fermi gas model - physics & astronomyphysics.valpo.edu/courses/p430/ppt/fgm.pdfheisenberg...

13
Fermi Gas Model

Upload: others

Post on 21-Jan-2021

5 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Fermi Gas Model - Physics & Astronomyphysics.valpo.edu/courses/p430/ppt/FGM.pdfHeisenberg Uncertainty Principle Identical conditions apply for the y, py, and z, pz--† dVps≡(dx⋅dpx)⋅(dy⋅dpy)⋅(dz⋅dpz)=h3

Fermi Gas Model

Page 2: Fermi Gas Model - Physics & Astronomyphysics.valpo.edu/courses/p430/ppt/FGM.pdfHeisenberg Uncertainty Principle Identical conditions apply for the y, py, and z, pz--† dVps≡(dx⋅dpx)⋅(dy⋅dpy)⋅(dz⋅dpz)=h3

Heisenberg Uncertainty Principle

dpx ⋅ dx ≥ h Æ dpx =hdx

px = px + dpx = px +hdx

Particle in dx will have a minimum uncertainty in px of dpx

dx

pxNext particle in dx will have a momentum px

Particles with px in dpx have minimum x-separation dx

dx ⋅ dpx = h

Page 3: Fermi Gas Model - Physics & Astronomyphysics.valpo.edu/courses/p430/ppt/FGM.pdfHeisenberg Uncertainty Principle Identical conditions apply for the y, py, and z, pz--† dVps≡(dx⋅dpx)⋅(dy⋅dpy)⋅(dz⋅dpz)=h3

Heisenberg Uncertainty PrincipleIdentical conditions apply for the y, py, and z, pz --

dVps ≡ dx ⋅ dpx( )⋅ dy ⋅ dpy( )⋅ dz ⋅ dpz( )= h3

dVps = dV ⋅dp3

Therefore, in a fully degenerate system of fermions,(i.e., all fermions in their lowest energy state),we have 1 particle in each 6-dimensionl volume --

Phase spacevolume

Momentumvolume

Spatialvolume

= •

Page 4: Fermi Gas Model - Physics & Astronomyphysics.valpo.edu/courses/p430/ppt/FGM.pdfHeisenberg Uncertainty Principle Identical conditions apply for the y, py, and z, pz--† dVps≡(dx⋅dpx)⋅(dy⋅dpy)⋅(dz⋅dpz)=h3

Heisenberg Uncertainty Principle

dN =dVps

h3

In some dVps the maximum number dN of unique quantumstates (fermions) is

px

pz

py

p

dN =dV ⋅ 4p p2dp

2p h( )3

Number of states in a shell in p-spacebetween p and p + dp

Only Heisenberg uncertainty principle; completely general

Page 5: Fermi Gas Model - Physics & Astronomyphysics.valpo.edu/courses/p430/ppt/FGM.pdfHeisenberg Uncertainty Principle Identical conditions apply for the y, py, and z, pz--† dVps≡(dx⋅dpx)⋅(dy⋅dpy)⋅(dz⋅dpz)=h3

FGM for the nucleusTreat protons & neutrons separatelyConsider a simple model for nucleus--

V (x) = 0 ; 0 < x < L V (x) = • ; x ≥ LV (y) = 0 ; 0 < y < L V (y) = • ; y ≥ LV (z) = 0 ; 0 < z < L V (z) = • ; z ≥ L

V = V (x) + V (y) + V (z)

-h2

2M—2y + Vy = Ey

y = jx (x) ⋅ jy (y) ⋅jz (z)

E = E x + E y + Ez

jx (x) =2L

sin nxL

Ê

Ë Á

ˆ

¯ ˜

E x =hp( )2

2ML2 nx2

Page 6: Fermi Gas Model - Physics & Astronomyphysics.valpo.edu/courses/p430/ppt/FGM.pdfHeisenberg Uncertainty Principle Identical conditions apply for the y, py, and z, pz--† dVps≡(dx⋅dpx)⋅(dy⋅dpy)⋅(dz⋅dpz)=h3

FGM for the nucleus

E = E x + E y + Ez

E =hp( )2

2ML2 nx2 + ny

2 + nz2( ) ni =1,2,3,⋅ ⋅ ⋅

Total energy eigenvalue

y = jx (x) ⋅ jy (y) ⋅jz (z)

jx (x) =2L

sin nxL

Ê

Ë Á

ˆ

¯ ˜

ynxnynzx,y,z( )

E x =hp( )2

2ML2 nx2

E x =px

2

2M Æ px =

hpL

nx

unique states

degenerateeigenvalues

Page 7: Fermi Gas Model - Physics & Astronomyphysics.valpo.edu/courses/p430/ppt/FGM.pdfHeisenberg Uncertainty Principle Identical conditions apply for the y, py, and z, pz--† dVps≡(dx⋅dpx)⋅(dy⋅dpy)⋅(dz⋅dpz)=h3

