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Intro to Nuclear Chemistry. http://www.chem.orst.edu/graduate/pics/Reactor.jpg. How does a nuclear reactor work?. http://www.lanl.gov/science/1663/images/reactor.jpg. How does a small mass contained in this bomb cause……. Nuclear Bomb of 1945 known as “fat man”. - PowerPoint PPT Presentation

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Page 1: Intro to Nuclear Chemistry

Intro to Nuclear Chemistry

http://www.chem.orst.edu/graduate/pics/Reactor.jpg

Page 2: Intro to Nuclear Chemistry

How does a nuclear reactor work?

http://www.lanl.gov/science/1663/images/reactor.jpg

Page 3: Intro to Nuclear Chemistry

How does a small mass contained in this bomb cause……

• Nuclear Bomb of 1945 known as “fat man”

http://www.travisairmuseum.org/assets/images/fatman.jpg

Page 4: Intro to Nuclear Chemistry

…this huge nuclear explosion?

http://library.thinkquest.org/06aug/01200/Graphics/705px-Nuclear_fireball.jpg

Page 5: Intro to Nuclear Chemistry

Is there radon in your basement?

http://a.abcnews.com/images/Blotter/abc_1radon_ad_070625_ssh.jpg

Page 6: Intro to Nuclear Chemistry

Notation

Page 7: Intro to Nuclear Chemistry

NUCLEAR CHEMISTRY

• Deal with the nucleus of the atom.• Inside the nucleus there are 2 type of

subatomic particles. They are called NUCLEONS = Protons and neutrons

• The nucleons are bound together by a strong force called binding force.

Page 8: Intro to Nuclear Chemistry

Isotopes

• Atoms of a given element with: same #protons

but different # neutrons

Page 9: Intro to Nuclear Chemistry

H H H

http://education.jlab.org/glossary/isotope.html

Page 10: Intro to Nuclear Chemistry

Isotopes of Carbon

Page 11: Intro to Nuclear Chemistry

• Isotopes of certain unstable elements that spontaneously emit particles and energy from the nucleus.

• Henri Beckerel 1896 accidentally observed radioactivity of uranium salts that were fogging photographic film.

• His associates were Marie and Pierre Curie.

Radioactive Isotopes

Page 12: Intro to Nuclear Chemistry

Marie Curie: born 1867, in Poland as Maria Sklodowska

• Lived in France• 1898 discovered the

elements polonium and radium.

http://www.radiochemistry.org/nuclearmedicine/pioneers/images/mariecurie.jpg

Page 13: Intro to Nuclear Chemistry

Marie Curie a Pioneer of Radioactivity

• Winner of 1903 Nobel Prize for Physics with Henri Becquerel and her husband, Pierre Curie.

• Winner of the sole 1911 Nobel Prize for Chemistry.

Page 14: Intro to Nuclear Chemistry

RADIOACTIVITY

• Emission of rays and particles from unstable nuclei.

• When a nucleus is emitting rays or particles it is said that is DECAYING or is disintegrating.

Page 15: Intro to Nuclear Chemistry

Stability of nuclei:

• Depend on the ratio between the neutrons and protons. Too many or too few neutrons lead to an unstable nucleus. All elements with more than 83 protons are unstable.

Page 16: Intro to Nuclear Chemistry

Types ofNatural Decay

Page 17: Intro to Nuclear Chemistry

NATURAL DECAY

There are 4 types of naturally occurring disintegration or decay. USE TABLE O!

• Alpha ( a ) decay - Nucleus of He

• Beta ( b ) decay - Electrons• Gamma (g ) radiation - Energy• Positron emission

Page 18: Intro to Nuclear Chemistry
Page 19: Intro to Nuclear Chemistry

SeparationAlphaBetaGamma.MOV Separation of Radiation

Page 20: Intro to Nuclear Chemistry
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Transmutation• When the nucleus of one element is

changed into the nucleus of another element. IT CAN ONLY HAPPEN IN A NUCLEAR REACTION!!!

Page 24: Intro to Nuclear Chemistry

Nuclear Reactions• The chemical properties of the nucleus are

independent of the state of chemical combination of the atom.

