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Fundamental Forces of the Universe

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Title: Fundamental Forces of the Universe


1
Fundamental Forces of the Universe
2
There are four fundamental forces, or
interactions in nature.
  • Strong nuclear
  • Electromagnetic
  • Weak nuclear
  • Gravitational

3
Strong nuclear force
  • Holds the nuclei of atoms together
  • Very strong, but only over very, very, very short
    distances (within the nucleus of the atom)

4
Electromagnetic force
  • Causes electric and magnetic effects
  • Like charges repel each other
  • Opposite charges attract each other
  • Interactions between magnets
  • Weaker than the strong nuclear force
  • Acts over a much longer distance range than the
    strong nuclear force

5
Weak nuclear force
  • Responsible for nuclear decay
  • Weak and has a very short distance range

6
Gravitational force
  • Weakest of all fundamental forces, but acts over
    very long distances
  • Always attractive
  • Acts between any two pieces of matter in the
    universe
  • Very important in explaining the structure of the
    universe

7
Remember
  • The weak nuclear force is NOT the weakest of the
    fundamental forces.
  • GRAVITY is the weakest force, but most important
    in understanding how objects in the universe
    interact.

8
Nuclear Reactions
  • There are two kinds of nuclear reactions
  • Fusion
  • Fission
  • Protons and neutrons are the two most important
    subatomic particles in the nucleus and
    participate in these reactions.

9
Fusion
  • Fusion is the process of combining nuclei of
    atoms to make different atoms.
  • This reaction is going from SMALL to LARGE
    particles.
  • Think of fusing two things together.

10
Fusion
  • Nuclear fusion happens at the sun.
  • One isotope of hydrogen-3 and one isotope of
    hydrogen-2 combine to form a helium atom, a
    neutron and lots of energy!!!

11
Fusion
  • Where does the energy come from?
  • Energy is gained when the two hydrogen atoms
    break apart.
  • Some of this energy is used up to create the
    helium atom, but the rest is given off as light.
  • Mass is converted to energy!
  • E mc2 (c 3.0 X 108 m/s) ? Speed of light
  • Since the speed of light is so large even a small
    mass will be converted to a very large energy.

12
About Nuclear Fusion
  • Nuclear Fusion is the energy source of the
    future.
  • It is what provides the sun and stars large
    amounts of energy for billions of years.
  • We have been able to use fusion on earth to make
    nuclear bombs but have not been able to make it a
    sustainable energy source.
  • If we were able to make fusion a sustainable
    energy source one teaspoon of fusion fuel (heavy
    hydrogen) could produce more than 20 tons of
    coal.
  • One ton is 2,000 lbs and roughly 250 gallons of
    oil so 20 tons would be approximately 5,000
    gallons of oil! That would fill up my tank 333
    times!

13
Fission
  • Fission is the process of breaking up the nucleus
    of an atom.
  • This reaction is going from LARGE to SMALL
    particles.
  • Think of breaking two things apart.

14
Fission
  • Nuclear fission begins when a neutron hits the
    nucleus of large atom.
  • Adding this neutron makes the nucleus unstable
    and it splits into two smaller nuclei and two
    neutrons.

15
Fission
16
About Nuclear Fission
  • Nuclear Fission happens on earth at Nuclear Power
    Plants.
  • This type of energy also made the atomic bombs
    that destroyed Hiroshima and Nagasaki in World
    War II.
  • Fission occurs with a radioactive, unstable
    material such as Uranium or Plutonium whose atoms
    nucleus is ready to fall apart at the slightest
    nudge and releases large amounts of energy and
    extra neutrons.

17
Fission Examples
18
More about Fission
  • The energy released is called radiation. The
    radioactive energy released from Plutonium can
    damage human cells. This can happen slowly
    naturally (with both Uranium and Plutonium)- but
    when it is combined with TNT (Trinitrotoluene)
    the Plutonium reaction compresses and becomes
    very dense.
  • The extra neutrons that are released bump into
    more Plutonium and a chain reaction occurs. The
    extra energy is released all at once causing
    disastrous consequences.

19
Video About Hiroshima and Nagasaki
20
Chain Reactions
  • If there are other 235U atoms nearby, the
    neutrons that came from splitting the first 235U
    nucleus can hit other atoms.
  • The nuclei of these other atoms will release more
    neutrons and split more 235U atoms.
  • This is called a chain reaction.

