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Phy 102: Fundamentals of Physics II
Chapter 33: The Atomic Nucleus & Radioactivity
Lecture Notes
Wilhem Rontgen(1845-1923)
• German physicist• Discovered x-rays &
studied ability of x-rays to penetrate solid materials
• Refused to file patents for his work on x-ray devices
• Winner of the 1st Nobel Prize in Physics (1901)
X-ray micrograph of Mrs. Roentgen’s hand (1895)
• First woman to win the Nobel Prize• Won 2 Nobel Prizes
– Physics (1903): the discovery of polonium and radium– Chemistry (1911): the isolation of radium and the study of its
chemical properties
• Some of her contributions:– Discovered radium and polonium– Studied the properties of radioactivity– During WWI proposed the use of x-rays to locate bullets and
facilitate surgery– Invented x-ray vans
• Died from leukemia (thought to be due to radiation exposure)
Marie Curie (1867-1934)
Types of RadiationAlpha particles ():
– Helium nuclei– positive charge– Occurs when the nucleus of an atom ejects 2 protons & 2 neutrons (the identity of the
atom changes!)
Beta particles (): – Electrons– Negative charge– Usually occurs when a neutron transmutes to a proton (the identity of the atom changes!)
Gamma rays (): – High frequency electromagnetic (X ray) radiation (e.g. light)– No charge– Usually occurs when an “excited” nucleus “relaxes” to a lower state (the identity of the
atom does not change!)
Isotopes & Radioactivity• Isotopes are atoms of the same element that have different
numbers of neutrons (& different masses)• The skinny:
– Two fundamental forces involved: Electric and Strong force– Electric force acts over longer distances than Strong force– Protons repel each other (Electric force)– Protons and neutrons attract each other (Strong force)– The more nucleons that are in the nucleus the greater the distance of
separation between protons– At some point, the electric force repels the nucleons and the Strong
force cannot balance it out• The nucleus is susceptible to nuclear decay
Half-Life
• The nuclei of “radioactive” isotopes are unstable and inevitably decay to produce smaller nuclei (and some nuclear radiation)
• The half life (t1/2) of an isotope is the time it will take an isotope sample to decay to ½ of its original value
Examples:t1/2 for 3H is 12.43 years
t1/2 for 235U is 704 million years
t1/2 for 14C is 5730 years
Decay of 1000 Tritium Atoms
0
200
400
600
800
1000
1200
0 10 20 30 40 50 60time (years)
#o
f T
riti
um
ato
ms
The Nuclear Decay for Tritium
1 half-life
2 half-lives3 half-lives
Transmutation of Elements
• When radioactive isotopes decay they become different elements. This process is called transmutation.
Example 1: Decay of 14C to 14N14C 14N + {this is a beta decay}
Example 2: Decay of 241Am to 237Np241Am 237Np + {this is an alpha decay}
Enrico Fermi (1901-1954)• Italian-American physicist• Early work was theoretical
– Explained the statistics of nuclear particles that obey the Pauli Exclusion Principle (now called Fermions)
• Discovered artificial radioactivity– produced by bombarding elements with neutrons– Performed 1st successful transmutation
experiments
• Discovered the “chain-reaction”• A project leader & important contributor on
the “Manhattan Project”
Carbon Dating• 14C is produced in the upper atmosphere as 14N is bombarded by
cosmic rays• The 14C drops to the earth where it is absorbed by plants and animals• The 14C levels in an organism are constant throughout the
organism’s life (since it continuously adds and removes 14C through nutrition & respiration)
– There is one 14C atom for every trillion 12C atoms
1 carbon-14 : 1 x 1012 carbon-12• When an organism dies it can no longer replenish its 14C levels &
the 14C begins to decay (remember, t1/2 for 14C is 5730 years)
• Radioactivity levels of 14C are measured & the level of decay from the original value is used to estimate the organism’s age