Nuclear Physics. Final Paper and Presentation
|
|
- Grace Casey
- 5 years ago
- Views:
Transcription
1 Nuclear Physics Phys 1020, Day 20: Nuclear Weapons Blmfld 16.1 Reminders: All paper drafts in Review and midterm next week Office hours 1 Final Paper and Presentation Opportunity to explain some physics to a non-scientist using everyday object/phenomenon as an example Paper: 4-5 pages double spaced Hand in via SafeAssign by 11am, Tuesday 4/20 40 points Must complete to pass course Presentation: 3 min presentation, 1-2 min of questions In lab sections, week of 4/20 Bonus presentations in class 4/27 Digital projector (and laptop), overhead projector, chalk board 10 (+5) points 1
2 Sample paper outline - Introduction - Brief description of topic you re exploring - Background physics (the broad area of physics this falls into) - Discussion: More detailed description of the topic Physical principles that it employs Further applications of the area / physics - Conclusion: What are the next big steps in this field? How might someone expand on this work you ve done? Presentation - Don t try to cover everything - Pick one aspect of paper and explain in detail. - Don t read directly from your paper - Make sure your laptop/files connect/run smoothly Further instructions and grading rubric on course website Nuclear physics covers so many topical everyday life issues Local: Should I ask my realtor about radon? What about walking my dog at the rocky flats nature reserve? Did the radiation leak at NIST 2 years ago endanger you? International: Was the Manhattan project necessary? How can we stop rogue states acquiring a nuclear bomb? Should the world build more nuclear power plants? Basic knowledge of nuclear physics important for everyone 2
3 Structure of an atom and nucleus Nuclear forces and stored energy Nuclear fission - Alpha decay (spontaneous) - Fission bomb (neutron induced fission) Nuclear Fusion Nuclear Physics Radioactivity - Alpha, beta and gamma radiation - Why its bad for you Other interesting stuff that we won t have time for - Nuclear power - Nuclear medicine Sadly, (or perhaps much to your relief), demos will be limited Recipe- how to make an atom: Proton Neutron Electron Ingredients: 1 pinch protons 1 pinch neutrons 1 cup of electrons Charge C Zero C Mass kg kg kg 1. Mix protons and neutrons thoroughly. 2. Bake at 100 million degrees until sticks together to form solid dense nucleus (about s). 3. Frost with lightly with fluffy layer of negative electrons. 4. Chill before serving! atom size: Radius of nucleus is 10,000 times smaller than nucleus-electron distance 6 3
4 Elements different types of atom Each element has a unique number of protons An atom has the same number of electrons as protons (electrically neutral) Different numbers of neutrons make different isotopes of the same element - same chemical properties (electrons do the same stuff) - different nuclear properties - Isotopes defined by mass number: 235 U, 238 U hydrogen 1 p deuterium 1 p, 1n helium 2 p, 2 n Uranium p, 146 n Hydrogen isotopes Note: Atomic radii not well defined. Oxygen has 8 protons, 8 neutrons: Building Nuclei Consider a nucleus with 7 protons, 7 neutrons (nitrogen atom)..what if we want to add another proton to make oxygen (8 protons)? What will we need to do to get proton stuck to nucleus: a. just give it a little push so it will hit nucleus dead on and it will drift towards nucleus and stick. b. the closer it gets, the harder you have to push, will take lots of work c. you ll need to push really hard at first and then less as you get closer d. you ll have to push the proton towards the nucleus with a fixed amount of force (constant force). 8 4
5 Building What will we need to do to get proton stuck to nitrogen nucleus: b. the closer it gets, the harder you have to push, will take lots of work.. Lots of energy 7 positives One positive Big repelling force Bigger repelling force Force on proton given by Coulomb s law (k = Coulomb s constant): In general: Force = k x charge of object #1 x charge of object #2 (distance between objects) 2 F = k x charge of nucleus x charge of proton (distance nucleus-proton ) 2 The smaller the distance, the larger the force! 9 Potential energy curves Represent energy needed to bring charged particles together. Imagine throwing proton so starts out going towards nitrogen nucleus with a lot of speed (lots of kinetic energy): - Repelling force from nucleus slows it down - Proton s kinetic energy converted into electrostatic potential (stored) energy, as it gets closer to nucleus Potential energy Kinetic energy separation distance, r Gravity energy analogy. At center have lots of electrostatic energy proton wants to fly away Like ball at the top of a hill has gravitational energy and wants to roll down 10 5
6 Electrostatic potential energy of proton and N nucleus Potential energy Kinetic energy Separation (r) Potential energy = k x charge N nucleus. x charge of single proton at separation (separation distance) distance of r Charge of 1 proton = 1.6 x C; Charge of 7 protons=11.2 x C So at m away ~ radius of nucleus, Potential energy = (8.99 x 10 9 N m 2 /C 2 ) x (11.2 x C) x (1.6 x C) (10-15 m) = 1.61 x Joules = 10 million electron Volts. (1 electron volt = energy gained by electron moving through 1 Volt diff.= 1.6 x J) 11 What would the potential energy curve (potential energy vs. separation distance) for an electron and a proton look like? a. This curve would be flat, not going up or down b. Would look like curve for 2 protons except upside down (so going down as they got closer instead of up) c. Would be the same as the curve for 2 protons 12 6
7 Potential energy 3/28/2010 What would the potential energy curve (potential energy vs. separation distance) for an electron and a proton look like? b. Would look like curve for 2 protons except upside down (so going down instead of up) 0 Separation distance (r) Electron and proton get pulled together into a potential energy hole. We must SUPPLY energy to separate electron and proton. What about neutrons? no charge so no electrostatic interactions 13 Analyzing shape of potential energy curves between 2 particles: PE (1) Pushed apart very little, Potential energy not changing along top separation Particles repel Positive stored energy PE (3) PE separation Pushed apart hardest, Potential energy changing rapidly (2) Particles attract Energy required to separate Force on particles related to GRADIENT (SLOPE) of potential energy curve 14 7