21
Chain Reactions
22
How Nuclear Power Plants Use Fission
  • Nuclear Power Plants use Uranium because it
    naturally undergoes fission slowly making it
    easier to induce fission at power plants.
  • Pros- One pound of Uranium produces energy equal
    to about a million gallons of gasoline.
  • It allows us to become less dependent on fossil
    fuels and Nuclear Energy is sustainable.
  • Cons- Radioactive waste and transporting the fuel
    can be dangerous.
  • If not operated properly, disasters like
    Chernobyl Power Plant (1986) accident could
    occur. This accident released 50 tons of
    radioactive waste, contaminated millions of acres
    of land, and at least a 1,000 people died from
    health conditions from exposure to the
    radioactive material.

23
Chernobyl Disaster
24
Radioactivity
  • Radioactivity is the process where the nucleus
    emits particles or energy. It is the release of
    energy.
  • There are three types of radioactive decay
  • Alpha decay
  • Beta decay
  • Gamma decay

25
Alpha decay
  • The reason alpha decay occurs is because the
    nucleus has too many protons which cause
    excessive repulsion. In an attempt to reduce the
    repulsion, a Helium nucleus is emitted so that
    the nucleus of an atom can feel stable.
  • A particle with 2 protons and 2 neutrons (Helium
    atom) is released from an unstable nucleus.
  • Alpha decay can be stopped by clothing, skin, a
    few centimeters of air, or cardboard.

26
Alpha Decay Example
After Decay Stable Nucleus
Before Decay Unstable Nucleus
27
Beta decay
  • Beta decay occurs when the neutron to proton
    ratio is too great in the nucleus and causes
    instability.
  • This occurs when a neutron of an instable nucleus
    of a radioactive isotope splits into a proton and
    an electron.
  • The electron is emitted.
  • Beta decay can be stopped by dense clothing or
    wood.

28
Beta Decay Example
BlueNeutron
RedProton
29
Gamma decay
  • Gamma decay occurs because the nucleus is at too
    high an energy. The nucleus falls down to a lower
    energy state and, in the process, emits a high
    energy photon known as a gamma particle.
  • This involves the release of high-energy,
    electromagnetic radiation from the nucleus of the
    atom.
  • Gamma rays have even more energy than X-rays.
  • It can only be stopped with thick walls of
    concrete or lead.

30
Gamma Decay Example
31
Radioactive Decay
Alpha Decay Beta Decay Gamma Decay
of Protons
of Neutrons
What is released?
32
Radioactive Decay
Alpha Decay Beta Decay Gamma Decay
of Protons Decreases by 2 Increases by 1 unchanged
of Neutrons Decreases by 2 Decreases by 1 unchanged
What is released? An alpha particle An electron and energy A gamma ray (high energy)
33
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34
Half-Life
Time (years) Fraction of element left Amount left (g) Half-life
0 1 80 0
1000 1/2 40 1
2000 1/4 20 2
3000 1/8 10 3
35
Half-Life
  • The half-life of a radioactive element is the
    TIME it takes for HALF of the radioactive atoms
    to decay to stable ones.
  • If there are 80 grams of a radioactive element
    that has a half-life of 1000 years, then after
    1000 years half of the element, or 40 grams of
    the element, will remain.
  • Now that there are only 40 grams left, how many
    grams will be left after another 1000 years has
    passed?
  • There will be only 20 grams remaining.

36
Half-Life
  • The number of half-lives that occur for an
    element is found by dividing the total time by
    the half-life of a radioactive element.
  • Total Time Half Life of half-lives
  • An element has a half-life of 1000 years. How
    many half-lives have occurred after 2000 years
    has passed?
  • Two half-lives because 2000 years 1000 years
    2

37
Half-Life
  • To find the fraction of the original amount think
    of the original amount as 1 and then divide by 2.
  • 1 2 1/2, one-half is how much remains after
    one half-life occurs.
  • If two half-lives occur then divide the original
    amount by 2 twice.
  • 1 (22) 1 4 1/4, one-fourth is how much
    remains after two half-lives occur.
  • What do you do if three half-lives occur?
  • 1 (222) 1 8 1/8, one-eighth is how much
    remains after three half-lives occur.

