/
Standard Model Standard Model

Standard Model - PowerPoint Presentation

alida-meadow
alida-meadow . @alida-meadow
Follow
404 views
Uploaded On 2016-09-05

Standard Model - PPT Presentation

Lagrangian with ElectroWeak Unification The Standard Model assumes that the mass of the neutrino is zero and that it is left handed travelling with its spin pointing opposite to its direction ID: 461228

helicity neutrino left interactions neutrino helicity interactions left model lagrangian standard photon mass weak interaction spin density handed sum

Share:

Link:

Embed:

Download Presentation from below link

Download Presentation The PPT/PDF document "Standard Model" is the property of its rightful owner. Permission is granted to download and print the materials on this web site for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.


Presentation Transcript

Slide1

Standard Model Lagrangianwith Electro-Weak Unification

The Standard Model assumes that the mass of the neutrino is zero and that

it is “left handed” -- travelling with its spin pointing opposite to its direction

of motion.

Since in this case there would be no “right handed” neutrino, the “flavor”

partner of the neutrino must be a “left handed” electron. This changes

the structure of the Standard Model

Lagrangian

– which is assumed to treat

only left handed flavor doublets.Slide2

The spinor for the

neutrino

is the same as for the

electron,if one substitutes m = 0 :

neutrino

spinorSlide3

The helicity operator,

p

, satisfies the following condition

So when acting on the

spinor

It’s a projection!

2

= u

u

1Slide4

left hand side gives

(p) (p)/

pp

= 1 (

2x2 unit matrix

)

1

From this we can determine conditions on a and bSlide5

So, we have the following condition on a and b:Slide6

These are the only

spinors

allowed for a zero mass neutrino!

positive

helicity

negative

helicity

The neutrino, if it has a zero mass can only have its spin

pointing along (or opposite to) it’s momentum.Slide7

Non-conservation of parity: Wu 1957

J

J-1Slide8

number of

electrons

e

JSlide9

The neutrino could have both values of helicity, and Wu’s experiment, while confirming non conservation of parity (left-right symmetry broken), did not conclusively determine the neutrino’s helicity

.

In 1958

Goldhaber determined the helicity of the neutrino in the K capture of an electron:

63Eu152 (J=0) 62Sm*

152 (J=1) + . The Sm* decays giving off a photon with the same

helicity

as the neutrino.

Goldhaber

measured the

helicity

of the photon by passing it through magnetized iron. If the photon has the same direction of spin as the magnetized iron, it would pass through, otherwise it would produce a spin flip. He reported a

helicity

of -1.

Helicity of the neutrino: Goldhaber

1958Since 1998 it has been accepted that the neutrino has a small mass. This produces some corrections in the Standard Model. For this

description of the Standard Model, it is assumed that the neutrino has no mass. Slide10

Each term in the SM

Lagrangian

density containing quarks and the leptons can be rewritten using the following expression. For

the neutrinos, however, only the left handed term exists.

In the following slide we use the notation d R

= dRSlide11

The Lagrangian density withthe U(1), SU(2) and SU(3)gauge particle interactions

neutral vector boson

heavy vectors bosons (W

, W

3

)

8 gluons

YSlide12

The following is the interaction Lagrangian density for the first generation of particles with the left and right handed parts shown explicitly.

B

B

B

B

B

B

W

1

W

1

W

2

+

W

2

+

W

3

W

3

a

G

a

sum over a = 1,2,…8

a

G

a

B

Sum over all leptons and quarks interacting

with

B

Sum over all left handed leptons and quarks interacting

with W

Sum over all quarks interacting

with

G

a

Slide13

Weinberg’s decomposition of the B and W

:

sin

2

W  0.23

-- to be determined experimentally!

W

= Weinberg angleSlide14

Next steps: rewriting interaction

Lagrangian

density so

that interactions with the photon are identified.

The neutrino has zero charge and can’t interact with the photon.

1.

2

.

3

.Slide15

After substituting the expressions for B and W0 (which takes some work),one can identify factors which equal e, the electronic charge, or the up quark charge, etc. This permits one to find relationships between

sin

W

, cos 

W , e, g

2

and

g

1

.

One finds that:

g

2 = e /

sinW

g 1 =

e / cosW

Y

L

= -1

Y

R

= 2 Y

L

Also one defines:

T

3

f

= + 1/2

for the

u

L

= -

1/2

for the

d

L

=

0 for

u

R

=

0 for

d

R

Slide16

(E & M) QED interactions

weak neutral current interactions

weak flavor changing interactions

QCD color interactions

+

+

The Standard Model Interaction

Lagrangian

for the 1

st

generationSlide17

The U(1) and SU(2) interaction terms

A

Z

+

Z

W

+

W

-

weak

neutral current interactions

(E & M)

QED

interactions

weak

flavor changing interactions

g

2

g

2

e

g

2

=

e

/

sin

W