The Penetrating Power of Radiation  Penetrating power  

LNK2LRN™ 2009/10

Physics Honors: Ch.30 - Nuclear Physics and Radioactivity.

May 14 to 26.

Daily Plans and Assignments:

1. Friday(05/14): Intro. to Ch.30, Nuclear Physics and Radioactivity.

 HW: Read and Study pages 798-805, then answer questions 45, 48, 50,

and 53 on page 828.

2. Monday(05/17): Review of Nuclear Physics and Radioactivity.

HW: Complete Review Handout #1.

3. Tuesday(05/18): Nuclear Equations and Binding Energy. HW: Read

and Study pages 806-14, then answer questions 59, 61, 64, and 66 on

page 829.

4. Wednesday(05/19): Calculating Half-Life. Particle Accelerators and

Detectors. HW: Answer questions 73, 74, and 78 on page 829.

5. Thursday(05/20): LAB on Half-Life Simulation. HW: Process lab

data and plot graph (lab report due Tuesday).

6. Friday(05/21): Post-Lab Discussion and Problem Solving.

HW: Write lab report (due tomorrow).

7. Monday(05/24): The Building Blocks of Matter. HW: Read and

Study pages 815-823, solve probs. 79, 80, 81, and 82 on page 829,

and prob. 86 on page 830.

8. Tuesday(05/25): REVIEW Chapter 30 - Nuclear Physics.

HW: Complete all review handouts started in class.

9. Wednesday(05/26):  TEST on Ch.30 - Nuclear Physics. HW: Visit

the web-site for notes and plans for Final Exam Review.

 

Very Important: If you have any questions, or were absent and

need to complete missing work, see me before school (8:00 -

8:30 AM), during Lunch, or after school. Best to send an email to

rpersin@fau.edu. Remember, all Make-up Work must be completed

within 3 days of absence.

 

Website Notes for Chapter 30: Nuclear Physics.

1. Henri Becquerel (1852-1908) accidentally found that all compounds

containing uranium emitted rays that penetrate and fog photographic plates,

after examining a mysterious rock.

2. Ernest Rutherford (1871-1937) identified alpha, beta, and gamma radiation

and used alpha particles to bombard gold foil. He found that most of an atom

is empty space but contains a massive positively charged nucleus.

3. The Curies, Pierre and Marie, were the first to discover other radioactive

elements, for example, Polonium and Radium.

4. The nucleus can be characterized by a mass number, A, an atomic number,

Z, and a neutron number, N, with A = Z + N. Atoms having the same number

of protons but different amounts of neutrons are called isotopes.

5. The nucleus of an atom contains most of the mass, consists of protons

and neutrons, with protons and neutrons termed as "nucleons."

6. We use the Atomic Mass Unit (amu), or u, for nucleon mass. To convert just

use the fact that 1 u = 1.6605x10-27 kg. This means that we now have the

mass of a proton as, 1 p = 1.007825 u, and a neutron, 1 n = 1.008665 u.

7. The change, transmutation, in an atomic nucleus can be natural or artificial.

Enrico Fermi (1901-1954) successfully produced artificially radioactive elements

in the laboratory.

8. Radioactive decay produces three kinds of particles: alpha, α, helium nuclei;

beta, β, high-speed electrons; and gamma, γ, ray photons.

9. Bombardment of nuclei by protons, neutrons, alpha particles, electrons,

gamma rays, or other nuclei can produce a nuclear reaction.

10. Linear accelerators, synchrotrons, and super-colliders produce high-energy

protons and electrons which can collide with each other or an atomic nucleus.

11. Particle detectors include photographic plates, the Geiger-Muller tube,

scintillation screens, and the cloud chamber.

12. Alpha can be stopped by thick paper, beta by thick aluminum foil, and a

few centimeters of lead will stop gamma.

13. During positron decay a proton changes into a neutron with the emission

of a positron and a neutrino.

14. When matter and antimatter combine, all matter is converted into energy,

or lighter matter-antimatter particle pairs. By pair production, energy is

converted into a matter-antimatter particle pair.

15. The weak interaction operates in beta decay while the strong force binds

the nucleus together. During beta decay a neutron changes into a proton and

the nucleus emits a beta particle and a mass-less antineutrino.

16. The binding energy is the energy equivalent of the mass defect. The

assembled nucleus has less mass than its constituent parts due to mass-to-

energy conversion, Binding Energy = (Δm)c2 , with Δm as the mass defect.

17. Nuclear reactors use the energy released in fission as heat to boil water,

which produces steam, that turns turbine blades to run a generator.

18. The binding energy of the nucleus is the difference in energy between its

nucleons when bound and its nucleons when unbound. Energy-mass equivalence

can be computed using 1 amu = 931 MeV.

19. The half-life, T½ , is the time required for half the original nuclei of a

radioactive substance to undergo radioactive decay. We use the equation

A = A0∙2-n where n is the number of half-lives, and A indicating amount.

20. The decay constant, lambda, λ, indicates the rate of radioactive decay.

Half-life can also be calculated by T½ = .693/λ .

21. Nuclear reactions involve a change in the nucleus and can be given by

equations. In equations for nuclear reactions, subscripts and superscripts must

agree on both sides.

22. In a nuclear equation the sums of the subscripts (atomic number or particle

charge) on both sides of the equation are equal and the sums of the superscripts

(mass number) on both sides of the equation are equal.

23. In fission, heavier nuclei split to form lighter nuclei and energy is released.

In fusion, lighter nuclei combine to form heavier nuclei with more binding energy.

24. Physicists currently believe there are three types of basic building blocks of

matter: quarks, leptons, and bosons.

25. Quarks and leptons make up everyday matter, which is held together by

bosons. Each boson is associated with a force.

26. The photon, the unit of the electromagnetic force, holds the electron to

the nucleus in the atom. The way these particles combine dictates the structure

of matter.

27. And to get full credit for your homework make sure you are following

these steps

(i) read the problem and identify the given variables

(ii) determine what you are asked to solve for

(iii) find the correct formula to use

(iv) use algebra to isolate the unknown

(v) substitute-in the given information and simplify.

View the PowerPoint™

 

animated open door gifTHE HONORS PHYSICS ARCHIVES
Ch.1: Physics Intro. Ch.2&3: Linear Motion. Ch.4&5: Forces.
Ch.6: 2-Dim Motion. Ch.7: Gravitation. Ch.8: Rotary Motion.
Ch.9: Momentum. Ch.10&11: Work&Energy. Ch.12: Thermal Energy.
Ch.13: States of Matter. Semester Review. Ch.14&15: Waves&Sound.
Ch.16: Study of Light. Ch.17&18: Mirrors & Lenses. Ch.19: Light Interference.
Ch.20&21: Electrostatics. Ch.22&23: DC Circuits. Ch.24-26: Electromagnetics.
Ch.27: Quantum Theory. Ch.28: The Atom.  
 

CLICK ON THE LINKS BELOW TO LEARN MORE ABOUT THIS WEEK'S TOPICS

Radioactivity

Particle Accelerators

Radioactive Elements

Nuclear Science

Building Blocks of Matter
MAY THE NET FORCE BE WITH YOU!

Black History Month

Honda ASIMO

Ancient Technology

Einstein Logo

 

And Always Remember...

"From  Newtonian Mechanics,

Through Quantum Theory,  

Without  Physics,  

Life Would Be Dreary."

LINK TO YOUR TEXTBOOK.

  ENGINEERS EDGE

   LAB ABSTRACT