Tuesday 1 June:

 

Key Concept(s) Today:

 

Journal:

 

L#93/95/96 (Relativity)

#93:1 - 3, 17, 18  #95: 1, 2, 6

#96: 1, 2, 5, 7

(due Today  1 June)

 

#98 (Half-Life): 1 - 4, 6, 7, 10, 14, 16, 19,   (due Thursday 3 June)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

Projects:

 

 

Mouse Trap Car Friday 4 June

 

Final: Tues 8 June

 

 

 

3. Power Pt on Nobel Prize (Physics) 15 June

 

 

 

 

 

 

New Material:

  • The Speed of Light is the same for all observers.

 

  • However, Mass, Time and Length change.

 

  • Mass, Time and Length will remain normal to the observer in their own reference frame. "Everything is relative"  (except light).

 

Relativity Factor:

 

 

 

  • Equation relating speed of light, speed of object and constant, gamma "c" is the speed of light
    "v" is the speed of the object in question

     

     

    For example, in space when an rocket reaches a speed of 0.999c,  its length was 1 meters, its mass was 1 kg and it traveled for 1 year (its time), what would we measure its

    a. length

    b. mass

    c. time

 

 

g = 1/ 1- (V2/c2)

 = 1 / 1- (0.999c2/c2)

= 1 / 1- (0.998) 

g= 1/√.002   -->  22.4 times

 

So,

Length is shorter

             1/22.4 or .045 meters

Mass is greater by 22.4 times =

                      22.4 meters

Time is greater by 22.4 times =

                      22.4 years

 

 

 

 

 

__

Half‑life:

The time it takes for ½ of the atoms to decay. If you have 200 atoms, how long will it take before you have 6 atoms left if the half-life is 15 days?

Start with  200 atoms

1st ½ life: 100 atoms à 15 days

2nd ½ life: 50 atoms à 30 days

3rd ½ life: 25 atoms à 45 days

4th ½ life: 12.5 atoms à 60 days

5th ½ life: 6 atoms à 75 days

_

Final: Tues 8 June

 

Turn in Tex Books by 8 June

 

Photoelectric Effect (PEE): If a beam of light is pointed at the negative end of a pair of charged plates, a current is produced. Each photon of blue light released an electron. But red photons did not.

 
 

          

 

·       The maximum kinetic energy K of the photoelectrons as a function of the frequency of incident light?

 

 

 

Nuclear Reactions

 

The following are conserved in a nuclear reactions:

    r (momentum) , electrical charge and nucleons

 

Fusion (combining):

               4 11Hà  42He + energy (E = mc2)

 Difference in mass = 0.048 x 10-27kg à E = mc2

à  E = (.048 x 10-27)(3 x 108)2

                             à E = 0.43 x 10-11 J

 

 

 

 

 

 

Fission: (breaking apart):

q   Beta Decay:

 

Beta decay results in the emission of an electron and antineutrino, or a positron and neutrino.

 

q   (Beta-minus):                           ­­_

 10 à       P+    +     e        +    h         +  Q

           neutron à  proton  + electron + Anti-neutrino + KE

 

q   Alpha Decay (Helium nucleus w/o electrons):

  23892 à 23490Th   + 42He     + Q

 

 Uranium 238 à  Thorium 234 + Alpha + disintegration energy

          (Parent)     à      (Daughters)           + 4.3 MeV