Two questions from the exam
|
|
- Maurice Rafe Watkins
- 5 years ago
- Views:
Transcription
1 Two qestions from the exam 3. When the sn is located near one of the horizons, an observer looking at the sky directly overhead will view partially polarized light. This effect is de to which of the following processes? a) reflection b) refraction c) diffraction d) inteference e) scattering 4. If different filters are sed with an astronomical telescope, which of the following wold give the best resoltion? (Hint: think Rayleigh criterion.) a) red b) green c) ble d) black e) all yield the same resoltion q min = 1.22l/D ble has smallest wavelength of above (know yor spectrm)
2 Another problem 10. In hydrogen, an electron makes a transition from the n = 6 to n = 2 state. What is wavelength of the emitted photon? a) 334 nm b) 372 nm c) 410 nm d) 448 nm e) 486 nm E n = ev/n 2 E 6 = ev/36 = 0.38 ev E 2 = ev/4 = 3.4 ev E 6 -E 2 =Eg=3.02 ev=hc/l l=hc/eg=(6.62x10-34 J.s)(3X10 8 m/s) /[3.02 ev X 1.6 X10-19 J/eV)] =410 nm
3 Bands and band gaps If we have a single atom, then we ve learned abot the energy levels possible for electrons in the atom If we have many atoms close together (like in a solid), the energy levels smsh ot (technical term) into bands electrons in the solid can have energies within the bands and the energies between the bands are forbidden (band gaps) highest filled band (in grond state) is called valence band next higher empty band is called condction band
4 Condctors and inslators Sppose I apply a voltage across a condctor. What happens? Some of the electrons can accelerate and gain energy. This is possible becase the condction band is close in energy to the valence band and there are empty energy states to jmp into. This can t happen with inslators where there is too large of an energy gap between.
5 Semi-condctors In between a condctor and an inslator is a semicondctor where there is a small band gap of abot 1 ev silicon gallim arsenide The size of the band gap energy E g depends on the temperatre of the semicondctor the lower the temperatre, the smaller the band gap In a light-emitting diode, electrons jmping from the condction band back to the valence band emit a photon of energy E g E photon =hc/l l=hc/e for E~few ev, l is visible
6 Back to the ncles In 1919, Rtherford starts to collect the first data indicating that there is another strctre within the ncles- the proton. Two years later, James Chadwick and E.S. Bieler conclde that some strong force holds the ncles together. Why? If protons in ncles (and not electrons) then what keeps the replsive force from driving the ncles apart? Ncles confined to a very small volme (<10-14 m in diameter), 0.01% of diameter of atom s density is kg/m 3
7 So here we are in 1930 There were three fndamental particles- electron, proton, and photon. There were three fndamental forces- gravity, electromagnetic, and the strong nclear force. Gravity we know is mch weaker than the other forces strong force is abot 100X stronger than EM force s natrally occring elements only have p to 100 protons s strong force between protons satrates bt EM replsive force doesn t s for more than 100 protons replsive force wins There were still some details to work ot bt many felt like Max Born, who said, "Physics as we know it will be over in six months." Who is Max Borns granddaghter?
8 Olivia Newton-John as far as I know, John Travolta is not related to any famos physicist
9 The ncles l The ncles had ceased to be fndamental. It was composed of positively charged protons and netrally charged netrons (not actally discovered ntil 1931 by Chadwick).