38
Half-Life Practice Problem 1
  • The radioactive isotope Fluorine-11 has a
    half-life of 11.0 s. How many half-lives occur
    in 11.0 s for Fluorine-11?
  • Only one half-life occurs because the half-life
    of Fluorine-11 is 11.0 s.
  • If you started with 30 g, how many grams are left
    after 11.0 s?
  • Since one half life occurs, 30 g is divided by 2
    and there are 15 g left.
  • What fraction of the original amount is left?
  • One-half of the original amount is left.

39
Half-Life Practice Problem 2
  • The radioactive isotope Carbon-15 decays very
    fast and has a half-life of 2.5 s. How many
    half-lives occur in 5.0 s for Carbon-15?
  • Two half-lives occur because 5.0 s 2.5 s 2.
  • If you started with 100 g, how many grams are
    left after 5.0 s?
  • Since 2 half-lives occur, the 100 g must be
    divided by 2 twice 100 g 4 25 g.
  • What fraction of the original amount is left?
  • 1 (22) 1 4 1/4, one-fourth remains.

40
Half-Life Practice Problem 3
  • Neon-15 has a half-life of 30 s. How many
    half-lives occur in 1.5 min?
  • Three half-lives occur because 1.5 min 90 s and
    90 s 30 s 3.
  • If you started with 56 g, how many grams are left
    after 1.5 min?
  • Since 3 half-lives occurred, the 56 g must be
    divided by 2 three times 56 g 8 7 g.
  • What fraction of the original amount is left?
  • 1 (222) 1 8 1/8, one-eighth is left

41
1. The strongest of the four fundamental forces?
  1. Strong nuclear
  2. Weak nuclear
  3. Gravity
  4. electromagnetic

42
2. Gravity depends on two thingsone is distance
the other is
  1. Inertia
  2. Orbits
  3. Mass
  4. Volume

43
3. This type of force that holds the nuclei of
atoms together
  1. electromagnetic
  2. Weak nuclear
  3. gravitational
  4. Strong nuclear

44
4. This is the force where opposite charges
attract
  1. Strong nuclear
  2. Weak nuclear
  3. Gravitational
  4. Electromagnetic

45
5.If an element is radioactive it means that its
nucleus is _______.
  1. small
  2. unstable
  3. large
  4. stable

46
6. This is the type of decay that is the weakest
and two protons and two neutrons are released.
  1. alpha
  2. beta
  3. gamma
  4. fusion

47
7. What is the force that is responsible for
nuclear decay?
  • A. Electromagetic
  • B. Strong nuclear
  • C. Gravitational
  • D. Weak nuclear

48
8. This type of reaction goes from large to small
and breaks up a big atom into smaller atoms.
  1. beta
  2. fusion
  3. alpha
  4. fission

49
9. The half-life for Krista-26 is 4.5 years. If
the initial amount is 1500 g. how much will be
left after 4 half-lives.
  1. 187.5
  2. 46.88
  3. 93.75
  4. 102.32

50
10. As the distance between objects increase the
gravity
  1. increases
  2. decreases
  3. Stays the same

51
11. The more mass an object has
  1. The closer an object is to another object
  2. The less gravity it has acting on it
  3. The more gravity is acting on it

52
12. Where does nuclear fission take place?
  1. Earth
  2. Sun
  3. Moon

53
13.This type of decay is the strongest and
releases a photon
  1. alpha
  2. beta
  3. gamma
  4. fusion

54
14. After 4 half-lives a radioactive substance
will have only about..?
  1. 1/8
  2. 1/16
  3. 1/2
  4. 1/32

55
15. Paper clips attracted to a piece of metal is
an example of what type of force
  1. Weak nuclear
  2. Strong nuclear
  3. Gravity
  4. electromagnetic

56
16. When multiple nuclear fissions occur it is
called?
  1. Nuclear fission
  2. Chain reaction
  3. Nuclear fusion
  4. Dominos

57
17. This is the process where the nucleus of an
atom releases particles or energy.
  1. fusion
  2. fission
  3. decay
  4. Radioactive decay

58
18.A 560 g sample of Webb-42 decays to 140 ghow
many half-lives have passed?
  1. 1
  2. 4
  3. 3
  4. 2

59
19. What force makes it difficult for me to dunk
a basketball?
  1. Weak nuclear
  2. Strong nuclear
  3. Gravity
  4. electromagnetic

60
20. How many neutrons are lost during gamma decay?
  1. 1
  2. 2
  3. 4
  4. 0
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