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Brief History of Nuclear Physics

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Brief History of Nuclear Physics 1896 - Henri Becquerel (1852-1908) discovered radioactivity 1911 - Ernest Rutherford (1871-1937), Hanz Geiger (1882-1945) and Ernest ... – PowerPoint PPT presentation

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Title: Brief History of Nuclear Physics


1
Brief History of Nuclear Physics
1896 - Henri Becquerel (1852-1908) discovered
radioactivity
1911 - Ernest Rutherford (1871-1937), Hanz Geiger
(1882-1945) and Ernest Marsden (1888-1970)
conducted scattering of alpha particles on nuclei
1930 - John D. Cocroft (1897-1967) and Ernest
T.S. Walton (1903-1995) conducted the first
artificial nuclear reaction
1932 - James Chadwick (1891-1974) discovered the
neutron
1933 - Frederick Joliot (1900-1958) and Irene
Joliot-Curie (1897-1956) synthesized artificial
elements
1938 - discovery of nuclear fission by Otto Hahn
(1879-1968) and Fritz Strassman (1902-1980)
1942 - Enrico Fermi (1901-1954) builds a fission
reactor
2
Properties of nuclei
Mass Number A
- number of nuclei
- number of protons (charge, element)
Atomic Number Z
Neutron Number N
- number of neutrons
A
X
A nucleus is represented by symbol
Z
Elements with different numbers of neutrons are
called isotopes.
3
relativistic energy relativistic momentum
relativistic mass
relativistic energy
relativistic momentum
energy momentum relation
4
attributes of selected particles
proton 1.67262?10-27 1.007276 938.28 e ½
neutron 1.67493?10-27 1.008665 939.57 0 ½
electron 9.1094 ?10-31 0.0005486 0.510999 -e ½
positron 9.1094 ?10-31 0.0005486 0.510999 e ½
photon 0 0 0 0 0
neutrino 0 0 0 0 ½
5
the spin
Spin angular momentum like quantity
responsible for the magnetic moment of particles.
z
quantum numbers
  • spin quantum number I

- the magnitude of the spin is
  • magnetic quantum number mI -I, . I

- the z component of the spin is
6
Nucleus size and shape
Rutherfords experiment
m
Ze
2e
d
7
Nuclear Stability
Coulomb interaction - repulsive
Nuclear interaction - attractive
line of stability
magic numbers (very stable nuclei)
Z, N 2, 8, 20,
8
Binding Energy
The total (relativistic) energy of a nucleus is
always less than the combined energy of the
separated nucleons.
The difference Eb (MeV) ( Zmp Zmn - MA )
931.491 MeV/a.u. is called the binding energy of
the nucleus.
Example (alpha particle)
Eb (2 1.0073au 2 1.0087au 4.0026au)
931.491 MeV/au ? 27.4 MeV
9
Fission and Fusion
Fission heavy nuclei (Agt60) split releasing
energy
Fusion light nuclei (Alt60) combine releasing
energy
10
Radioactivity
- spontaneous emission of radiation resulting
from disintegration (decay) of unstable nuclei.
Types of radioactive decay
lead shield
photographic plate
11
Activity the decay rate
The number of disintegrated nuclei in a unit time
is proportional to the number of radioactive
nuclei in the source.
? the decay constant
Hence
N0 initial number of radioactive nuclei
Activity
R0 initial activity
units
1Ci 3.7 1010 Bq (curie)
12
Half life time
The decay constant can be expressed in terms of
time T½, in which activity (the number of
radioactive nuclei) decreases by a factor of two.
t
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