Chemistry
- Chapter 22: The Nucleus
I.
Subatomic particles
A. Leptons (6): elementary particles;
have no internal structure; do
not respond to the strong nuclear force;
B. Hadrons:
not an elementary particle; have
internal structure; does respond to the
strong nuclear force; made of quarks
1. quarks (6):
elementary particles; have no
internal structure; responds to the
strong nuclear force
a. "flavors": types of quarks; each "flavor" is charged; there are three pairs of quarks
1.
up and down: up = +2/3; down = -1/3
2. strange and charm: charm = +2/3;
strange = -1/3
3. top and bottom (or truth and beauty): top = +2/3; bottom = -1/3
b. "colors": (not in the conventional meaning of the word
color) red, blue or green
2. baryons:
made of three quarks; proton and
neutron
a. proton:
two up quarks and one down quark, and one of each "color"
((+2/3) + (+2/3) + (-1/3) = +1)
b. neutron:
two down quarks and one up quark and one of each "color"
((+2/3) + (-1/3) + (-1/3) = 0)
3. mesons:
made of one quark and one antiquark of complimentary "colors"
C. each lepton and quark has a corresponding
antiparticle
1. an antielectron is a positron: massless;
positive
2. an antidown quark: same mass as down quark but the opposite "flavor" and
"color"
II.
Nucleons: those particles in the
nucleus, the protons and neutrons
III.
Nuclide: a unique, specific atom
with a specified number of protons and neutrons in the nucleus
IV.
Isotope: an atom of an element
with a different mass due to a different number of neutrons, carbon-14 and carbon-12
V.
Nuclear symbol:
VI.
Nuclear Stability: how stable
the nucleus is to radioactive decay
A. Nuclear Mass Defect and Binding Energy
1.
Mass
defect is the difference between the mass you expect when you add the masses of
all the protons, neutrons and electrons and the actual mass that is measured
a. proton:
1.007276 amu
b. neutron:
1.008665 amu
c. electron:
0.0005486 amu
2.
Binding
energy is the energy released when the nucleus is formed from its component
parts, it is related to nuclear
mass defect by Einstein’s equation E = mc2; the larger the binding energy, the more
stable the nuclei
B. Stability
1. plotting the number of neutrons versus the
number of protons shows there is a narrow band of stability for nuclei
2. neutron to proton ratio
a. for element up to #20, more stable isotopes have a n0 to p+ ratio of 1:1
b. for higher elements, more stable isotopes
have a n0 to p+ ratio of 1.5:1
c. elements with even numbers of protons and
neutrons tend to be more stable
B.
elements
above #83 have no stable isotopes
C.
elements
with more than 92 protons are called transuranium elements and are all
radioactive
VII. Radioactivity: nucleus will decay or disintegrate to a lighter nucleus by giving
off particles and electromagnetic radiation (energy) or both
VIII.
Types of radioactivity:
radioactive particles can be emitted from the nucleus or absorbed by the
nucleus
A. Alpha particles
1. symbol:
a or
; a helium nucleus (a
helium atom stripped of its electrons)
2. has two protons and two neutrons; mass = 4;
charge = +2
3.
low penetrating power (0.05 mm of body tissue), can be stopped by paper
or clothing
4. most damaging because they are the most
ionizing
5. usually restricted to very heavy nuclei
1.
when
a nucleus emits an alpha particle its atomic mass decreases by four and its
atomic number decreases by two; when a
nucleus absorbs an alpha particle its atomic mass increases by four and its
atomic number increases by two
B. Beta particles
1. symbol:
b or
; like an electron but it originates from the
nucleus
2. a neutron is converted into a proton and an
electron and the proton stays in the nucleus but the electron is ejected into
the
electron cloud or beyond: ![]()
3. mass = 0;
charge = -1
4. medium penetrating power (4 mm of body
tissue), can be stopped by metal foil
5.
medium damage
6. nuclei above the band of stability usually
emit beta particles because they have too many neutrons (the neutron to
proton ratio is too high)
7. when a nucleus emits a beta particle its
atomic mass remains the same and its atomic number increases by one
C. Positron
1. symbol:
; a positive electron originating from the
nucleus
2. a proton is converted into a neutron and a
positron and the proton stays in the nucleus but the electron is ejected into
the
electron cloud or beyond: ![]()
3. mass = 0;
charge = +1
4.
nuclei below the band of stability usually emit positron particles
because they have too many protons (the
neutron to
proton ratio is too low)
5. when a nucleus emits a beta particle its
atomic mass remains the same and its atomic number decreases by one
6. antiparticle of an electron; when a positron collides with an electron
they annihilate each other and release energy
D. Electron capture, also called K-capture
1.
nuclei below the band of stability have too many protons and can lower
the neutron to proton ratio by capturing an
inner
orbital electron; the captured electron
combines with a proton to form a neutron: ![]()
E. Gamma rays
1. symbol:
g or
; high-energy, very short-wavelength photons
2. mass = 0;
charge = 0
3. most penetrating power, can be only partial
stopped by several inches of lead or feet of concrete
4. least damage
5. when a nucleus emits a gamma ray its atomic
mass remains the same and its atomic number remains the same but
the energy of the nucleus is lowered
F. Other common decay particles; can be emitted or absorbed
1. Neutron:
2. Hydrogen nuclei
a. hydrogen:
![]()
b. deuterium:
![]()
c. tritium:
![]()
IX.
Transmutation: when a nuclide
decays to a different nuclide with a different number of protons; element is changed
X. Decay
series: a series of successive decays
involving several different nuclides of different elements; chain reactions
A. Parent nuclide – the heaviest nuclide of
each decay series
B. Daughter nuclide – the nuclides produced by
the decay of the parent nuclides
XI.
Nuclear equation
A. conservation of mass number
B. conservation of numbers of protons (nuclear
charge)
C. example:
; the numbers on
the top to the left of the arrow equal the numbers on the top to
the
right of the arrow (conservation of mass number) and the numbers on the bottom
to the left of the arrow equal the
numbers
on the bottom to the right of the arrow
(conservation of nuclear charge)
XII.
Half-Life: decay rate
A. the amount of time it takes for half of a
sample to undergo radioactive decay
B. time varies from milliseconds to billions of
years
Xo = initial amount, X = final amount,
C.
; t = amount of
time, t1/2 = half-life
XIII.
Damage
A. energy of the radiation (rad)
B. penetrating ability
C. ionizing ability
D. chemical properties of the radiation source
E. effects are cumulative
XIV. Ionization: radioactive particles cause electrons to be
removed or stripped from atoms or molecules forming ions; for living
tissues this happens at the cellular level
XV. Uses
of radiation
A. used for dating old materials
1.
carbon-14 by beta emission
2.
Uranium to lead
3. potassium to argon
B.
medical
applications
C.
agriculture
XVI.
Radiation
Detection
A.
film
badge
B.
Geiger-Müller
counter
C.
Scintillation
counter
XVII.
Nuclear Fission and Fusion
A. Fission
1. nucleus of a large atom breaks up into more
stable intermediate sized nuclei: ![]()
2.
energy released
3. chain reactions – when fission releases a
neutron the released neutron can hit other large nuclei causing them to
become
unstable and break releasing more neutrons to smash into other nuclei à chain reaction
4. Nuclear Reactor
a. controlled fission chain reactions
b. neutrons
c. control rods
B. Fusion
1. two or more small nuclei join to form a
larger nucleus: ![]()
2. releases more energy than fission
3. occurs at only very high temperatures
4. does not produce radioactive waste
5. the sun