8 So how can a bunch of positively charged protons stick together? Two different types of forces involved - Electrostatic forces - Repulsive - Only affects charged particles (protons) - Long range (each protons repels all other protons in nucleus) - Nuclear force - Attractive - Affects protons and neutrons (nucleons) in same way - Short range only bonds nucleons that are touching - Overwhelms electrical force when protons and/or neutrons (nucleons) are REALLY close together Hopper toy analogy Spring legs - like electrical force, pushes man away from base over large distance. Suction cup - like nuclear force, bonds man to base but only strong when in contact (Or nuclear force like double-sided tape - only works if in objects in close contact.) Why is the nuclear force so different? That is the way nature is! 15 Complete potential energy curve for proton approaching nucleus Electrostatic repulsion + PE PE r r Nuclear energy scale GIGANTIC compared to chemical energy. Why? Simple coulomb s law: F= k (charge 1)(charge 2) r 2 Nuclear attraction Chemistry: - Forces between electrons and protons on distance scale of atomic size (> m). Complete nuclear potential PE r Nuclear forces: - Forces between nucleons on distance scale of nuclear size - 10,000 times smaller than atom - Forces 100,000,000 times bigger because of 1/r 2. - Lots more potential energy stored!!! 16 8
9 Binding energy per nucleon Small Large Binding energy per nucleon Small Large Why is binding energy increasing with mass number for small? Why is binding energy decreasing with mass number for large? 9
10 Small Consider how forces in nucleus change when we go from 4 He (2 protons) to 7 Lithium (3 protons) 4 He 7 Li Electrostatic repulsion: - Protons feel repulsion of 1 more proton - Electrostatic repulsion increases Nuclear attraction: - All nucleons have more nucleons in contact - Nuclear binding increases A LOT Average effect More strongly bound nucleus Large Consider how forces in nucleus change when we go from 235 U (92 protons) to 237 Np (93 protons) Electrostatic repulsion: - All 90+ protons feel repulsion of 1 more proton - Electrostatic repulsion increases ALOT Nuclear attraction: - Only a couple of nucleons at edge increase number in contact - Nuclear binding increases only a little Average effect Less strongly bound nucleus 10
11 What is this curve useful for? Max binding energy for medium Small Large There are 2 types of nuclear bombs fission and fusion. Which elements should I choose for each type of bomb (be ready to explain why)? a) Small for both b) Medium sized for both c) Large for both d) Fission small, fusion large e) Fusion small, fission large What is this curve useful for? Max binding energy for medium Small Large There are 2 types of nuclear bombs fission and fusion. Which elements should I choose for each type of bomb (be ready to explain why)? a) Small for both b) Medium sized for both c) Large for both d) Fission small, fusion large e) Fusion small, fission large 11
12 Fission and fusion Fission Fusion Energy is conserved. For bomb we must RELEASE energy stored in nucleus Each nucleon in product(s) must be more tightly bound (in bigger potential energy hole) than in original nucleus(i) E = mc 2. Mass of product(s) less than mass of original nucleus(i) Fuse small Fission (break) large To release energy and create explosion Fission of large Spontaneous - Radioactive (nuclear) decay Neutron induced - Fission bomb - Nuclear power 12
13 No. of radon atoms 3/28/2010 Spontaneous fission alpha decay Alpha particle (2p + 2n) spontaneously breaks away from nucleus Nucleus is changed from one element to another 2P-2N Quantum mechanical tunneling: Small particles not localised (fuzzy) Occasionally a outside range of nuclear binding force Has lots of electrostatic PE Converts PE to KE and runs for it - a tunnels out of potential well - Never had enough energy to climb out Potential energy curve for alpha particle and product nucleus 25 Radon example of alpha decay 4.5 billion years 238 U 234 Th + a 222 Rn 3.8 days 218 Po + a T 1/2 Time Half life: Time for half of in sample to decay Decay time of any particular nucleus is unknown and random Radon exposure: Radon is a gas Biggest cause of public exposure to nuclear radiation Occurs where lots of 238 U in soil (like round here) Accumulates in basements pump it out 2 nd biggest cause of lung cancer 13
14 A useful simulation alpha decay 27 Potential curves for alpha decay from different Tunneling difficulty = width x depth of tunnel E E E 1. Hard - takes long time, - billions of years! r r r 2. Medium 3. Easy Takes millionths of a second! How much energy released? a. 1 most, 2 second, 3 least b. 2 most, 1, 3 least c. 3 most, 2, 1 least d. 3 most, 1, 2 least 28 14
15 Potential curves for alpha decay from different Tunneling difficulty = width x depth of tunnel E E E Energy released 1. Hard - takes long time, - billions of years! r r r 2. Medium 3. Easy Takes millionths of a second! How much energy released? a. 1 most, 2 second, 3 least b. 2 most, 1, 3 least c. 3 most, 2, 1 least d. 3 most, 1, 2 least energy released is potential energy at bottom of crater 29 15
Nuclear Weapons (and Energy)
Nuclear Weapons (and Energy) the how, the what and why? Phys 1020, Day 25: Questions? Finish buoyancy Nuclear Weapons Blmfld 16.1 Reminders: work on projects 1 Air vs. Helium Balloon F buoyancy SAME VOLUMES
More informationNuclear Weapons (and Energy)
Nuclear Weapons (and Energy) PV + ½ mv 2 + mgh = E total Finish Bernoulli s Equation Consider one little bit of water of volume V and mass m: the how, the what and why? Phys 1010, Day 13: Questions? Finishing
More informationLECTURE 25 NUCLEAR STRUCTURE AND STABILITY. Instructor: Kazumi Tolich
LECTURE 25 NUCLEAR STRUCTURE AND STABILITY Instructor: Kazumi Tolich Lecture 25 2 30.1 Nuclear structure Isotopes Atomic mass 30.2 Nuclear stability Biding energy 30.3 Forces and energy in the nucleus
More informationThere are 82 protons in a lead nucleus. Why doesn t the lead nucleus burst apart?
