Transcript Slide 1

16.451 Lecture 12: The neutron Particle Data Group entry: 14/10/2003 1 ???

• slightly heavier than the proton by 1.29 MeV

(otherwise very similar)

• electrically neutral (q/e < 10 -21 !!!) • spin = ½ • magnetic moment  = - 1.91  N

(should be zero if pointlike: Dirac)

• unstable, with a lifetime of about 15 minutes:

n

p

e

• accounts for a little more than half of all nuclear matter 

v e

Recall the nuclear “landscape” from lecture 1:

100 Heavy nuclei, N > Z

light nuclei have N  Z

0 0 neutron number, N 140

http://www.nscl.msu.edu/future/ria/science/toi.html

2

Neutron electric form factor: G e n

(from elastic electron scattering, etc.)

3 • difficult to measure! no free neutron target ... • recall the form factor expansion from lecture 8: (compare 1 H and (magnetic contribution dominates) 2 H, etc...) • very small contribution to total cross section, since net charge = 0

F

(

q

2 )    1  

i q

r

  ( 

q

r

 ) 2 / 2  ...

  (

r

)

d

3

r

 

q

2

r

2 6  ...

for

  (

r

)

d

3

r

 0 !

All the world’s data (2003): Positive slope implies negative !

G e n (0) = 0 Various quark model theories

What does negative mean?

r

2  

r

2  (

r

)

d

3

r

 

r

2 4 

r

2  (

r

)

dr

• charge density must have both –ve and +ve regions, since net charge = 0 • integral is weighted with r 2  more negative charge at large radius 4

Neutron magnetization distribution: about the same as the proton Neutron 5 Both plots show ratios to “dipole” fit:

G

D

  1 

Q

2 1 / 0 .

71 GeV 2 2  Proton Recall: G M (0) =  , i.e. the magnetic moment is the “magnetic charge” ...

Isospin and the nucleon:

(Krane, 11.3)

6 • the neutron and proton are very similar apart from a small mass difference (0.1%) and of course the difference in electric charge • both play an equally important role in determining the properties of nuclei • postulate that n,p are two “substates” of a “nucleon”, with “Isospin ½”, by analogy with ordinary spin s

(Heisenberg, 1932)

for spin, S:

s

  1 2 ,

s

2 

s

(

s

 1 ),

s z

m s

  1 2 e.g. electron: spin “up” and spin “down” states have different values of m s , but this is a trivial difference – both are electrons! for Isospin, T:

T

  1 2 ,

T

2 

T

(

T

 1 ),

T z

m t

  1 2 by convention, the proton has m

t

= + ½ , and the neutron has m

t

= - ½ ; these are two “substates” of the nucleon (N) with isospin T = ½ ! (PDG table uses I)

Nucleon states: 7

E

( MeV ) 939 .

6 938 .

3 Nucleon, N

m

t

  1 / 2 ,

neutron m

t

  1 / 2 ,

proton

• both neutrons and protons have spin S = ½ • S and T are independent quantum numbers • S is “real” in that it has classical analogs in mechanics (intrinsic angular momentum) and electrodynamics (magnetic moment)  = g s S  N • T has no classical analog; it is a quantum mechanical vector, literally “like spin” (iso = ‘like’), so it follows the same addition rules as S, L, J, etc...

• in this language, (n,p) are isospin-substates of the nucleon, N • as far as the strong interaction is concerned, = neutron from a proton

m

t

is all that distinguishes a

Why isospin?

8 • It turns out to be rather a lucky guess that isospin is a symmetry of the strong interaction: both m

t

and T are conserved in strong scattering and decay processes. • The electromagnetic interaction breaks isospin symmetry; i.e. it can distinguish between different values of m t  There is a simple relation between m t and electric charge for all hadrons, (particles made up of quarks, exhibiting strong interactions...)