10 Characterizing atoms Nclei of atoms consist of protons and netrons Srronding the ncles are the electrons Characterize nclei by following characteristics Atomic nmber Z: # of protons in ncles (also eqal to # electrons for normal atom) Netron nmber N: # of netrons in ncles Mass nmber A: # of ncleons (protons + netrons) in ncles A ZX : X is symbol for element, A is atomic mass and Z is atomic nmber Isotopes of an element have the same atomic nmber bt different atomic weight same nmber of protons and electrons s same chemical properties different nmber of netrons s different nclear properties
11 Masses E R = mc 2 note the factor of 2000 difference nified mass nit: 12C has a mass of 12 am 1 = X kg
12 Radis of ncles Rtherford fond an expression for how close an alpha particle can come to a ncles For a head-on collision all of kinetic energy is changed to potential energy 1 2 (2e)(Ze) 2 mv = k d d is the distance of closest approach
13 Solve for d 4kZe 2 d = mv 2 or a distance of abot 3.2 X m for alpha particles on a gold ncles From these reslts, Rtherford conclded that the positive charge in a ncles is concentrated in a sphere whose radis is no greater than ~10-14 m or abot 10 fermis (1 fermi = 1 X m) Nclear radii go as: r=r o A 1/3 A is the # of ncleons and r o =1.2X10-15 m all nclei have roghly the same density
14 The ncles can exist only becase the strong nclear force between ncleons in a ncles is stronger than the electrostatic replsive force between the protons Light elements have roghly the same nmber of protons and netrons Heavier elements have more netrons than protons (netrons contribte to the strong binding force inside the ncles bt not to the replsive EM force) Isotopes within the shaded region are stable Stable nclei
15 The heavier elements in the niverse were all made in spernova explosions Unstable isotopes are prodced (too many netrons) which then decay to the stable isotopes One of areas of concentration of NSCL (and of RIA) Unstable nclei
16 Binding Energy The total mass of a ncles is less than the sm of the masses of the protons and netrons that comprise it This difference is called the binding energy of the ncles and can be thoght of as the energy that mst be added to a ncles to break it apart iron has the highest binding energy
17 In 1896, Henri Becqerel, while investigating floresence in ranim salts, accidentally discovered radioactivity Work by Cries and others showed that radioactivity was the reslt of the decay or disintegration of nstable nclei Up til that point, atoms were believed to be indestrctible and forever Cleared p a major qestion as to why the interior of the Earth was still molten Shared the 1903 Nobel prize with the Cries Work by Cries and others showed that radioactivity was the reslt of the decay or disintegration of nstable nclei Radioactivity
18 Alpha particles are helim nclei (2 p, 2 n): Beta particles are speedy electrons: Gamma radiation is a stream of photons: Radiation these are spposed to be x s
19 Half-life If a radioactive sample contains N radioactive nclei at some instant, the nmber of nclei that decay in a time Dt is proportional to N DN/Dt a N DN = -lndt where l is a decay constant R = DN/Dt = ln rate of which atoms decay N=N o e -lt T 1/2 (half-life) is time it takes for half of sample to decay Decay constants vary greatly for different radioactive decays and ths so do halflives
What is fundamental? wwhat is it made of? whow is it all held together? The TWO most fundamental questions about the universe are: Fig. 15.1, p.
What is fndamental? The TWO most fndamental qestions abot the niverse are: wwhat is it made of? whow is it all held together? Fig. 15.1, p. 467 For Fndamental Elements l The Hnt for the answers to those
More informationCosmic rays. l Some come from the sun (relatively low energy) and some from catastrophic events elsewhere in the galaxy/universe
Special relativity The laws of physics are the same in all coordinate systems either at rest or moving at constant speed with respect to one another The speed of light in a vacm has the same vale regardless
More informationChapter 44. Nuclear Structure
Chapter 44 Nuclear Structure Milestones in the Development of Nuclear Physics 1896: the birth of nuclear physics Becquerel discovered radioactivity in uranium compounds Rutherford showed the radiation
More informationElectric and Magnetic Fields
Electric and Magnetic Fields Jst as we want to define an electric field for electrostatic forces, we also want to define a magnetic field for magnetic forces. E (nits of N/C, or V/m) B (nits of Tesla)
More informationPROBLEMS
PROBLEMS------------------------------------------------ - 7- Thermodynamic Variables and the Eqation of State 1. Compter (a) the nmber of moles and (b) the nmber of molecles in 1.00 cm of an ideal gas
More informationGeneral Physics (PHY 2140)