Question 32.1 The Nucleus There are 82 protons in a lead nucleus. Why doesn t the lead nucleus burst apart? a) Coulomb repulsive force doesn t act inside the nucleus b) gravity overpowers the Coulomb repulsive
More informationA is called the mass number gives, roughly, the mass of the nucleus or atom in atomic mass units = amu = u
5/5 A is called the mass number gives, roughly, the mass of the nucleus or atom in atomic mass units = amu = u The number of neutrons in the nucleus is given by the symbol N. Clearly, N = A Z. Isotope:
More information[2] State in what form the energy is released in such a reaction.... [1]
(a) The following nuclear reaction occurs when a slow-moving neutron is absorbed by an isotope of uranium-35. 0n + 35 9 U 4 56 Ba + 9 36Kr + 3 0 n Explain how this reaction is able to produce energy....
More informationNJCTL.org 2015 AP Physics 2 Nuclear Physics
AP Physics 2 Questions 1. What particles make up the nucleus? What is the general term for them? What are those particles composed of? 2. What is the definition of the atomic number? What is its symbol?
More informationNuclear Physics Questions. 1. What particles make up the nucleus? What is the general term for them? What are those particles composed of?
Nuclear Physics Questions 1. What particles make up the nucleus? What is the general term for them? What are those particles composed of? 2. What is the definition of the atomic number? What is its symbol?
More informationL-35 Modern Physics-3 Nuclear Physics 29:006 FINAL EXAM. Structure of the nucleus. The atom and the nucleus. Nuclear Terminology
9:006 FINAL EXAM L-5 Modern Physics- Nuclear Physics The final exam is on Monday MAY 7:0 AM - 9:0 AM in W90 CB The FE is not cumulative, and will cover lectures through 6. (50 questions) The last regular
More informationFundamental Forces of the Universe
Fundamental Forces of the Universe There are four fundamental forces, or interactions in nature. Strong nuclear Electromagnetic Weak nuclear Gravitational Strongest Weakest Strong nuclear force Holds the
More informationCollege Physics B - PHY2054C
College - PHY2054C Physics - Radioactivity 11/24/2014 My Office Hours: Tuesday 10:00 AM - Noon 206 Keen Building Review Question 1 Isotopes of an element A have the same number of protons and electrons,
More informationPhys 1020 Day 27 Finish nuclear energy Radiation and Nuclear Reactors, Blmfd 16.2 Exponential Growth Energy Use
Energy Resources or what am I going to drive in 30 years? How do Nuclear Reactors Work? What about accidents? What is the nature of exponential growth? What are our energy resources? Phys 1020 Day 27 Finish
More informationPhysics 1C. Lecture 29A. "Nuclear powered vacuum cleaners will probably be a reality within 10 years. " --Alex Lewyt, 1955
Physics 1C Lecture 29A "Nuclear powered vacuum cleaners will probably be a reality within 10 years. " --Alex Lewyt, 1955 The Nucleus All nuclei are composed of protons and neutrons (they can also be called
More informationUnit 3: Chemistry in Society Nuclear Chemistry Summary Notes
St Ninian s High School Chemistry Department National 5 Chemistry Unit 3: Chemistry in Society Nuclear Chemistry Summary Notes Name Learning Outcomes After completing this topic you should be able to :
More informationL 37 Modern Physics [3]
L 37 Modern Physics [3] Nuclear physics what s inside the nucleus and what holds it together what is radioactivity carbon dating Nuclear energy nuclear fission nuclear fusion nuclear reactors nuclear weapons
More informationTerm 3 Week 2 Nuclear Fusion & Nuclear Fission
Term 3 Week 2 Nuclear Fusion & Nuclear Fission Tuesday, November 04, 2014 Nuclear Fusion To understand nuclear fusion & fission Nuclear Fusion Why do stars shine? Stars release energy as a result of fusing
More informationPage 1. ConcepTest Clicker Questions Chapter 32. Physics, 4 th Edition James S. Walker
ConcepTest Clicker Questions Chapter 32 Physics, 4 th Edition James S. Walker There are 82 protons in a lead nucleus. Why doesn t the lead nucleus burst apart? Question 32.1 The Nucleus a) Coulomb repulsive
More informationIsotopes Atoms of an element (same # p+) that differ in their number of neutrons
Isotopes Atoms of an element (same # p+) that differ in their number of neutrons Radio-isotopes Isotope of an element that is UNSTABLE. They spontaneously emit particles (energy) in order to achieve a
More informationRadioactivity: the process by which atoms emit energy in the form of electromagnetic waves, charged particles, or uncharged particles.