• In writing nuclear equations we are not concerned with the chemical form of the atom in which the nucleus resides.

• It makes no difference if the atom is as an element or a compound.

• Mass and charges MUST BE BALANCED!!!

Page 25: Intro to Nuclear Chemistry

Emission of alpha particles a :

• helium nuclei • two protons and two neutrons • charge +2e  • can travel a few inches through air• can be stopped by a sheet of

paper, clothing.

Alpha Decay

Page 26: Intro to Nuclear Chemistry

Alpha Decay

Uranium Thorium

Page 27: Intro to Nuclear Chemistry

Alpha Decay

http://education.jlab.org/glossary/alphadecay.gif

Page 28: Intro to Nuclear Chemistry

Alpha Decay:

Loss of an a-particle (a helium nucleus)

He42

U23892 Th234

90 He42+

Page 29: Intro to Nuclear Chemistry

Alpha Decay

• Mass changes by 4• The remaining fragment has 2 less

protons• Alpha radiation is the less penetrating of

all the nuclear radiation (it is the most massive one!)

Page 30: Intro to Nuclear Chemistry

Alpha decay:• When a nucleus emits alpha particles.• * Atomic number decreases by 2.• * Mass number decreases by 4.• * Neutrons decrease by 2.

Page 31: Intro to Nuclear Chemistry

Beta Decay:

Loss of a b-particle (a high energy electron)

b0

−1 e0−1or

I13153 Xe131

54 + e0−1

Page 32: Intro to Nuclear Chemistry

Beta Decay

• Beta particles b: electrons ejected from the nucleus when neutrons decay

( n -> p+ +b- ) • Beta particles have the same charge and

mass as "normal" electrons.

Page 33: Intro to Nuclear Chemistry

Beta Decay• Beta particles b: electrons ejected from the

nucleus when neutrons decay n -> p+ +b-

• Beta particles have the same charge and

mass as "normal" electrons.

• Can be stopped by aluminum foil or a block of wood.

Page 34: Intro to Nuclear Chemistry

Beta Decay • When a neutron becomes a proton and

emits an electron.• * Atomic Number or number of protons

increases by 1• * Number of neutrons decreases by one.• * Mass number remains the same. 

Page 35: Intro to Nuclear Chemistry

Beta Decay

Page 36: Intro to Nuclear Chemistry

Beta Decay

Thorium Protactinium

Page 37: Intro to Nuclear Chemistry

Beta Decay

• Involves the conversion of a neutron in the nucleus into a proton and an electron.

• Beta radiation has high energies, can travel up to 300 cm in air.

• Can penetrate the skin

Page 38: Intro to Nuclear Chemistry

Beta decay

• Write the reaction of decay for C-14

Page 39: Intro to Nuclear Chemistry

Positron Emission• When a proton changes to a neutron emits

a positron.• *Atomic number (number of

protons)decreases by 1• *Number of neutrons increase by 1.• *Mass number remains same

Page 40: Intro to Nuclear Chemistry

Gamma Emission:

Loss of a g-ray (high-energy radiation that almost always accompanies the loss of a nuclear particle)

g00

Page 41: Intro to Nuclear Chemistry

• Gamma radiation g : electromagnetic energy that is released. 

• Gamma rays are electromagnetic waves.• They have no mass.• Gamma radiation has no charge.

– Most Penetrating, can be stopped by 1m thick concrete or a several cm thick sheet of lead.

Gamma Decay

Page 42: Intro to Nuclear Chemistry

3 Main Types of Radioactive Decay

• Alpha a

• Beta b

• Gamma g

Page 43: Intro to Nuclear Chemistry

Examples of Radioactive DecayAlpha Decay

Po Pb + He

Beta Decay p n + en p + e

C N + eGamma Decay

Ni Ni + g(excited nucleus)

Page 44: Intro to Nuclear Chemistry
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Page 46: Intro to Nuclear Chemistry

Nuclear Stability

• Depends on the neutron to proton ratio.

