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Chapter 18: standard 11

• Nuclear processes are those in which an atomic

nucleus changes, including radioactive decay of

naturally occurring and human-made isotopes,

nuclear fission, and nuclear fusion. As a basis for

understanding this concept:

• Standard11. a. Students know protons and neutrons in

the nucleus are held together by nuclear forces that

overcome the electromagnetic repulsion between the

protons.



• Standard 11. b. Students know the energy release

per gram of material is much larger in nuclear fusion

or fission reactions than in chemical reactions. The

change in mass (calculated by E = mc2) is small but

significant in nuclear reactions.

Recap

• The atom is made up of Protons, Neutrons, and

Electrons. Protons and neutrons are located in

the nucleus while the electrons orbit on the

shells or orbital. Protons are positively charged

and neutrons have no charge.

• Standard 11 studies only the nucleus, that is,

protons and neutrons. The nucleus of an atom

(X) called nuclide is represented as AzX; where

A is the atomic mass (p + n) and z is atomic

number (number of protons only). Isotopes

have same atomic number, z but different A.

Electrostatic law

• The law of electrostatics states that like charges will

repel and unlike charges will attract each other. That

is

Proton-proton or electron-electron are like charges.

Proton-electron or anion - cation are unlike charges

• So, why should protons, that are like charges, stay

together in the nucleus?

• The neutrons have no charge so they function like

sandwich between the protons providing an opposing

force called the strong nuclear force which holds the

protons together in the nucleus

Helium atom

x

P+n 4 He

n p+ = 2

x

Stability of the nucleus

• What is nuclear stability? The ability of protons

and neutrons to stay together in the nucleus for

a long time.

• What factors promote nuclear stability?

- Strength of the nuclear force - the stronger

the nuclear force the more stable is the

nucleus.

- neutron/Proton ratio – atoms with atomic # s

1 – 20 favor a 1:1 ratio for the nucleus to be

stable. For atoms with atomic # more than 20, a

ratio of 3neutron to 2proton is favored. Or (3:2)

or Neutron/Proton = 3/2 =1.5

Nuclear binding energy

• The energy required to separate protons from neutrons in the

nucleus.

• When the nucleus of an atom is weighed, it will weigh less than

if the protons and neutrons were weighed separately and their

masses summed.

• Let us say the sum of individual masses of protons and

neutrons is A and the mass of the nucleus is B. The difference

in mass is A – B = m. m is called the mass defect.

A - B = m



Ex: Masses of (P+ + N + p+ + N ) - Pn = mass defect (m)

np





• Binding energy, E = mc2 where c is the speed of light.

• Assignment: If the sum of protons and neutrons is 20.000g and

the mass of the nucleus is 19.998g,What is the binding

energy? c = 300,000,000 m/s. (hint: convert mass difference to

kg)

Comparing Energy release

Chemical Fission Fusion





n + 235U → 143Ba +

Reaction C + O2 → CO2 91Kr + 2n

2H + 3H → 4He + n









UO2

(3%U-235 + 97% Deuterium + Tritium

Fuel Coal

U- 238)





700K 10,000K 100,000,000K

Temperature





Energy 3.3 x 107 2.1 x 1012 3.4 x 1014

J/Kg

Answer the following questions

1) What particles are found in an atom? State each

particle location within the atom.

2) Define the following words: a) atomic number;

b) mass number; c) isotope.

3) a) What is a nuclide? b) If nuclide of an atom X is

represented as AzX, what is i) A and ii) z called? c) if

the # of neutron is represented as n, what is the

relationship between A, z, and n?

4) a) What forces hold the nucleons together? b) what

is mass defect? c) What is the relationship between

mass defect and binding energy?

5) a) What is nuclear stability? b) What 2 factors are

responsible for nuclear stability? c) How can you

predict the stability of the nucleus of an atom?

11c. Students know some naturally occurring isotopes of elements

are radioactive, as are isotopes formed in nuclear reactions.

Name of isotope How it occurs Type of radiation Half-life uses

produced



radiometric dating:

determination of age

Carbon - 14 Natural Beta 5730 years of carbon-containing

artifacts up to about

70,000 years; also

used as a biological

tracer, for example,

in studies of

photosynthesis

Chlorine - 36 Natural beta 301,000 years measurement of

sources of chloride

and determining the

age of water up to

about 2 million years

old.

Sodiun-24 Nuclear reactor Beta & gamma 15 hours location of leaks in

water pipes, studies

of body electrolytes

Chromium-51 Nuclear reactor Alpha 27.7 days labeling of red blood

cells & quantifying

gastro-intestinal

protein loss

11d. Students know the three most common forms of radioactive

decay (alpha, beta, and gamma) and know how the nucleus

changes in each type of decay

Disintegration of the nucleus

• The spontaneous disintegration of the nucleus is called

radioactive decay. Radioactive decay is divided into Fission and

fusion. The energy or particles released during radioactive

decay is called radiation.

3 types of radiations produced are

• a) Alpha radiation = 42 He2+ ; symbol α (Helium nucleus)

• b) Beta radiation = o-1e ; symbol β (high speed electron)

• c) Gamma radiation = 00 γ ; symbol γ (photon – light)

Characteristics of each radiation

Radiation Charge mass also called in magnetic/electric field

• Alpha radiation +2 4 amu deflected

• Beta radiation -1 small high speed deflected

mass electron

• Gamma radiation 0 0 Electromagnetic wave Not deflected

Deflection of various radiations by magnetic or Electric fields



• Deflection by Magnetic field;

Magnetic field



N β



γ



α

S









• Deflection by Electric field Electric field





+ β

γ

_

α

How does the nucleus change with the production of

each radiation?

• When alpha radiation is produced, the atomic #

reduces by 2 and the atomic mass reduces by

4. Alpha particle





Ex: 22688Ra → 22286Rn + 24He

• When Beta radiation is produced, the atomic #

increases by 1 and that atomic mass stays the

same. Beta (electron)





Ex: 14 C → 14 N + 0 e

6 7 -1

• When gamma radiation is produced, the atomic

# and the atomic mass stay the same.

Gamma radiation





Ex: 13153I → 131

53I + γ

11e. Students know alpha, beta, and gamma radiation produce different

amounts and kinds of damage in matter and have different penetrations

• Penetration and damage caused by various radiations



• Alpha radiations are stopped by any thing made

of wood. Ex: a piece of paper. But they are very

damaging because of their high mass. They

ionize air as they move through.

• Beta radiations are stopped by Metal foil. Ex

Aluminum foil. They are not very damaging

since they have very little mass. They also

ionize air but to a lesser scale.

• Gamma radiation can only be stopped by a

thick block of lead or concrete. They are not

very damaging and will not ionize air.

Diagrammatic representation of Radiations penetration.





Aluminum Thick block of

paper foil Lead or concrete





Alpha radiation (α)





Beta radiation (β)









Gamma radiation (γ)

Answer the following questions

• 1) a) Define radioactivity. b) In what part of the atom does

radioactivity occur? c) What radiations are produced during

radioactivity? d) How is each radiation represented in a nuclear

equation?

• 2) In a tabular format, State the characteristics of each

radiation.

• 3) a) What do you need to know when balancing a nuclear

equation?

b) Balance the following nuclear equations

i) 22286Rn → 21884Po + _____, ii) 2813Al → ___ + 0-1e;



iii) 3718Ar + 0-1e → ____ ; iv) 94Be + ___ → 136C

• 4) name 2 types of nuclear reaction and give an example where

each occurs.

• 5) what is a) chain reaction, b) critical mass c) How are they

related.

• 6) Define nuclear waste. How is it disposed?



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