General Physics (PHY 140) Lecture 18 Modern Physics Nuclear Physics Nuclear properties Binding energy Radioactivity The Decay Process Natural Radioactivity Last lecture: 1. Quantum physics Electron Clouds
More informationFundamental Forces. Range Carrier Observed? Strength. Gravity Infinite Graviton No. Weak 10-6 Nuclear W+ W- Z Yes (1983)
Fundamental Forces Force Relative Strength Range Carrier Observed? Gravity 10-39 Infinite Graviton No Weak 10-6 Nuclear W+ W- Z Yes (1983) Electromagnetic 10-2 Infinite Photon Yes (1923) Strong 1 Nuclear
More informationL = 2 λ 2 = λ (1) In other words, the wavelength of the wave in question equals to the string length,
PHY 309 L. Soltions for Problem set # 6. Textbook problem Q.20 at the end of chapter 5: For any standing wave on a string, the distance between neighboring nodes is λ/2, one half of the wavelength. The
More informationParticles and fields. Today: Review Particle Physics. Question. Quantum Electrodynamics: QED. Electrons and photons
Exam 4: Fri. May 10, in-class 20 qestions, covers fission, fsion, particle physics No final exam. Essays retrne Friay Toay: Review Particle Physics Particles an fiels: a new pictre Qarks an leptons The
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 informationUniversity of California, Berkeley Physics H7C Fall 1999 (Strovink) SOLUTION TO FINAL EXAMINATION
University of California Berkeley Physics H7C Fall 999 (Strovink SOUTION TO FINA EXAMINATION Directions. Do all six problems (weights are indicated. This is a closed-book closed-note exam except for three
More informationV. Hadron quantum numbers
V. Hadron qantm nmbers Characteristics of a hadron: 1) Mass 2) Qantm nmbers arising from space-time symmetries : total spin J, parity P, charge conjgation C. Common notation: 1 -- + 2 J P (e.g. for proton:
More informationUNIT-VIII ATOMIC NUCLEUS 1) what conclusions were drawn from the observation in which few alpha-particle were seen rebounding from gold foil? 2) which observation led to the conclusion in the α-particle
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 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 informationEXCITATION RATE COEFFICIENTS OF MOLYBDENUM ATOM AND IONS IN ASTROPHYSICAL PLASMA AS A FUNCTION OF ELECTRON TEMPERATURE
EXCITATION RATE COEFFICIENTS OF MOLYBDENUM ATOM AND IONS IN ASTROPHYSICAL PLASMA AS A FUNCTION OF ELECTRON TEMPERATURE A.N. Jadhav Department of Electronics, Yeshwant Mahavidyalaya, Ned. Affiliated to
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 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 informationCHAPTER 12 The Atomic Nucleus
CHAPTER 12 The Atomic Nucleus 12.1 Discovery of the Neutron 12.2 Nuclear Properties 12.3 The Deuteron 12.4 Nuclear Forces 12.5 Nuclear Stability 12.6 Radioactive Decay 12.7 Alpha, Beta, and Gamma Decay
More informationPhys102 Lecture 29, 30, 31 Nuclear Physics and Radioactivity
Phys10 Lecture 9, 30, 31 Nuclear Physics and Radioactivity Key Points Structure and Properties of the Nucleus Alpha, Beta and Gamma Decays References 30-1,,3,4,5,6,7. Atomic Structure Nitrogen (N) Atom
More informationFisika Inti Nuclear Physics 5/14/2010 1
Fisika Inti Nuclear Physics 5/14/2010 1 Pengertian Modern: Gambar onion Modern understanding: the ``onion picture Atom Let s see what s inside! 5/14/2010 2 Pengertian Modern: Gambar onion Modern understanding:
More informationChapter 4. The structure of the atom. AL-COS Objectives 1, 2,3,4,7, 10, 15, 20, 21, 22, 27and 28
Chapter 4 The structure of the atom AL-COS Objectives 1, 2,3,4,7, 10, 15, 20, 21, 22, 27and 28 You ll learn to Identify the experiments that led to the development of the nuclear model of atomic structure
More informationPhysics 3204 UNIT 3 Test Matter Energy Interface
Physics 3204 UNIT 3 Test Matter Energy Interface 2005 2006 Time: 60 minutes Total Value: 33 Marks Formulae and Constants v = f λ E = hf h f = E k + W 0 E = m c 2 p = h λ 1 A= A T 0 2 t 1 2 E k = ½ mv 2
More informationSlide 1 / 57. Nuclear Physics & Nuclear Reactions Practice Problems
Slide 1 / 57 Nuclear Physics & Nuclear Reactions Practice Problems Slide 2 / 57 Multiple Choice Slide 3 / 57 1 The atomic nucleus consists of: A B C D E Electrons Protons Protons and electrons Protons
More informationQuantum Physics and Atomic Models Chapter Questions. 1. How was it determined that cathode rays possessed a negative charge?
Quantum Physics and Atomic Models Chapter Questions 1. How was it determined that cathode rays possessed a negative charge? 2. J. J. Thomson found that cathode rays were really particles, which were subsequently
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 informationMultiple Choice Questions
Nuclear Physics & Nuclear Reactions Practice Problems PSI AP Physics B 1. The atomic nucleus consists of: (A) Electrons (B) Protons (C)Protons and electrons (D) Protons and neutrons (E) Neutrons and electrons
More informationPSI AP Physics How was it determined that cathode rays possessed a negative charge?
