ch23 Flashcards
unified atomic mass units
One unified atomic mass unit (1u) is defined as being equal to one-twelfth of the mass of a carbon-12 atom. 1u is equal to 1.66 × 10−27kg
mass defect
difference between mass of nucleus and total mass of nucleons where nucleons are separated to infinity
binding energy
energy required to separate nucleons to infinity
Binding energy per nucleon
the total energy needed to completely separate all the nucleons in a nucleus divided by the number of nucleons in
the nucleus
nuclear fusion
two nuclei combine to form a single nucleus. it is initiated by very high temperature
nuclear fission
a single large nucleus divides to form smaller nuclei. it is initiated by neutrons bombardment
thermonuclear reactions
Reactions requiring conditions of extremely high temperature and pressure, similar to those found at the centre of the Sun
Radioactive decay
when unstable nuclei emit particles and/or electromagnetic radiation to become stable. it is a random process in that it cannot be predicted which nucleus will decay next. it is a spontaneous process because it is not affected by any external factors, such as temperature or pressure
decay curve
A graph, such as that seen in radioactive decay, that shows an exponential decrease – the value decreases by the same fraction over equal time intervals
decay constant λ
probability of decay per unit time
becquerels
Unit used to measure the activity of a radioactive source, where 1 becquerel is 1 decay per second.
activity
the number of nuclear decays occurring per unit time in aradioactive source
The half-life
time taken for the number of undecayed nuclei to be reduced to half its original number
activity equation
-dN/dt== λN
−λN
dN/dt
equation of N
N0e^−λt where N0 = the initial number of undecayed nuclei (when t = 0)
exponential decay
An exponential decrease – the value decreases by the same fraction over equal time intervals.
equation of A
A0 e^−λt where A0= is the initial activity
decay constant equation
0.693/t(1/2)
Isotopes of hydrogen have binding energies per nucleon of less than 3MeV.
Suggest why a nucleus of helium‑4 does not spontaneously break down to become nuclei of
hydrogen.
binding energy per nucleon is much greater M1
so would require a large amount of energy to separate the nucleons in helium
Suggest an explanation for any difference between the actual activity of the sample
shown in Fig. 12.1 and the curve you have drawn for the activity of isotope X.
(activity of sample is greater than activity of X so) there must be an additional source of activity C1
the decay product (of isotope X) is radioactive
The decay constant λF of nuclide F is very much larger than the decay constant λE of
nuclide E.
By reference to the half-life of nuclide F, explain why the number of nuclei of nuclide F in the
sample is always small.
half-life of F is much shorter than half-life of E B1
nuclei of F decay (almost) as soon as they are produced