Radioactivity: the process by which atoms emit energy in the form of electromagnetic waves, charged particles, or uncharged particles. In 1896, Henri Bequerel discovered that uranium and other elements
More informationNuclear forces and Radioactivity. Two forces are at work inside the nucleus of an atom
Nuclear forces and Radioactivity Two forces are at work inside the nucleus of an atom Forces act in opposing directions Electrostatic repulsion: pushes protons apart Strong nuclear force: pulls protons
More informationAlta Chemistry CHAPTER 25. Nuclear Chemistry: Radiation, Radioactivity & its Applications
CHAPTER 25 Nuclear Chemistry: Radiation, Radioactivity & its Applications Nuclear Chemistry Nuclear Chemistry deals with changes in the nucleus The nucleus of an atom contains Protons Positively Charged
More information3 Types of Nuclear Decay Processes
3 Types of Nuclear Decay Processes Radioactivity is the spontaneous decay of an unstable nucleus The radioactive decay of a nucleus may result from the emission of some particle from the nucleus. The emitted
More informationChapter 22. Preview. Objectives Properties of the Nucleus Nuclear Stability Binding Energy Sample Problem. Section 1 The Nucleus
Section 1 The Nucleus Preview Objectives Properties of the Nucleus Nuclear Stability Binding Energy Sample Problem Section 1 The Nucleus Objectives Identify the properties of the nucleus of an atom. Explain
More information! Exam 1 in this classroom in 1 week (Oct 1 st )! 40 Multiple choice questions! Will cover material up to and including today.!
This Class (Lecture 12): Why does the Sun Shine? Next Class: Why is the Sun Yellow? HW5 due Monday Exam 1 next Friday!! Exam 1 in this classroom in 1 week (Oct 1 st )! 40 Multiple choice questions! Will
More informationBasic Nuclear Theory. Lecture 1 The Atom and Nuclear Stability
Basic Nuclear Theory Lecture 1 The Atom and Nuclear Stability Introduction Nuclear power is made possible by energy emitted from either nuclear fission or nuclear fusion. Current nuclear power plants utilize
More informationNuclear Physics and Nuclear Reactions
Slide 1 / 33 Nuclear Physics and Nuclear Reactions The Nucleus Slide 2 / 33 Proton: The charge on a proton is +1.6x10-19 C. The mass of a proton is 1.6726x10-27 kg. Neutron: The neutron is neutral. The
More informationUNIT 10 RADIOACTIVITY AND NUCLEAR CHEMISTRY
UNIT 10 RADIOACTIVITY AND NUCLEAR CHEMISTRY student version www.toppr.com Contents (a) Types of Radiation (b) Properties of Radiation (c) Dangers of Radiation (d) Rates of radioactive decay (e) Nuclear
More informationInstead, the probability to find an electron is given by a 3D standing wave.