Page 47: Intro to Nuclear Chemistry

Band of Stability

Number of Neutrons, (N)

Number of Protons (Z)

Page 48: Intro to Nuclear Chemistry

What happens to an unstable nucleus?

• They will undergo decay

• The type of decay depends on the reason for the instability

Page 49: Intro to Nuclear Chemistry

What type of decay will happen if the nucleus contains too many

neutrons?

• Beta Decay

Page 50: Intro to Nuclear Chemistry

Example:C N + e

In N-14 the ratio of neutrons to protons is 1:1

14

7 -1

014

6

Page 51: Intro to Nuclear Chemistry

Artificial Transmutations

• To change one element into another. Only possible in nuclear reactions, never in a chemical reaction.

• TWO REACTANTS, A FAST MOVING PARTICLE AND A TARGET MATERIAL

• In order to modify the nucleus huge amount of energy are involved.

• These reactions are carried in particle accelerators or in nuclear reactors

Page 52: Intro to Nuclear Chemistry

Artificial transmutations

• Type I : Collision of a charged particle with a target nucleus. Carried in a particle accelerator.

• Charged particles could be protons, alpha particles or electrons. Positive particles have to move very fast to overcame electrostatic repulsions between them and the nucleus.

Page 53: Intro to Nuclear Chemistry

• Particle accelerators or smashers are used to accelerate charged particles with magnetic or electrostatic fields .

Page 54: Intro to Nuclear Chemistry

Particle Accelerators(only for charged particles!)

These particle accelerators are enormous, having circular tracks with radii that are miles long.

Page 55: Intro to Nuclear Chemistry

Cyclotron and synchrotron are particle accelerators

Nuclear transformations can be induced by accelerating a particle and colliding it with the nuclide.

Page 56: Intro to Nuclear Chemistry

Type 2: when a neutron collides with a target nucleus.

• Neutrons can not be accelerated. • Neutrons are products of natural decay,

natural radioactive materials or are expelled of an artificial transmutation.

• Neutrons are obtained as by-products in nuclear reactors.

• These reactions are used to prepare radioactive nuclei from stable nuclei.

Page 57: Intro to Nuclear Chemistry

Mass defect• The mass of the nucleus is always

smaller than the masses of the individual particles added up.

• The difference is the mass defect.• That small amount translate to huge

amounts of energy E = (m) c2

• That energy is the Binding energy of the nucleus, and is the energy needed to separate the nucleus.

Page 58: Intro to Nuclear Chemistry

Energy in Nuclear Reactions

For example, the mass change for the decay of 1 mol of uranium-238 is −0.0046 g.

The change in energy, E, is then

E = (m) c2

E = (−4.6 10−6 kg)(3.00 108 m/s)2

E = −4.1 1011 J This amount is 50,000 times greater than the combustion of 1 mol of CH4

Page 59: Intro to Nuclear Chemistry

Types of nuclear reactionsfission and fusion

• The larger the binding energies, the more stable the nucleus is toward decomposition.

• Heavy nuclei gain stability (and give off energy) if they are fragmented into smaller nuclei. (FISSION)

Page 60: Intro to Nuclear Chemistry

• Even greater amounts of energy are released if very light nuclei are combined or fused together. (FUSION)

Page 61: Intro to Nuclear Chemistry

Nuclear Fission

• Nuclear fission is the type of reaction carried out in nuclear reactors.

Page 62: Intro to Nuclear Chemistry

Nuclear fission:

A large nucleus splits into several small nuclei when impacted by a neutron, and energy is released in this process

Page 63: Intro to Nuclear Chemistry

Nuclear Fission

• Bombardment of the radioactive nuclide with a neutron starts the process.

• Neutrons released in the transmutation strike other nuclei, causing their decay and the production of more neutrons.

Page 64: Intro to Nuclear Chemistry

Nuclear Fission

This process continues in what we call a nuclear chain reaction.

Page 65: Intro to Nuclear Chemistry

Controlled vs Uncontrolled nuclear reaction

• Controlled reactions: inside a nuclear power plant

• Uncontrolled reaction: nuclear bomb

Page 66: Intro to Nuclear Chemistry

Nuclear ReactorsIn nuclear reactors the heat generated by the reaction is used to produce steam that turns a turbine connected to a generator.