PSI AP Physics 2 Name Chapter Questions 1. How was it determined that cathode rays possessed a negative charge? 2. J. J. Thomson found that cathode rays were really particles, which were subsequently named
More informationn 1 sin 1 n 2 sin 2 Light and Modern Incident ray Normal 30.0 Air Glass Refracted ray speed of light in vacuum speed of light in a medium c v
Light and Modern E hf n speed of light in vacm speed of light in a medim c v n sin n sin Incident ray Normal TIP. The reqency Remains the Same The freqency of a wave does not change as the wave passes
More informationChapter 29. Nuclear Physics
Chapter 29 Nuclear Physics Ernest Rutherford 1871 1937 Discovery that atoms could be broken apart Studied radioactivity Nobel prize in 1908 Some Properties of Nuclei All nuclei are composed of protons
More informationDEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS
DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS TSOKOS LESSON 6-6 NUCLEAR PHYSICS IB Assessment Statements Topic 13.2, Nuclear Physics 13.2.1. Explain how the radii of nuclei may be estimated from
More informationEarly Atomic Theories and the Origins of Quantum Theory. Chapter 3.1
Early Atomic Theories and the Origins of Quantum Theory Chapter 3.1 What is Matter Made of? People have wondered about the answer to this question for thousands of years Philosophers Matter is composed
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 informationUNIT VIII ATOMS AND NUCLEI
UNIT VIII ATOMS AND NUCLEI Weightage Marks : 06 Alpha-particles scattering experiment, Rutherford s model of atom, Bohr Model, energy levels, Hydrogen spectrum. Composition and size of Nucleus, atomic
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 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 4 The Atom. Philosophers and scientists have proposed many ideas on the structure of atoms.
Chapter4 TheAtom 4.1 Early Models of the Atom An atom is the smallest particle of an element that retains its identity in a chemical reaction. Philosophers and scientists have proposed many ideas on the
More informationThe wavefunction ψ for an electron confined to move within a box of linear size L = m, is a standing wave as shown.
1. This question is about quantum aspects of the electron. The wavefunction ψ for an electron confined to move within a box of linear size L = 1.0 10 10 m, is a standing wave as shown. State what is meant
More informationNuclear Properties. Thornton and Rex, Ch. 12
Nuclear Properties Thornton and Rex, Ch. 12 A pre-history 1896 Radioactivity discovered - Becquerel a rays + (Helium) b rays - (electrons) g rays 0 (EM waves) 1902 Transmutation observed - Rutherford and
More informationNuclear Powe. Bronze Buddha at Hiroshima
Nuclear Powe Bronze Buddha at Hiroshima Nuclear Weapons Nuclear Power Is it Green & Safe? Nuclear Waste 250,000 tons of Spent Fuel 10,000 tons made per year Health Effects of Ionizing Radiation Radiocarbon
More informationBasic science. Atomic structure. Electrons. The Rutherford-Bohr model of an atom. Electron shells. Types of Electrons. Describing an Atom
Basic science A knowledge of basic physics is essential to understanding how radiation originates and behaves. This chapter works through what an atom is; what keeps it stable vs. radioactive and unstable;
More informationThursday, April 23, 15. Nuclear Physics
Nuclear Physics Some Properties of Nuclei! All nuclei are composed of protons and neutrons! Exception is ordinary hydrogen with just a proton! The atomic number, Z, equals the number of protons in the
More informationMIDTERM 3 REVIEW SESSION. Dr. Flera Rizatdinova
MIDTERM 3 REVIEW SESSION Dr. Flera Rizatdinova Summary of Chapter 23 Index of refraction: Angle of reflection equals angle of incidence Plane mirror: image is virtual, upright, and the same size as the
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 information16.5 Coulomb s Law Types of Forces in Nature. 6.1 Newton s Law of Gravitation Coulomb s Law
5-10 Types of Forces in Nature Modern physics now recognizes four fundamental forces: 1. Gravity 2. Electromagnetism 3. Weak nuclear force (responsible for some types of radioactive decay) 4. Strong nuclear
