1
0 as their so small in mass in comparison
a nuclide
Z
N
A
diff physical properties but identical chem properties (how they interact)
when the nucleus of an isotope become unstable it may undergo radioactive decay or transmutation
radiation is emitted
>82 protons (bismuth and above) as well as TC (43) and Pm(61)
any change to the nucleus of an atom
-diff from chem reaction as thats only electrons
all the same thing!
the loss of 2 protons and 2 neutrons
the lose of 1 electron is minus as a neutron turns into a proton
the lose of 1 antielectron (positron) (proton basically)
the release of gamma particle (y) from high energy nucleus (too high so releases gamma)
a photon of electromagnetic radiation (light) which is a gamma ray
no mass or charge
the tendency for radiation to pass through metalsd instead of being blocked (higher means pass through higher density)
the tendency for radiation to ionise materials by adding or removing electrons
turns the material into ions which fundementally changes the biological material of something
slow
double positive charge loss
high concentration
high ionising
low penetrating
little energy is passed onto interacting atoms every time meaning it slows down for every interaction
eventually slow enough to gain two electrons and become helium or smt
fast
negative charge loss
repelled by valence electrons bc negative
ok on surface of people but bad if inside
has glancing collisions due to repulsion but is slowed down less per interaction than alpha
also occasionally dislodged electrons if at correct angle
very fast
no charge
only interacts if direct collision w/nucleus/electron which is rare
low ionising
high penetration
a=paper
B=aluminium
y=lead
the time is takes for hald a radioactive substance to decay
measured in time
N=N0(1/2)^t/t(1/2)
N0 is original mass/number
t is time passed
t(1/2) is time for half life
N0(1/2)^n
n is how many half lives occured
look at half the original # of particles
look at the time
is uncertain, half it
the word used to describe the frequency of decay
Becquerels or Bq
1 decay per second
A= A0 (1/2)^n
the repulsion then attraction of nucleons
first so they dont compress too much
then so they dont repulse and fuck up the nucleus
the repulsion is stronger than the nuclear force
a very small unit
eV= Joules/1.6 x 10^-19 (charge of electron)
the mass lost when the protons and neutrons combine (they share mass like siamese twins)
the energy required to fulfill the neutrons and protons when splitting the nucleus into the individul atoms
E= m c^2
m is mass
E is energy in joules
c is speed of light (3x 10^8)
higher binding energy
thus more mass shared/lost when combined
when a nucleus is struck by a neutron and the substance splits into two nuclei, neutrons and energy
when the fission occurs, neutron(s) fly off and hit another nucleus and assuming it can produce fissile fragments (has critical mass(enough mass to split)) then another fission reaction occurs
the energy required to split an atom into all individual neutrons and protons separately
pushing atoms close enough to form a bond
high pressure and temp
J= eV x 1.6 x 10^-19