Nucleon: N = (n,p)

 T = ½ isospin doublet, m

t

=  ½ electric charge (q/e) = m

t

+ ½ (mass ~ 940 MeV)

Delta:

(1232) = (  ++ ,  + ,  °,  ) T = 3 / 2 isospin quartet, m

t

= (

3

/

2

, ½, - ½ , -

3

/

2

)

 electric charge (q/e) = m

t

+ ½ (mass ~ 1232 MeV)

Pion or

-meson = (  + ,  °,  ) T = 1 isospin triplet, m

t

= (1, 0, -1)  electric charge (q/e) = m

t

(mass ~ 140 MeV )

Conservation Laws: A conserved quantity is the same before and after an interaction takes place, e.g.:     total energy linear momentum angular momentum (quantum vector) electric charge   parity isospin (exception: weak interaction) (strong interaction only) from classical mechanics quantum mechanics 9 Example:  resonance decay,  +  p +  ° in the  rest frame:  

M

“before”

p

o

“after” Total energy and momentum conservation:  M(  ) = m(p) + m(  ) + K(p) + K( 

p p

 

p

  0

what about the other quantities?

Adding angular momentum

(review: lecture 3, hydrogen atom...)

Whether we are adding “spin” or “orbital” or “total” angular momentum (s, same rules apply, so we will use “j” in the formalism here: Consider: 

j

1 

j

 2 

J

l

, j), the • the total angular momentum has quantum number

J

and z-projection

m J

• the z-projections add linearly:

m j

1 

m j

2 

m J

• the solutions for

J

must be consistent with a complete set of configurations which can be found by writing down all possibilities,

as in lecture 3, slide 11 m J ,

• this leads to the general rule:

J

 (

j

1 

j

2 ), (

j

1 

j

2  1 ) ...

| (

j

1 

j

2 ) | • an exact prescription is beyond the scope of this course, but it involves writing the quantum state |J,m J > as a linear superposition of configurations |j 1 ,m 1 ,j 2 ,m 2 >:

J

,

m J

m

1  ,

m

2

a

(

j

1 ,

m

1 ,

j

2 ,

m

2 ,

J

,

m J

)

j

1 ,

m

1 ,

j

2 ,

m

2

(The coefficients a(j 1 ,m 1 ...) are just numbers; they are called “Clebsch-Gordon” coefficients in advanced books on quantum mechanics.)

10

Application:  +  p +  ° (the quantum numbers have to add up!) 11   “before” Angular momentum: J = 3/2 Parity: + Isospin: T = 3/2, m

t

= ½

p

o

“after” Angular momentum: proton: s = ½ pion: s = 0 orbital:

L

 1 2  

L

J

L

 1 Parity: proton: + pion: orbital: (-1)

L

(  Isospin: proton: T = ½, m t pion: T = 1, m t = ½ = 0 )(  )(  1 )

L

T m

t

  ( 3 1 / /   2 2 , 1 / 2 ) All the conservation laws are observed. Reaction proceeds in the “T=3/2 channel”

Isospin and quarks: There are a total of 6 quarks in the Standard Model (u,d,s,c,t,b – more later!) only two play a significant role in nuclear physics: u and d.

but Not surprisingly, isospin carries over into the quark description: the “up” quark has isospin T = ½ “up” and similarly for the “down” quark: Quark “flavor” u (“up”) Spin, s 1/2 Charge, q/e + 2/3 Isospin projection, 1/2

m

t

12 d (“down”) 1/2 - 1/3 -1/2 Isospin addition for the proton: p = (uud), m

t

neutron: n = (udd), m

t

= ½ + ½ - ½ = ½  = ½ - ½ - ½ = - ½  What about the delta? Addition of 3 x isospin- ½ vectors: T = 1/2 or 3/2; T = 3/2 is the  :  ++ = (uuu),  + = (uud),  ° = (udd),  = (ddd)  What about antiquarks? same isospin but opposite m

t

 e.g. pion: (  + ,  °,  )   

u d

,

m t

 1 2  1 2   1 ,

etc

...