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71 Cards in this Set

  • Front
  • Back

Nucleon

A constituent particle of the atomic nucleus, either a neutron or proton

Nuclide

A species of an atom characterized by the constitution of its nucleus

Isotope

Nucleus which have the same number of protons but different number of neutrons


any nucleus that have the same atomic number but different atomic mass numbers

Mass energy equivalence

Mass and energy are interchangeable


Mass May be transformed to energy and vice versa

Pair annihilation

Two particles with mass specifically a positron and a electron collide and are transformed into two rays of electromagnetic energy

Mass defect

The total mass of the atom is less than the sum of the masses of the individual proton and neutron

Binding energy

The energy equivalent of mass defect

Binding energy per nucleon

Binding energy divided by the total number of nucleons in the nucleus

Fission

The splitting of the nucleus into at least two smaller nuclei with an accompanying release of energy

Criticality

The condition in which the neutrons produced by fission are equal to the number of neutrons in a previous generation


Neutrons in one generation go on to produce an equal number of fission event

Fusion

The act of combining or fusing two or more atomic nuclei


The process of fusing nuclei into a larger nucleus with an accompanying release of energy

4 sources of background radiation

Terrestrial


Internal emitters


Cosmic


Inhaled radionuclides

Origin, Radionuclides, variables an contribution to exposure of terrestrial radiation

Found in soil and rock


Uranium and thorium


18 mrem a year

Origin, Radionuclides, variables an contribution to exposure of cosmic radiation

Primary Galactic Cosmic rays and secondary Solar Cosmic rays


Decreases with latitude and increases with altitude


30mrem a year

Origin, Radionuclides, variables an contribution to exposure of internal emitters

Intake and ingestion from the food chain


K40, Rb87, Ra226, U238, Po210, and C14


30mrem a year

Origin, Radionuclides, variables an contribution to exposure of inhaled radionuclides

Inhaled through air


Radon and Thoron


<1 mrem a year

The four artificially produced radiation

Nuclear fallout


Medical exposure


Consumer products


Nuclear facilities

Magnitude of dose received from Nuclear fall out

Debris that settles to the earth as a result of nuclear blast


<1 mrem a year

Magnitude of dose received from Medical exposures

Diagnostic x-rays: Radiography, fluoroscopic, and photo fluoroscopic


Medical radionuclides: nuclear medicine


300 mrem a year


Magnitude of dose received from Consumer products

Tv, microwaves, smoke-alarms, watches


12mrem year

Magnitude of dose received from Nuclear Facilities

<1 mrem a year

Nuclear stability

Governed by the particular combination and arrangement of neutrons and protons in a given nucleus

Three forces acting in the nucleus

Gravitational


electrostatic


nuclear force

Gravitational

Negligible attractive force between all nucleons


Relatively long

Electrostatic

Strong repulsive Force between like charged particles


Relatively long

Nuclear force

Strong attractive force between all nucleons


extremely short

How is the neutron to proton ratio related to nuclear stability

In a stable atom there is a balance between attractive and repulsive forces in the nucleus if the forces do not balance out that item cannot be stable

Radioactivity

The property of certain nuclides of spontaneously Imitating energy from the nucleus in the form of particles and packets of electromagnetic waves

Radioactive decay

The process by which a nucleus spontaneously disintegrates or is transformed by one or more discrete energy steps until a stable state is reached

Alpha decay

Two protons and two neutrons


4 atomic mass units


Electric charge of +2

Beta minus decay

A nuclide that has an excessive number of neutrons will usually decay by changing a neutron into a proton through an emission of negatively charged particle


High neutron to proton ratio

Positron decay

Low neutron to proton ratio

Electron capture

Low neutron to proton ratio

Gamma

Electromagnetic radiation


it is energy photon

For unique aspects associated with the decay of radioactive nuclide

Modes of decay


types of a emission


Energies of the mission involved


rate of decay

Artificial radioactivity

Man-made nuclear reactions


Produce radionuclides generally revert to stability in only a few decay steps


Activation and Fission products decay by Beta or positron a mission or by orbital electron capture