Lecture 24-1 The Hydrogen Atom According to the Uncertainty Principle, we cannot know both the position and momentum of any particle precisely at the same time. The electron in a hydrogen atom cannot orbit
More informationnuclear chemical change CH4 + 2O2 CO2 + 2H2O carbon dating
Nuclear Chemistry I. What is nuclear chemistry? a. Nuclear changes vs. chemical changes i. A nuclear change is a change in which the nucleons (things in the nucleus) change. For instance, if the number
More informationUNIT 10 RADIOACTIVITY AND NUCLEAR CHEMISTRY
UNIT 10 RADIOACTIVITY AND NUCLEAR CHEMISTRY teacher version www.toppr.com Contents (a) Types of Radiation (b) Properties of Radiation (c) Dangers of Radiation (d) Rates of radioactive decay (e) Nuclear
More informationNice Try. Introduction: Development of Nuclear Physics 20/08/2010. Nuclear Binding, Radioactivity. SPH4UI Physics
SPH4UI Physics Modern understanding: the ``onion picture Nuclear Binding, Radioactivity Nucleus Protons tom and neutrons Let s see what s inside! 3 Nice Try Introduction: Development of Nuclear Physics
More informationL 37 Modern Physics [3] The atom and the nucleus. Structure of the nucleus. Terminology of nuclear physics SYMBOL FOR A NUCLEUS FOR A CHEMICAL X
L 37 Modern Physics [3] [L37] Nuclear physics what s inside the nucleus and what holds it together what is radioactivity carbon dating [L38] Nuclear energy nuclear fission nuclear fusion nuclear reactors
More informationNuclear Decays. Alpha Decay
Nuclear Decays The first evidence of radioactivity was a photographic plate, wrapped in black paper and placed under a piece of uranium salt by Henri Becquerel on February 26, 1896. Like many events in
More informationRadioactivity. L 38 Modern Physics [4] Hazards of radiation. Nuclear Reactions and E = mc 2 Einstein: a little mass goes a long way
L 38 Modern Physics [4] Nuclear physics what s inside the nucleus and what holds it together what is radioactivity, halflife carbon dating Nuclear energy nuclear fission nuclear fusion nuclear reactors
More informationForces and Nuclear Processes
Forces and Nuclear Processes To understand how stars generate the enormous amounts of light they produce will require us to delve into a wee bit of physics. First we will examine the forces that act at
More informationNUCLEAR ENERGY! DAY 1: (RADIATION, FISSION, FUSION)
NUCLEAR ENERGY! DAY 1: (RADIATION, FISSION, FUSION) Nucleus Stability Stability of the nucleus depends on the nuclear forces that act between protons and neutrons Protons repel each other Protons attract
More informationAlpha Decay Simulation
Alpha Decay Simulation Go to class website, select Computer Simulations, Physics 30, Alpha Decay. Part A: Radioactive Decay in a single atom: go to the SECOND tab (single atom). 1. In the simulation, a
More informationName Chemistry-PAP Per. Notes: Atomic Structure
Name Chemistry-PAP Per. I. Historical Development of the Atomic Model Ancient Greek Model Notes: Atomic Structure Democritus (460-370 BC) was an ancient Greek philosopher credited with the first particle
More informationPreview. Subatomic Physics Section 1. Section 1 The Nucleus. Section 2 Nuclear Decay. Section 3 Nuclear Reactions. Section 4 Particle Physics
Subatomic Physics Section 1 Preview Section 1 The Nucleus Section 2 Nuclear Decay Section 3 Nuclear Reactions Section 4 Particle Physics Subatomic Physics Section 1 TEKS The student is expected to: 5A
More informationNuclear Chemistry Lecture Notes: I Radioactive Decay A. Type of decay: See table. B. Predicting Atomic Stability
Nuclear Chemistry Lecture Notes: I Radioactive Decay A. Type of decay: See table Type Symbol Charge Mass (AMU) Effect on Atomic # Alpha α +2 4 decrease by 2 Beta β- -1 0 increase electron by 1 Beta β+
More informationFriday, 05/06/16 6) HW QUIZ MONDAY Learning Target (NEW)
Friday, 05/06/16 1) Warm-up: If you start with 100g of a radioactive substance, how much will be left after 3 half-lives? 2) Review HW & Nuclear Notes 3) Complete Modeling Energy Investigation 4) Complete:
More informationRadioactivity pp Topic 9: Nuclear Physics Ch. 10. Radioactivity. Radioactivity
Topic 9: Nuclear Physics Ch. 10 pp.244-249 results from radioactive decay, which is the process in which unstable atomic nuclei transform and emit radiation. has existed longer than the human race. Unstable
More informationAn odd world. Midterm 2 review. Mid term on Thursday. Conservation of energy
Midterm review Day 15: Any final questions about nukes? Review Reminders: No HW this week! An odd world You find yourself in some diabolical plot where you are given an alpha (a) source, beta (b) source,
More informationPE q. F E = q. = kq 1q 2 d 2. Q = ne F e
Chapters 32 & 33: Electrostatics NAME: Text: Chapter 32 Chapter 33 Think and Explain: 1-6, 8 Think and Explain: 1, 4, 5, 8, 10 Think and Solve: Think and Solve: 1-2 Vocabulary: electric forces, charge,
More informationAtomic and Nuclear Physics. Topic 7.3 Nuclear Reactions
Atomic and Nuclear Physics Topic 7.3 Nuclear Reactions Nuclear Reactions Rutherford conducted experiments bombarding nitrogen gas with alpha particles from bismuth-214. He discovered that fast-moving particles
More informationCHAPTER 25: NUCLEAR CHEMISTRY. Mrs. Brayfield
CHAPTER 25: NUCLEAR CHEMISTRY Mrs. Brayfield CHEMICAL VS. NUCLEAR When you hear the word nuclear, what do you think of? What makes nuclear reactions different from chemical reactions? The speed of nuclear
More informationFrom Last Time. Stronger than coulomb force, But much shorter range than coulomb force.
From Last Time Nucleus is small, tightly bound system of protons & neutrons. Proton number determines the element. Different isotopes have different # neutrons. Some isotopes unstable, radioactively decay
More informationCh Radioactivity. Henry Becquerel, using U-238, discovered the radioactive nature of elements in 1896.