Page 67: Intro to Nuclear Chemistry

Nuclear Reactors• The reaction is kept in

check by the use of control rods.

• These block the paths of some neutrons, keeping the system from reaching a dangerous supercritical mass.

Page 68: Intro to Nuclear Chemistry

FUSION

• Combining small nucleii to form a larger one.

• Require millions of K of temperature

Page 69: Intro to Nuclear Chemistry

Fusion• 1H + 1H 2H + 1e + energy• 1H + 2H 3He + energy• 3He + 3He 4He + 21H + energy• Reaction that occurs in the sun• Temperature 107 K• Heavier elements are synthesized in

hotter stars 108 K using Carbon as fuel

Page 70: Intro to Nuclear Chemistry

Nuclear Fusion

• Fusion would be a superior method of generating power.– The good news is that the

products of the reaction are not radioactive.

– The bad news is that in order to achieve fusion, the material must be in the plasma state at several million kelvins.

Page 71: Intro to Nuclear Chemistry

Nuclear Fusion(thermonuclear reactions)

• Tokamak apparati like the one shown at the right show promise for carrying out these reactions.

• They use magnetic fields to heat the material.

• 3 million K degrees were reached inside but is not enough to begin fusion which requires 40 million K

Page 72: Intro to Nuclear Chemistry
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Fission is the release of energy by splitting heavy nuclei such as Uranium-235 and Plutonium-239

Fusion is the release of energy by combining two light nuclei such as deuterium and tritium

How does a nuclear plant work?• Each fission releases 2 or 3

neutrons• These neutrons are slowed down

with a moderator to initiate more fission events

• Control rods absorb neutrons to keep the chain reaction in check

• The goal of fusion research is to confine fusion ions at high enough temperatures and pressures, and for a long enough time to fuse

• This graph shows the exponential rate of progress over the decadesControlled Fission Chain Reaction

Confinement Progress

• Magnetic Confinement uses strong magnetic fields to confine the plasma

• This is a cross-section of the proposed International Thermo-nuclear Experimental Reactor (ITER)

• Inertial Confinement uses powerful lasers or ion beams to compress a pellet of fusion fuel to the right temperatures and pressures

• This is a schematic of the National Ignition Facility (NIF) being built at Lawrence Livermore National Lab

Nuclear Power Plant

There are two main confinement approaches:The energy from the reaction drives a steam cycle to produce electricity

Nuclear Power produces no greenhouse gas emissions; each year U.S. nuclear plants prevent atmospheric emissions totaling:• 5.1 million tons of sulfur dioxide• 2.4 million tons of nitrogen oxide• 164 million tons of carbon

Nuclear power in 1999 was the cheapest source of electricity costing 1.83 c/kWh compared to 2.04 c/kWh from coal

D

T

D-T Fusion4He3.52 MeVNeutron14.1 MeV

Page 74: Intro to Nuclear Chemistry

January 11

HALF LIFE

Page 75: Intro to Nuclear Chemistry

Radioactive Half-Life (t1/2 ):

The time required for one half of the nuclei in a given sample to decay.

• After each half life the mass of sample remaining is half.

• Different Isotopes have different half lives. Use table N

Page 76: Intro to Nuclear Chemistry

Common Radioactive Isotopes

Isotope Half-Life Radiation Emitted

Carbon-14 5,730 years b, g

Radon-222 3.8 days a

Uranium-235 7.0 x 108 years a, g

Uranium-238 4.46 x 109 years a

Page 77: Intro to Nuclear Chemistry

Radioactive Half-Life

• After one half life there is 1/2 of original sample left.

• After two half-lives, there will be 1/2 of the 1/2 = 1/4 the original sample.

Page 78: Intro to Nuclear Chemistry

Graph of Amount of Remaining Nuclei vs Time

A

Page 79: Intro to Nuclear Chemistry

Example

You have 100 g of radioactive C-14. The half-life of C-14 is 5730 years.

• How many grams are left after one half-life? Answer:50 g

• How many grams are left after two half-lives?