Why are fission products unstable

The nuclear fragments directly resulting from fission invariably have too large a proportion of neutrons to protons for stability and consequently tend to achieve stability by beta minus emissions

The three natural occurring radioactive families and the products of each

Uranium 238 series


thorium 232 series


uranium 235 actinium series


Decay to lead

Curie

That amount of radioactive material that will produce 3.7 e10 disintegrates per second

Becquerel

Quantity of a radioactive material in which one atom is transformed per second or undergoes one disintegration per second

Specific activity

The activity per Unit mass of a radioactive substance and is reported in units such as curies per gram CI/g or becquerels per kilogram BQ/KG

Half life

The time that is required for the activity present to be reduced to 1/2

Activity, time of decay and radiological half-life formula

At=a0e(1/2)t/t1/2

Exposure

The measure of the ability of photons to produce ionization in the Air


Roentegen

Absolute dose

Units of those measure the amount of radiation energy absorbed or deposited per unit of mass

Equivalent dose

Calculated as the absorbed dose multiplied by the quality factor which relates the relative risk from the type of radiation absorbed to the risk from the same dose of X or gamma radiation

Radiation weighting factor

The modifying factor used to calculate the equivalent dose from average tissue or organ absorbed dose


That absorb dose multiplied by the appropriate radiation weighting factor

Roentgen

Exposure

Rad

100 ergs of energy in one gram of any material

No equilibrium

The half-life of the parent is shorter than that of the daughter that you never reach a state of equilibrium

When two or more light nuclei combine to form a large nucleus in fusion this changes the

Binding wnergy

A neutron or proton in a nucleus may be called a

Nucleon

The total binding energy of a nucleus divided by the total number of nucleons in the nucleus is the

Binding energy per nucleon

The process in which two or more nuclei combine to form a larger nucleus is called

Fusion

The binding energy per nucleon is average energy which must be added in order to remove

A nucleon from a nucleus

The two elements who’s radionuclides are generally considered to be the greatest contributor of those equivalent from natural terrestrial background radiation sources are

Uranium


Thorium

The radionuclide generally considered to be the greatest contributor of dose from internal emitters as part of natural background radiation source is

Potassium 40

The average dose to the general population of the US from all combined medical exposures as part of man-made background radiation sources is approximately how many mrem a year

53

The factor which contributes the greatest variability in dose from natural terrestrial background radiation is

Geology

When two or more light nuclei combine to form a large nucleus in fusion this changes the

Binding energy

How many rems equal 1 Sievert

100 rem

Each radionuclide has unique qualities of

Rate of decay type and energy of decay

Which is an aspect associated with the radioactive decay of a specific radionuclide

Modes of decay

Rem

The quantity of ionizing radiation whose biological affect in man is equal to that produced by one roentgen of x-rays or gamma radiation the Dose equivalent in rem is numerically equal to that absorb those in rad multiplied by the quality factor


Rem = radxQ

Sievert

The SI the derived unit of dose equivalence equal to the absorbed dose in grays multiplied by the quality factor sievert= grayxQ


1Sv=100 rem

Parent

The nucleus before the decay or transformation

Daughter

The nucleus after the decay

Decay chain

The various steps from parent to daughter that trace to stability a series of transmutations from parent to stable daughter

Equilibrium

That amount of activity being produced is the same as amount that is decaying

Secular equilibrium

The half-life of the parent is very much longer than a half life of the daughter the majority of the activity will be contributed by the parentAs more of the parent nuclear decay is the amount of activity contributed by the daughter will increase when in equilibrium the activity of the daughter is equal to the activity of the parents

Transient equilibrium

The half-life of other parent is longer than that of the daughter but not very long in a freshly purified parent fraction the daughter activity build up then decays with the same rate of decay as the parent