Ch. 10 - Radioactivity Henry Becquerel, using U-238, discovered the radioactive nature of elements in 1896. Radioactivity the process in which an unstable atomic nucleus emits charged particles and energy
More informationChemistry 201: General Chemistry II - Lecture
Chemistry 201: General Chemistry II - Lecture Dr. Namphol Sinkaset Chapter 21 Study Guide Concepts 1. There are several modes of radioactive decay: (1) alpha (α) decay, (2) beta (β) decay, (3) gamma (γ)
More informationTHE NUCLEUS OF AN ATOM
VISUAL PHYSICS ONLINE THE NUCLEUS OF AN ATOM Models of the atom positive charge uniformly distributed over a sphere J. J. Thomson model of the atom (1907) ~2x10-10 m plum-pudding model: positive charge
More informationNuclear Chemistry. Transmutations and the Creation of Elements
Nuclear Chemistry Transmutations and the Creation of Elements Nuclear Fusion When two smaller elements are fused together to form a larger element. Fusion is Hard! There are two competing forces in an
More informationFission and Fusion Book pg cgrahamphysics.com 2016
Fission and Fusion Book pg 286-287 cgrahamphysics.com 2016 Review BE is the energy that holds a nucleus together. This is equal to the mass defect of the nucleus. Also called separation energy. The energy
More informationL 36 Modern Physics [3] The atom and the nucleus. Structure of the nucleus. The structure of the nucleus SYMBOL FOR A NUCLEUS FOR A CHEMICAL X
L 36 Modern Physics [3] [L36] Nuclear physics what s inside the nucleus and what holds it together what is radioactivity carbon dating [L37] Nuclear energy nuclear fission nuclear fusion nuclear reactors
More informationNuclear Physics. Radioactivity. # protons = # neutrons. Strong Nuclear Force. Checkpoint 4/17/2013. A Z Nucleus = Protons+ Neutrons
Marie Curie 1867-1934 Radioactivity Spontaneous emission of radiation from the nucleus of an unstable isotope. Antoine Henri Becquerel 1852-1908 Wilhelm Roentgen 1845-1923 Nuclear Physics A Z Nucleus =
More informationFUSION NEUTRON DEUTERIUM HELIUM TRITIUM.
FUSION AND FISSION THE SUN Nuclear Fusion Nuclear fusion is the process by which multiple nuclei join together to form a heavier nucleus. It is accompanied by the release or absorption of energy depending
More informationAtomic Quantum number summary. From last time. Na Optical spectrum. Another possibility: Stimulated emission. How do atomic transitions occur?
From last time Hydrogen atom Multi-electron atoms This week s honors lecture: Prof. Brad Christian, Positron Emission Tomography Course evaluations next week Tues. Prof Montaruli Thurs. Prof. Rzchowski
More informationNicholas J. Giordano. Chapter 30. Nuclear Physics. Marilyn Akins, PhD Broome Community College
Nicholas J. Giordano www.cengage.com/physics/giordano Chapter 30 Nuclear Physics Marilyn Akins, PhD Broome Community College Atomic Nuclei Rutherford s discovery of the atomic nucleus caused scientists
More informationStatic Electricity Lecture
Static Electricity Lecture Atoms are made of protons, which have a positive charge, and electrons, that have a negative charge. This little electron is what carries the electric current in wires. Charges
More informationNuclear Physics. PHY232 Remco Zegers Room W109 cyclotron building.
Nuclear Physics PHY232 Remco Zegers zegers@nscl.msu.edu Room W109 cyclotron building http://www.nscl.msu.edu/~zegers/phy232.html Periodic table of elements We saw that the periodic table of elements can
More informationStructure of the Nuclear Atom
Structure of the Nuclear Atom I. The II. A. The is the smallest particle of an element that retains its of the element. History of the Atom A. Democritus 1. Democritus (460 B.C. 370 B.C) was the first
More information11/19/08. Gravitational equilibrium: The outward push of pressure balances the inward pull of gravity. Weight of upper layers compresses lower layers
Gravitational equilibrium: The outward push of pressure balances the inward pull of gravity Weight of upper layers compresses lower layers Gravitational equilibrium: Energy provided by fusion maintains
More informationThe Sun. the main show in the solar system. 99.8% of the mass % of the energy. Homework due next time - will count best 5 of 6
The Sun the main show in the solar system 99.8% of the mass 99.9999...% of the energy 2007 Pearson Education Inc., publishing as Pearson Addison-Wesley Homework due next time - will count best 5 of 6 The
More informationNUCLEI, RADIOACTIVITY AND NUCLEAR REACTIONS
NUCLEI, RADIOACTIVITY AND NUCLEAR REACTIONS VERY SHORT ANSWER QUESTIONS Q-1. Which of the two is bigger 1 kwh or 1 MeV? Q-2. What should be the approximate minimum energy of a gamma ray photon for pair
More informationCard #1/28. Card #2/28. Science Revision P2. Science Revision P2. Science Revision P2. Card #4/28. Topic: F = ma. Topic: Resultant Forces
Card #1/28 Card #2/28 Topic: Resultant Forces Topic: F = ma Topic: Distance-TIme Graphs Card #3/28 Card #4/28 Topic: Velocity-Time Graphs Card #2/28 Card #1/28 Card #4/28 Card #3/28 Card #5/28 Card #6/28
More informationMidterm 2 PRS Questions
Midterm 2 PRS Questions PRS questions from the lectures after Midterm 1 but before Midterm 2 PRS Question. You want to launch a rocket into space, and you want to maximize its kinetic energy. Suppose that
More informationA. Incorrect! Do not confuse Nucleus, Neutron and Nucleon. B. Incorrect! Nucleon is the name given to the two particles that make up the nucleus.