FGM for the nucleus

px =hpL

nx Æ p =hpL

Ê

Ë Á

ˆ

¯ ˜ nx

2 + ny2 + nz

2 = p nxnynz( )

ynxnynzx, y,z( )

unique states quantized momentum states

px

pz

py

p

px , px , px( ) =hpL

nx ,ny ,nz( )

px , px , px( )

dp3

dp3 =hL

Ê

Ë Á

ˆ

¯ ˜

3=

hpL

Ê

Ë Á

ˆ

¯ ˜

3

from Heisenberguncertainty relation

Page 8: Fermi Gas Model - Physics & Astronomyphysics.valpo.edu/courses/p430/ppt/FGM.pdfHeisenberg Uncertainty Principle Identical conditions apply for the y, py, and z, pz--† dVps≡(dx⋅dpx)⋅(dy⋅dpy)⋅(dz⋅dpz)=h3

FGM for the nucleus

\ All momentum states up to pF are filled (occupied)

px

pz

py

p

px , px , px( )

dp3

Assume extreme degeneracy Æ all low levels filled up to amaximum -- called the Fermi level (EF)

We want to estimate EF and pF for nuclei --

The number N of momentum states withinthe momentum-sphere up to pF is --

N =18

Ê

Ë Á

ˆ

¯ ˜

43

p pF3

dp3one p-state per dp3

1/8 of sphere because nx, ny, nz > 0

Page 9: Fermi Gas Model - Physics & Astronomyphysics.valpo.edu/courses/p430/ppt/FGM.pdfHeisenberg Uncertainty Principle Identical conditions apply for the y, py, and z, pz--† dVps≡(dx⋅dpx)⋅(dy⋅dpy)⋅(dz⋅dpz)=h3

FGM for the nucleus

N =18

Ê

Ë Á

ˆ

¯ ˜

43

p pF3

2ph

Ë Á

ˆ

¯ ˜ 3

N =18

Ê

Ë Á

ˆ

¯ ˜

22ph( )3

43

p pF3V

N = pV3

2MEFh2p 2

È

Î Í ˘

˚ ˙

3/2†

pF = 2MEF

L3 = V( )

EF =hp( )2

2M3NpV

È

Î Í ˘

˚ ˙

2 /3Fermi energy

(most energetic nucleon(s)

pF = h 3p 2( )1/3 N

Î Í ˘

˚ ˙

1/3Fermi momentum

(most energetic nucleon(s)

protonsN = Z

neutronsN = (A-Z)

2 spin states

N =18

Ê

Ë Á

ˆ

¯ ˜

43

p pF3

dp3

Page 10: Fermi Gas Model - Physics & Astronomyphysics.valpo.edu/courses/p430/ppt/FGM.pdfHeisenberg Uncertainty Principle Identical conditions apply for the y, py, and z, pz--† dVps≡(dx⋅dpx)⋅(dy⋅dpy)⋅(dz⋅dpz)=h3

FGM for the nucleus

pF = h 3p 2( )1/3 Z

Î Í ˘

˚ ˙

1/3

Protons Neutrons

pF = h 3p 2( )1/3 A - Z

Î Í ˘

˚ ˙

1/3

Assume Z = N

pF = h 3p 2( )1/3 A /2

Î Í ˘

˚ ˙

1/3

pF = h 3p 2( )1/3 A /2

Î Í ˘

˚ ˙

1/3

V =43

p R3

R = RoA1/3

V =43

p Ro3A = 4.18Ro

3A

pF =h

Ro

3p 2

2 ⋅ 4.18

Ê

Ë Á Á

ˆ

¯ ˜ ˜

1/3

Page 11: Fermi Gas Model - Physics & Astronomyphysics.valpo.edu/courses/p430/ppt/FGM.pdfHeisenberg Uncertainty Principle Identical conditions apply for the y, py, and z, pz--† dVps≡(dx⋅dpx)⋅(dy⋅dpy)⋅(dz⋅dpz)=h3

FGM for the nucleus

pF = h 3p 2( )1/3 Z

Î Í ˘

˚ ˙

1/3

Protons Neutrons

pF = h 3p 2( )1/3 A - Z

Î Í ˘

˚ ˙

1/3

Assume Z = N

pF =197Mev

Roc3p 2

2 ⋅ 4.18

Ê

Ë Á Á

ˆ

¯ ˜ ˜

1/3

=300Ro

MeV /c

pF = 231 MeV /c (Ro =1.3F)

EF =pF( )2

2M= 28 MeV

Page 12: Fermi Gas Model - Physics & Astronomyphysics.valpo.edu/courses/p430/ppt/FGM.pdfHeisenberg Uncertainty Principle Identical conditions apply for the y, py, and z, pz--† dVps≡(dx⋅dpx)⋅(dy⋅dpy)⋅(dz⋅dpz)=h3

FGM potential

Page 13: Fermi Gas Model - Physics & Astronomyphysics.valpo.edu/courses/p430/ppt/FGM.pdfHeisenberg Uncertainty Principle Identical conditions apply for the y, py, and z, pz--† dVps≡(dx⋅dpx)⋅(dy⋅dpy)⋅(dz⋅dpz)=h3

Test ofFGM

not FGM