Page 80: Intro to Nuclear Chemistry

Problem

If 80 g of a radioactive sample decays to 10 g in 30 min what is the element’s half life?

Page 81: Intro to Nuclear Chemistry

• How many days will take a sample of I-131 to undergo three half life periods?

Page 82: Intro to Nuclear Chemistry

• What is the total mass of Rn-222 remaining in an original mass 160 mg sample of Rn-222 after 19.1 days?

Page 83: Intro to Nuclear Chemistry

CHEM CYCLE 2 FINAL REVIEW

TOPICS

Page 84: Intro to Nuclear Chemistry

MAIN TOPICS• 1 -Matter – definition – classification • Element – compounds- mixtures – Homogeneous

heterogeneous - representations• 2 .-Physical and Chemical Properties and changes• 3.-Temperature – definition –scales– conversions• 4.-Heat problems /heat of fusion / heat of

vaporization• 5.-Heating curves• 6.-Gas problems • 7.-Liquids – boiling vs evaporation / Vapor pressure• 8.-Solids – definition – sublimation• 9- Measuring- units. Density – significant figures

Page 85: Intro to Nuclear Chemistry

• 9. The atom – history , subatomic particles, isotopes, atomic number, atomic mass, mass number, ground state, excited state.

• 10. Nuclear chemistry – table O and N Natural decay, half life, natural decay,

artificial transmutation, fission vs fusion, uses of radioisotopes.

Page 86: Intro to Nuclear Chemistry

Answers to Nuclear reaction and half life

• 1 d 2 d 3 b 4 d• 5 37.2/12.4= 3 half lives 2g • 6 10days 7 71.5/14.3= 5 hl 1g • 8a) 4g b) 25 y• 9) a) alpha b) 1.4 1010 years c) 3hl 12.5g• 10) a)+b b)positron decay

Page 87: Intro to Nuclear Chemistry

Working with half life• 1 7.64 days• 2 2 g• 3 3 hl• 4 1/8• 5 3 hl• 6 8.021 d• 7 ~ 128 g• 8 58.2 y• 9 1/8

Page 88: Intro to Nuclear Chemistry

Measuring Radioactivity

• One can use a device like this Geiger counter to measure the amount of activity present in a radioactive sample.

• The ionizing radiation creates ions, which conduct a current that is detected by the instrument.

Page 89: Intro to Nuclear Chemistry

Uses of radioisotopesMedicine

• Medical imaging –Trace amounts of short half life isotopes can be ingested and the path of the isotope traced by the radiation given off

• I-131 is used to treat and diagnosed thyroid disorders

• Cancer treatment – radiation kills cancerous cells more easily than healthy cells.

• Cobalt-60 emits g rays • Technetium-99 is accumulated in

cancerous tumors and can be detected by a scan.

Page 90: Intro to Nuclear Chemistry

• Sterilization – γ – rays can be used to kill germs and hence sterilize food and plastic equipment Co-60 and Cs-137 are used as source of g rays.

• Industry – used to trace blockages in pipes, or to test the thickness of materials (by putting a source on one side of the material and detector on the other)

Page 91: Intro to Nuclear Chemistry

• Carbon dating• Once a living organism dies, it is no

longer taking in any Carbon.• C14 is radioactive, and decays over time.• By measuring the activity of C14 in an

object and comparing it with the amount of C14 which was present initially you can estimate when the organism died

Page 92: Intro to Nuclear Chemistry

• Each gram of carbon in a living organism emits about 15 disintegration per minute (dmp). After the organism dies and time passes, C-14 continues to decay but it is not replaced. 7dpm per gram of carbon implies that de organism lived 5700 years ago.

• After 4 half lives C-14 becomes ineffective.• U-238 decays to Pb-206. The ratio of the 2 is

used to date rocks and geological formations.

Page 93: Intro to Nuclear Chemistry
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Smoke detectors

• A radioactive source ionizes the air between two electrodes. Thus current flows between them

• If smoke particles enter this space they stick to the ions and the current is reduced.

• This reduced current triggers the alarm