NUCLEAR INSTABILITY Flashcards
(19 cards)
what are the four reasons nucleis will be unstable
- too many protons
- too many neutrons
- too many nucleons
- too much energy
what emmision do neutron rich nuclei under go
beta minus emission
n > p
what emissions do proton rich nuclei undergo
beta plus and electron capture
p > n
what emissions do nuclei with too many nucleons undergo
alpha decay
what is the imbalance of stability of a nucleus
- nucleus is bound together by SNF
- more protons causes more electrostatic repulsion
- more neutrons are needed to balance this
- neutrons dont repel, they add to SNF
what is meant by a metastable nucleus
- nucleus that exists in a particularly stable excited state
on an N - Z graph which direction is arrow of beta minus
south - east
N - 1
Z + 1
on an N - Z graph what direction is beta plus and electron capture
north - west
N+1
Z-1
on an N - Z graph what direction is alpha decay
south - west
N - 2
Z - 2
for a beta minus energy diagram how can we determine
1. max KE
2. number of lambdas possible
3. longest lambda
- Eoriginal - Elargest energy gap
- count the possible outcomes
- shortest energy gap
in closest approach how do we calculate the radius
Ek = Electric potential energy
r = Qq / 4pieoEk
what are advantages of closest approach
- gives a good estimate to upper limit of radius
- alpha particles are only scatted by protons
what are disadvantages of closest approach
- will always be an overestimate, measures seperation not radius
- alpha particles contain hadrons which are affected by SNF
what is electron scattering
- use the wavelength of an electron to determine the radius of a nucleus by measuring the first minimum intensity angle
sin theta = 1.22 lambda / d
advantages of electron scattering
- electrons are leptons not affected by SNF
- much more accurate than closest approach
disadvantages of electron scattering
- electrons must be accelerated to high speeds, because significant diffraction occurs when lambda is gap size
- electrons can be scattered by neutrons difficult to determine intensity
whats the nuclear radius equation
R = RoA^1/3
how can we plot the radius equation
ln R = ln Ro + 1/3lnA
how can we derive nuclear density
v = 4/3pir^3 ( assuming spherical nucleus )
v = 4/3pi (RoA^1/3 ) ^3 = 4/3piRo^3A
p = m / v so m = pv
Au / 4/3piRo^3A = 3u / 4piRo^3