AP Physics - Problem Drill 24: Nuclear Physics 1. Identify what is being described in each of these statements. Question 01 (1) It is held together by the extremely short range Strong force. (2) The magnitude
More informationChapter 20: Phenomena. Chapter 20: The Nucleus: A Chemist s View. Nuclear Decay. Nuclear Decay. Nuclear Decay. Nuclear Decay
Chapter 20: Phenomena Phenomena: Below is a list of stable isotopes of different elements. Examine the data and see what patterns you can identify. The mass of a electron is 0.00055 u, the mass of a proton
More informationPhysics 142 Modern Physics 2 Page 1. Nuclear Physics
Physics 142 Modern Physics 2 Page 1 Nuclear Physics The Creation of the Universe was made possible by a grant from Texas Instruments. Credit on a PBS Program Overview: the elements are not elementary The
More informationSome differences: Some basic similarities: Charges. Electrons vs. Protons 3/25/12. Chapters 22-25: Electromagnetism!
Chapters 22-25: Electromagnetism! Electric Force vs. Gravitational Force What properties does the gravitational force depend on? What properties does the electric force depend on? F grav = G*m 1 *m 2 /d
More informationLecture Presentation. Chapter 21. Nuclear Chemistry. James F. Kirby Quinnipiac University Hamden, CT Pearson Education, Inc.
Lecture Presentation Chapter 21, Inc. James F. Kirby Quinnipiac University Hamden, CT Energy: Chemical vs. Chemical energy is associated with making and breaking chemical bonds. energy is enormous in comparison.
More informationNuclear Physics. AP Physics B
Nuclear Physics AP Physics B Nuclear Physics - Radioactivity Before we begin to discuss the specifics of radioactive decay we need to be certain you understand the proper NOTATION that is used. To the
More informationChemistry 1000 Lecture 3: Nuclear stability. Marc R. Roussel
Chemistry 1000 Lecture 3: Nuclear stability Marc R. Roussel Radioactive decay series Source: Wikimedia commons, http://commons.wikimedia.org/wiki/file: Decay_Chain_Thorium.svg Forces between nucleons Electrostatic
More informationFXA Candidates should be able to :
1 Candidates should be able to : INTRODUCTION Describe qualitatively the alpha-particle scattering experiment and the evidence this provides for the existence, charge and small size of the nucleus. Describe
More informationRadioactivity. Nuclear Physics. # neutrons vs# protons Where does the energy released in the nuclear 11/29/2010 A=N+Z. Nuclear Binding, Radioactivity
Physics 1161: Lecture 25 Nuclear Binding, Radioactivity Sections 32-1 32-9 Marie Curie 1867-1934 Radioactivity Spontaneous emission of radiation from the nucleus of an unstable isotope. Antoine Henri Becquerel
More informationLecture 21 Fundamentals of Physics Phys 120, Fall 2015 Nuclear Physics
Lecture 21 Fundamentals of Physics Phys 120, Fall 2015 Nuclear Physics A. J. Wagner North Dakota State University, Fargo, ND 58102 Fargo, November 13, 2015 Overview Why care about nuclei? How do nuclei
More informationChapter 25: Radioactivity, Nuclear Processes, and Applications. What do we know about the nucleus? James Chadwick and the discovery of the neutron
Chapter 25: Radioactivity, Nuclear Processes, and Applications What do we know about the nucleus? Rutherford discovered Contains positively charged protons. Held together by the Nuclear Strong Force. The
More informationhttp://imgs.xkcd.com/comics/cell_phones.png Announcements: Thursday: Group A to Hayes 105 for hands-on experience Group B comes here to work on worksheet Both groups: bring your calculator! Next Tuesday
More informationNuclear Binding Energy
Nuclear Energy Nuclei contain Z number of protons and (A - Z) number of neutrons, with A the number of nucleons (mass number) Isotopes have a common Z and different A The masses of the nucleons and the
More informationCLASS 32. NUCLEAR BINDING ENERGY
CLASS 3. NUCLEAR BINDING ENERGY 3.. INTRODUCTION Scientists found that hitting atoms with alpha particles could induce transformations in light elements. (Recall that the capture of an alpha particle by
More informationUNIT 13: NUCLEAR CHEMISTRY
UNIT 13: NUCLEAR CHEMISTRY REVIEW: ISOTOPE NOTATION An isotope notation is written as Z A X, where X is the element, A is the mass number (sum of protons and neutrons), and Z is the atomic number. For
More informationEnergy: Forms and Changes
Energy: Forms and Changes The Energy Story Nature of Energy Energy is all around you! l You can hear energy as sound. l You can see energy as light. l And you can feel it as wind. Nature of Energy You
More informationPhysics 115 Future Physics Midterm Review Exam will be closed book; no calculators; no computers.
Physics 115 Future Physics Midterm Review 2016 Exam will be closed book; no calculators; no computers. You can bring a 3 x 5 index card with whatever notes and equations you want written on ONE SIDE ONLY.
