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Precision Measurements Precision Measurements

Precision Measurements - PowerPoint Presentation

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Precision Measurements - PPT Presentation

after the Higgs Discovery MV Chizhov Sofia University Bulgaria and JINR Russia 09062014 2 Why do we need the Higgs boson S ½ S 1 S 0 09062014 Harmonic Oscillator Analytical ID: 583150

higgs 2014 goldstone 1964 2014 higgs 1964 goldstone phys rev scalar model mass particles symmetry salam mechanism boson yang 1961 potential standard

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Slide1

Precision Measurementsafter the Higgs Discovery

M.V. ChizhovSofia University, Bulgaria and JINR, RussiaSlide2

09/06/20142

Why do we need the Higgs boson?

S = ½

S = 1

S = 0Slide3

09/06/2014Harmonic Oscillator

(Analytical Mechanics)

Joseph-Louis Lagrange

(

Giuseppe Lodovico

Lagrangia)

, 1788

3Slide4

R

> 0

R

< 0

09/06/2014

Harmonic

Oscillator

(Scalar

F

ield)

4Slide5

09/06/2014Scalar Potential of Anharmonic

Oscillator

5Slide6

09/06/2014Discrete Z2

Symmetry of

t

he Scalar Potential

6Slide7

Two Scalar Fields

(

or Complex

S

calar

F

ield

)

Potential with Broken

S

ymmetry

7Slide8

09/06/2014Continuous U(1) Symmetry of

the Potential with Complex Scalar Field

J. Goldstone, Nuovo Cim. 19 (1961) 154.

8Slide9

09/06/2014

Goldstone Particle (Theorem)

“if

there is continuous symmetry transformation under which the

Lagrangian

is

invariant

, then either the vacuum state is also invariant under the transformation,

or

there must exist

spinless

particles of zero mass

.”

Jeffrey Goldstone, Abdus

Salam and Steven Weinberg, Phys. Rev. 127 (1962) 965

9Slide10

09/06/2014

Examples of Collective Goldstone Bosons

Spin waves in a

ferromagnet

Phonons in a crystal lattice

Superfluidity

(Bose condensate

, Боголюбов,1947)

Superconductivity

(

Cooper pairs

, 1956

;

Боголюбов,1958)

Pions in the chiral limit (Nambu, 1961)

10Slide11

09/06/2014In Nature there is not a massless spinless

colorless particle, which would have had an infinite radius of interaction!

Only gravitational and electromagnetic forces have

an

infinite radius

of interaction.

Massless Particles in Nature

11Slide12

09/06/2014

Gauge Invariance

a

nd Massless Particles

A

m

12Slide13

09/06/201413

As Yang relates: Wolfgang

Pauli (1900-1958) was spending

the

year in Princeton, and was deeply

interested

in symmetries and interactions....

Soon

after my seminar began, when I

had

written

on the blackboard,

(∂m

-iBm

)

Pauli asked, "

What is the mass of this field

B

m

?

" I said we did not know. Then I resumed my presentation but soon

Pauli asked the same question again

.

I said something to the effect that it was a very complicated problem, we had worked on it and had come to no definite conclusions. I still remember his repartee: "That is not sufficient excuse".

An Anecdote by C. N. Yang Slide14

09/06/2014S. L. Glashow, Nucl. Phys. 22 (1961) 579.

Birth of the Standard Model of

Elementary Particles

SU(2)

L

U(1)

Y

“Schwinger told me to think about unifying weak and EM.

So I did it. For two years ‒ I thought about it.”

14Slide15

09/06/201415

Unitarity

and Z bosonSlide16

09/06/201416

Unitarity

and Higgs boson

Not yet tested experimentally… but see the following slide! Slide17

09/06/201417Evidence of electroweak W

±W±jj

production

ATLAS-CONF-2014-013 (March 25,

2014),

arXiv:1405.6241

Inclusive

m

jj

QCD+EW region

Enriched VBS region:

m

jj

>500

GeV

, |

D

y

jj

|>2.4Slide18

09/06/2014

Gauge Invariance

a

nd Massive

P

articles

Schwinger

model

(1962):

two-

dimentional

quantum electrodynamics

, where the photon becomes massive.

Non-relativistic dynamics of the plasma:

Philip

W.

