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Nuclear Physics Micro-world Macro- world Lecture 16

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Nuclear Physics. Micro-world Macro-world Lecture 16. Neutron. By 1930, the charge and masses of many different nuclei were known. The charges were found to be Q nucleus = Z x proton charge & the masses were M nucleus = A x proton mass Z is always an integer - PowerPoint PPT Presentation

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Page 1: Nuclear Physics

Nuclear Physics

Micro-world Macro-world

Lecture 16

Page 2: Nuclear Physics

Neutron

By 1930, the charge and masses of many differentnuclei were known. The charges were found to be Qnucleus = Z x proton charge & the masses wereMnucleus = A x proton mass

Z is always an integer A is nearly an integer

But, except for hydrogen where A=Z=1,A & Z are different.

Page 3: Nuclear Physics

Electrons in the nucleus?

One idea was that the nucleus contained A protonsand A-Z electrons.

But Heisenberg’s uncertainty principle forbids this:

Suppose x= 1x10-14m typical size of a nucleus

px > 6.6x10-34Js1x10-14m

= 6.6x10-28kgm/s

vx > px me

6.6x10-28Js9x10-31kg

= >speed of light

non-relativistic calculationis invalid

Correct calculation gives Eelectron > 2x106 eV,such electrons would not stay inside a nucleus

Page 4: Nuclear Physics

Discovery of the neutron

James Chadwick

Po

Be

n detector

detectorsource

No electric charge; mass ≈ proton mass

Page 5: Nuclear Physics

Nucleons (protons & neutrons)

proton neutron

mass 1.672x10-27kg 1.675x10-27kg

mc2 938.27 MeV 939.57 MeV

Charge +1.6x10-19 C 0

+

Page 6: Nuclear Physics

Isotopes

Same chemistry; very different nuclear physics

Page 7: Nuclear Physics

Light isotopes

AX

Chemical symbol

A = number ofprotons + neutrons

ZZ=# of protons

Page 8: Nuclear Physics

All elements have isotopes

238

92U

235

92U

Page 9: Nuclear Physics

Nuclear force

++

The very powerful electrical repulsion (100’s of Newtons)

must be counteractedby some other verystrong attractive

force

This new force is called the Strong Nuclear force

Page 10: Nuclear Physics

Strong Nuclear force

Forc

e

Distance (x10-15m) 1.0 2.0 3.0 4.0 5.0

Attractive nuclear force

repulsive electrical force

attraction isstronger here

repulsion isstronger here

Page 11: Nuclear Physics

Strong Nuclear Force

• It is very strong– It overcomes the electrical

repulsion between positively charged protons that are only 10-

15m apart.

• It acts over a very short range– It is not felt by nucleons when they

are more than 10-15m apart.

• It is selective– It is felt by neutrons & protons, but

not by electrons

Page 12: Nuclear Physics

Nuclei can’t be too large

+++

++

+

+

+

+

+

+

++

++

A proton feelselectrical repulsionfrom every protonin the nucleus

It feels a Strong Nuclearattraction only to nearby nucleons

In larger nuclei, the electricalforce is bigger while the nuclear force stays the same.

There are no stable nuclei above Z=82 (Lead)

+

+

++

++

+++

Eventually, the electrical repulsionoverwhelms the nuclear attraction

Page 13: Nuclear Physics

Discovery of radioactivity

Page 14: Nuclear Physics

Different types of radiation

Marie Curie

---

+++

neutral

- charged

+ charged

Page 15: Nuclear Physics

decayZY Z-2X + 2A A-4 4

Page 16: Nuclear Physics

Conservation of energy in decay

ZY Z-2X + 2A A-4 4

parent daughters

Energy of parent= Energy of daughters

Page 17: Nuclear Physics

Conserv. of energy in decay

ZY Z-2X + 2A A-4 4

parent daughters

v

= MXc2 + Mc2 + KEMYc2KE = MYc2 - MXc2 - Mc2

Page 18: Nuclear Physics

Energy balancepar

ent d

aughte

rs

the mass difference,times c2, becomes KE

Page 19: Nuclear Physics

KE = Mparentc2 – (Mdaughters c2)

-particle Kinetic Energy

Some mass is changed into Kinetic Energy

All the a particles havethe same Kinetic Energy

Page 20: Nuclear Physics

ZY Z+1X + e-A A

n p + e-

Beta () decay

+ e-

6C147N14

+

++

+

++ +

++

+

+

++7p

7n6p8n

Page 21: Nuclear Physics

88Ra 89Ac + e-228 228

Other beta decays

Page 22: Nuclear Physics

1H 2He + e-3 3

Tritium Beta decay

+ e-

3H 3He+ +

+

Page 23: Nuclear Physics

Energy balance in beta decay

14C160 keV

14N+e-

1 keV = 1000 eV

Page 24: Nuclear Physics

Electron energy in 14C beta decay

160 keV KEe-

KEe-

None of the electrons have160 keV of kinetic energy they all have less than that amount

What has happened to the “missing” energy??

Page 25: Nuclear Physics

Pauli’s “desperate solution”

no chargeno mass

Another “unseen” particle isemitted in decay process

Page 26: Nuclear Physics

6C 7N + e- + 14 14

14C decay revisited

e-6C14

7N14

Page 27: Nuclear Physics

1H 2He + e- + 3 3

3H decay revisited

e-3H 3He

Page 28: Nuclear Physics

Energy balance in beta decay

parent KEe- + KE

daughters

Page 29: Nuclear Physics

Cosmic gallNEUTRINOS, they are very small. They have no charge and have no mass And do not interact at all. The earth is just a silly ball To them, through which they simply pass, Like dustmaids down a drafty hall Or photons through a sheet of glass. They snub the most exquisite gas, Ignore the most substantial wall, Cold shoulder steel and sounding brass, Insult the stallion in his stall, And scorning barriers of class, Infiltrate you and me! Like tall and painless guillotines, they fall Down through our heads into the grass. At night, they enter at Nepal and pierce the lover and his lass From underneath the bed-you call It wonderful; I call it crass.

John Updike

Page 30: Nuclear Physics

Radioactive half-life

N = N0 ( ½ )n

Number ofremaining atoms

Initial numberof atoms number

of halflives

Page 31: Nuclear Physics

Some half-lives

3H (3He + e- + ) 12.3 yrs14C(14N + e- +) 5730 yrs238U(234Th +) 4.5x109 yrs235U(231Th + ) 7.1x108 yrs226Ra(222Rn + ) 1600 yrs28Mg(28Al + e- + ) 21 hrs213Po(209Pb + ) 4x10-6 s

T1/2

Page 32: Nuclear Physics

Carbon-14 dating

Page 33: Nuclear Physics

14C content

Page 34: Nuclear Physics

Shroud of Turin