More informationLecture 33 Chapter 22, Sections 1-2 Nuclear Stability and Decay. Energy Barriers Types of Decay Nuclear Decay Kinetics
Lecture 33 Chapter 22, Sections -2 Nuclear Stability and Decay Energy Barriers Types of Decay Nuclear Decay Kinetics Nuclear Chemistry Nuclei Review Nucleons: protons and neutrons Atomic number number
More informationMockTime.com. Ans: (b) Q6. Curie is a unit of [1989] (a) energy of gamma-rays (b) half-life (c) radioactivity (d) intensity of gamma-rays Ans: (c)
Chapter Nuclei Q1. A radioactive sample with a half life of 1 month has the label: Activity = 2 micro curies on 1 8 1991. What would be its activity two months earlier? [1988] 1.0 micro curie 0.5 micro
More informationQuantifying Radiation. Applications
Today Quantifying Radiation Applications We need to try to quantify amount of radiation How much ionizing radiation is coming from a source? How much ionizing radiation has interacted with you? How much
More information4.4 Atomic structure Notes
4.4 Atomic structure Notes Ionising radiation is hazardous but can be very useful. Although radioactivity was discovered over a century ago, it took many nuclear physicists several decades to understand
More informationN = R *! f p! n e! f l! f i! f c! L
Astronomy 330 Drake Equation The class s first estimate is Frank Drake This class (Lecture 6): Stars Next Class: Star Formation Music: We are all made of Stars Moby Feb 5, 2009 Astronomy 330 N = R *! f
More informationRadioactivity & Nuclear. Chemistry. Mr. Matthew Totaro Legacy High School. Chemistry
Radioactivity & Nuclear Chemistry Mr. Matthew Totaro Legacy High School Chemistry The Discovery of Radioactivity Antoine-Henri Becquerel designed an experiment to determine if phosphorescent minerals also
More informationQuantum Mechanics. Exam 3. Photon(or electron) interference? Photoelectric effect summary. Using Quantum Mechanics. Wavelengths of massive objects
Exam 3 Hour Exam 3: Wednesday, November 29th In-class, Quantum Physics and Nuclear Physics Twenty multiple-choice questions Will cover:chapters 13, 14, 15 and 16 Lecture material You should bring 1 page
More informationUnit 1 Atomic Structure
Unit 1 Atomic Structure Defining the Atom I. Atomic Theory A. Modern Atomic Theory 1. All matter is made up of very tiny particles called atoms 2. Atoms of the same element are chemically alike 3. Individual
More informationA Nuclear Power Plant
A Nuclear Power Plant Fallout from Chernobyl The question that all countries asked in 1986, and continue to ask to this day: Could it happen here? Radioactivity Np Pu+ 239 239 0 93 94 1 Beta decay the
More informationChapter 10. Table of Contents. Section 1 What Is Radioactivity? Section 2 Nuclear Fission and Fusion. Section 3 Nuclear Radiation Today
Nuclear Chemistry Table of Contents Section 1 What Is Radioactivity? Section 2 Nuclear Fission and Fusion Section 3 Nuclear Radiation Today Section 1 What Is Radioactivity? Bellringer Before studying about
More informationRadioactivity One of the pieces of evidence for the fact that atoms are made of smaller particles came from the work of Marie Curie
1 Nuclear Chemistry Radioactivity 2 One of the pieces of evidence for the fact that atoms are made of smaller particles came from the work of Marie Curie (1876-1934). She discovered radioactivity or radioactive
More information[1] (c) Some fruits, such as bananas, are naturally radioactive because they contain the unstable isotope of potassium-40 ( K.
(a) State, with a reason, whether or not protons and neutrons are fundamental particles....... [] (b) State two fundamental particles that can be classified as leptons.... [] (c) Some fruits, such as bananas,
More informationNuclear Chemistry. Chapter 24
Nuclear Chemistry Chapter 24 Radioactivity Radioisotopes are isotopes that have an unstable nucleus. They emit radiation to attain more stable atomic configurations in a process called radioactive decay.
More informationLec 7: Classification of Stars, the Sun. What prevents stars from collapsing under the weight of their own gravity? Text
1 Astr 102 Lec 7: Classification of Stars, the Sun What prevents stars from collapsing under the weight of their own gravity? Text Why is the center of the Sun hot? What is the source of the Sun s energy?
More informationToday. Homework Due. Stars. Properties (Recap) Nuclear Reactions. proton-proton chain. CNO cycle. Stellar Lifetimes
Today Stars Properties (Recap) Nuclear Reactions proton-proton chain CNO cycle Stellar Lifetimes Homework Due Stellar Properties Luminosity Surface Temperature Size Mass Composition Stellar Properties
More informationNuclear Reactions and E = mc 2. L 38 Modern Physics [4] Hazards of radiation. Radiation sickness. Biological effects of nuclear radiation
L 38 Modern Physics [4] Nuclear physics what s s inside the nucleus and what holds it together what is radioactivity, halflife carbon dating Nuclear energy nuclear fission nuclear fusion nuclear reactors
More informationToday The Sun. Events
Today The Sun Events Last class! Homework due now - will count best 5 of 6 Final exam Dec. 20 @ 12:00 noon here Review this Course! www.case.edu/utech/course-evaluations/ The Sun the main show in the solar
More informationDEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS
DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS TSOKOS LESSON 7-2 NUCLEAR REACTIONS Review Videos-Radioactivity2 Review Videos - Strong and Weak Nuclear Forces Essential Idea: Energy can be released
More information