Anderson

(

1963) –

Yang

Mills fields acquire the mass

due to longitudinal oscillations in plasma

(

Meissner

Ochsenfeld

effect

)

.

A

m

2

“We conclude

, then, that the Goldstone zero-mass

d

ifficulty is

not a serious one, because we can

probably

cancel

it off

against an equal Yang-Mills

zero-mass problem.”

18Slide19

F. Englert and R. Brout, Phys. Rev.

Lett. 13 (1964) 321 (June 26

, 1964)

P. W. Higgs, Phys. Rev.

Lett

. 13 (1964)

508

(

August

31, 1964)

G. S. Guralnik,

C. R. Hagen, and T.

W.

B.

Kibble

,

Phys

. Rev.

Lett

. 13 (1964)

585

(

Octomber

12, 1964)

Englert

-

Brout

-Higgs-

Guralnik

-Hagen-Kibble mechanism on one page

19Slide20

09/06/2014

Goldstone

and

Higgs

Particles

Jeffrey

Goldstone

Peter

W. Higgs

Phys.

Rev

. 145 (1966) 1156

H → Z Z

“it

is worth noting that an

essential feature of

this type

of

theory is the

prediction of

incomplete

multiplets

of

scalar

and vector bosons

.”

Phys.

Rev

.

Lett

. 13 (1964) 508

20Slide21

09/06/2014Neither Salam and Ward, who worked at Imperial College in the same group with Guralnik, Hagen and Kibble, nor Glashow, who after Higgs seminar at Harvard on March 16, 1966 said: "that is a nice model, Peter" have

realized that they could use this mechanism for generation of masses.

Omitted Opportunities

Glashow (1961)

Salam & Ward

(1964)

Salam & Ward

(

Sept

24

,

1964→

Nov 15,

1964)(On

Monday, October 5

, Peter

Higgs gave a seminar about his mechanism at Imperial

College

?

)

GHK

(Oct

12

,

1964 →

Nov

16

,

1964

)

“All

of us,

Brout

,

Englert

and myself, had been going in the

wrong direction, looking at hadron symmetries

.

P.W. Higgs

21Slide22

SU(2)

L

U(1)

Y

Using of EBHGHK mechanism

S. Weinberg

(1967)

& A. Salam (196

8

)

→ Nobel Prize

1979

relation

between the masses of

intermediate

bosons

M

W

=

M

Z

cos

W

through

the

mechanism

of

spontaneous symmetry

breaking

09/06/2014

22Slide23

Lagrangian

of

t

he Standard Model

09/06/2014

23Slide24

09/06/2014

Mathematical Foundation oft

he Standard Model

(

theory

)

G

. ’t

Hooft

&

M. J. G.

Veltman

(1972)

→ Nobel Prize

19

9

9

renormalizability

of non-abelian gauge theories with broken symmetry is proven

a drawing of their most important discovery

24Slide25

Discovery of the weak neutral interactions mediated by Z boson

in experiment with bubble chamber Gargamelle at CERN (1973)

Establishment of

t

he Standard Model

(

experiment

)

sin

2

W

~ 0.3

-

0.5

M

W

=50

-

70

GeV

M

Z

=75

-

80

GeV

09/06/2014

25Slide26

09/06/2014

Hunt for the Higgs Boson

26

John F.

Gunion

,

Howard E.

Haber,

Gordon

L.

Kane, Sally Dawson,

The

Higgs Hunter's

Guide,

Upton,

NY:

Brookhaven

Nat. Lab., 1989. - 404 p.Slide27

09/06/2014began work on November 30, 1986 and

stopped on September 30, 2011

TeVatron

at FNAL

27Slide28

09/06/201428

Tevatron Higgs ExclusionSlide29

09/06/2014

Large

Electron

Positron

(

LEP) collider

at CERN

started in August 1989 and ended in late 2000

DELPHI

L3

ALEPH

OPAL

29Slide30

09/06/201430

Direct LEP exclusionSlide31

09/06/201431

Indirect constraints on Higgs massSlide32

Large Hadron Collider (LHC)

09/06/2014

32

10

9

interactions

per second

1.5

10

11

p

2

1380 bunchesSlide33

09/06/2014

July 4, 201233Slide34

09/06/201434Is it the Higgs, or isn’t Higgs?