e 1 e 2 1
6e
3
e
e2
e e e
PMNS
e U U U
U U UU
U U U
Wolfenstein parameterization
10/06/2014 40P. F. Harrison, D. H. Perkins and W. G. Scott, Phys. Lett. B 530 (2002) 167
4 2 2 0
3 1
R1 33
, , ; , , L LR
R RL L
uu d e
d e
ii
10/06/2014
Elementary Particles and Interactions of the Standard Theory
2
4 params
| | ( ) 2 params
Y 13 params
SM
i ij j
D F F
D V
L
41
n3n2n1 Lepton sector is least known:+9 parameters(5 known, 4 unknown)Neither electron neutrino, nor muon and tau neutrinos are real particles!
e 1 2 3
10/06/2014 42
OscillationsThe two necessary conditions for neutrino oscillations:
UPMNS is non-identity matrix: the flavour states are different from the mass states m1 m2 m3: non-degeneracy of the mass states
22 2 2
3 3 02
22* *3121
0 3 3 2 22 231 31
sin (1 ) sin sin (1 )( ) 4 8 cos( ) ( )
(1 ) (1 )
2 2, , arctan , .
4
e e
F ee e
V V VP U U
V V V
m L G N EmU U U U V
m E m
O
2 2 2 5 221 2 1
2 5 231
7.54(20) 10 eV
2.43(8) 10 eV
m m m
m
Oscillations!
10/06/2014 43
First indications of non-zero Ue3
and negative CP-phase d from T2K
Phys.Rev.Lett. 107 (2011) 041801arXiv:1106.2822 [hep-ex]
→ e Appearance!
PR
L 112 (
2014)
06180
2
arXiv:1405.3871
NH: 1.1
9
8
0% CL allo
IH: 0.91 0.0
0.15
wed interva s
8
l
new results
The T2K beam has restarted, including antineutrino test data.
10/06/2014 44
Ue3 = sin 13 e-i
2 22 2 4 2 231 21
13 13 12( ) 1 sin 2 sin cos sin 2 sin4 4e e
m L m LP
E E
e → e Disappearance
10/06/2014 45
10/06/2014 46
10/06/2014 47
Daya Bay sin2 213 fit from rate and energy spectra
Phys.Rev.Lett.112 (2014) 061801e-Print: arXiv: 1310.6732 [hep-ex]
2 0.00813 0.009
2 0.019 3 231 0.020
sin 2 0.090 ( 10 )
2.59 10 eVm
213
2 0.010 3 231 0.011
with 621 days of data:
sin 2 0.084 0.005 ( 17 )
2.44 10 eVm
Neutrino 2014
48
How burns the reactor?
10/06/2014 49
How burns the Sun?
pp-cycle >99% energy production
5 ν species
CNO-cycle <1% energy production
3 ν species
Neutrinos are produced in several reactions in both cycles
5050
,Borexino
Solar Neutrinos: the predicted spectrum
10/06/2014
10/06/2014 51
BorexinoarXiv:1308.0443
7
9 2 1
Be (862 keV)
9 2 1SSM
(4.43 0.22) 10 cm s
4.47(1 0.07) 10 cm s
10/06/2014 52
Accuracy determination ofmass differences and mixing angles
F. Capozzi, G.L. Fogli, E. Lisi, A. Marrone, D. Montanino, A. Palazzo
Phys. Rev. D89 (2014) 093018arXiv:1312.2878v2 [hep-ph] 5 May
2014
after Neutrino 2014 (June 2-7)
2 2 2 2 221 12 13 32 23 sin sin sin
3.2% 5.5% 8.3% 2.5% 13%
m m
2 2 2 2 221 12 13 32 23 sin sin sin
2.4% 4.2% 2.5% 1 6% 3%
m m
10/06/2014 53
2 22 2 2 2 1
sol 2 1 atm 3, .2
m mm m m
Neutrino Mass Spectrum
23 1
2
3
1
2 1
0.058 eV
2
ii
m m
m m
m
22 3
21 3
3
1
0.098
2
eV
2
ii
m m
m
m
m
10/06/2014 54
2
sensitive to effective Majorana
mass :
(0 )
ei ii
m U m
m
A M
Neutrinoless double beta (0nbb) decay
There are claims for 0νββ signal by Klapdor-Kleingrothaus et al.
0 76 0.37
0 76 0.44
251 2 0
251 2
.23
0.31
Phys. Lett. B 586 (2004) 198( Ge) 1.19 10 yr (4.2 )
(0.2 0.6) eV
Mod. Phys. Lett. A 21 (2006) 1547( Ge) 2.23 10 yr (7.2 )
(0.32 0.0
T
T
m
m
3) eV
GERDA CollaborationPhys. Rev. Lett. 111 (2013) 122503
0 76 251 2
0 251 2
( Ge) 2.1 10 yr @ 90%CLcombination of GERDA+HdM+IGEX:
3.0 10 yr @ 90%CL
T
T
10/06/2014 55
KamLAND-Zen and EXO-200 0 nbb 136Xe experiments
0 136 251 2 ( Xe) 1.1 10 yr
(0.19 0.45) eV
@ 90% CL
T
m
EXO-200, Nature (2014) doi:10.1038/nature13432KamLAND-Zen, Phys.
Rev. Lett. 110 (2013) 0625020 136 25
1 2 ( Xe) 1.9 10 yr
@ 90% CL
T
0 136 251 2 ( Xe) 3.4 10 yr
(0.
combined resul
12 0.25) eV
t
@ 90% L
:
C
T
m
GERDA combinedTheoretical and
experimental constraints in
the plane charted by the
0 nbb half-lives of 76Ge and 136Xe
56
The effective Majorana mass asa function of the lightest neutrino mass
0.05 eVT½~1027 y
10/06/2014
10/06/2014 57
10/06/2014 58
Evidence of non-zero lightest neutrino mass
Baryonic Oscillation Spectroscopic Survey (BOSS)
The 2.5-meter Sloan telescope in New Mexico
South Pole Telescope Sunyaev-Zel'dovich (SPT-SZ) survey
BOSS
SPT-SZ
combination
1 2
3
3
1 2
Quasi-Degenerate masses
NH0.105 0.025 eV
0.116 0.022 eV IH
0.105 0.025 eV0.116 0.022 eV
m mm
mm m
10/06/2014 59
Lattice Calculations
2
3
2 ( )
10 MeV
13
(250 M
0.7 M
eV)
eV
u d
u d
uu dd
uu dd
m m mF
m m
F
60
Hadron mass spectrum in lattice calculations
10/06/2014 61
The Standard Model of fundamental particles and their interactions is finally reconfirmed and it acquires the status of a complete theory of elementary particles. It is self-consistent and could work up to the Planck energies.
It is in good shape: Neither new particles nor any deviations beyond the Standard Model up to distances 2.510-18 cm have been found. This size is two order of magnitude smaller than the scale of the weak interactions.
In the next year we expect almost double increase of the collider energy and more deeper penetration into the secrets of Nature.
By 2022 it is expected to gather 10 times more data and by 2030 100 times more data than we have now and at almost twice higher collider energy.
Conclusions
10/06/2014 62
Thank you for your attention!