More informationThe Nucleus. PHY 3101 D. Acosta
The Nucleus PHY 30 D. Acosta Rutherford Scattering Experiments by Geiger & Marsden in 909 /5/005 PHY 30 -- D. Acosta Rutherford Model of the Atom Conclusion: the atom contains a positive nucleus < 0 fm
More informationChapter 3. Radioactivity. Table of Contents
Radioactivity Table of Contents Introduction 1. Radioactivity 2. Types of Radioactive Decays 3. Natural Radioactivity 4. Artificial Radioactivity 5. The Rate of Radioactive Decay 6. The Effects of Radiation
More information= : K A
Atoms and Nuclei. State two limitations of JJ Thomson s model of atom. 2. Write the SI unit for activity of a radioactive substance. 3. What observations led JJ Thomson to conclusion that all atoms have
More informationNuclear Properties. Thornton and Rex, Ch. 12
Nuclear Properties Thornton and Rex, Ch. 12 A pre-history 1896 Radioactivity discovered - Becquerel a rays + (Helium) b rays - (electrons) g rays 0 (EM waves) 1902 Transmutation observed - Rutherford and
More informationIllustrations of a Modified Standard Model: Part 1-The Solar Proton- Proton Cycle
Illstrations of a Modified : Part 1-The Solar Proton- Proton Cycle by Roger N. Weller, (proton3@gmail.com), Febrary 23, 2014 Abstract A proposed modification of the, when applied to the Solar Proton-Proton
More informationUnit 2 Atomic Structure and Nuclear Chemistry
Chemistry 1 West Linn High School Unit 2 Packet and Goals Name: Period: Unit 2 Atomic Structure and Nuclear Chemistry Unit Goals: As you work through this unit, you should be able to: 1. describe Dalton
More information3/29/2010. Structure of the Atom. Knowledge of atoms in 1900 CHAPTER 6. Evidence in 1900 indicated that the atom was not a fundamental unit:
3/9/010 CHAPTER 6 Rutherford Scattering 6.1 The Atomic Models of Thomson and Rutherford 6. Definition of Cross Section 6. Rutherford Scattering 6.3 Structure of the Nucleus The opposite of a correct statement
More informationNUCLEI. Atomic mass unit
13 NUCLEI Atomic mass unit It is a unit used to express the mass of atoms and particles inside it. One atomic mass unit is the mass of atom. 1u = 1.660539 10. Chadwick discovered neutron. The sum of number
More informationNUCLEAR STRUCTURE AND RADIOACTIVITY
Chapter 12 NUCLEAR STRUCTURE AND RADIOACTIVITY Radioactive isotopes have proven to be valuable tools for medical diagnosis. The photo shows gamma-ray emission from a man who has been treated with a radioactive
More informationModern Physics. Overview
Modern Physics Overview History ~1850s Classical (Newtonian) mechanics could not explain the new area of investigation atomic physics Macro vs Micro New field of Quantum Mechanics, focused on explaining
More informationVI. The quark model: hadron quantum numbers, resonances
VI. The qark model: hadron qantm nmbers, resonances Characteristics of a hadron: 1) Mass 2) Qantm nmbers arising from space symmetries : J, P, C. Common notation: J P (e.g. for proton: 1 2 --+ ), or J
More informationNuclear Chemistry. In this chapter we will look at two types of nuclear reactions.
1 1 Nuclear Chemistry In this chapter we will look at two types of nuclear reactions. Radioactive decay is the process in which a nucleus spontaneously disintegrates, giving off radiation. Nuclear bombardment
More informationChemistry 6A F2007. Dr. J.A. Mack 12/3/07. What do I need to bring? Exam 3: Friday 12/7/07 (here in lecture)
Chemistry 6A F2007 Dr. J.A. Mack Exam 3: Friday 12/7/07 (here in lecture) What will be covered on the exam? Chapter 6: 6.9-6.15 Chapter 7: All Chapter 8: All Chapter 9: 9.1-9.9 Any thing from lab as well
More informationNuclear Physics Part 1: Nuclear Structure & Reactions
Nuclear Physics Part 1: Nuclear Structure & Reactions Last modified: 25/01/2018 Links The Atomic Nucleus Nucleons Strong Nuclear Force Nuclei Are Quantum Systems Atomic Number & Atomic Mass Number Nuclides
More informationmolar mass = 0.239kg (1) mass needed = = kg (1) [7]
PhysicsAndMathsTutor.com 1 1. (a) (i) proton number 82 and nucleon number 214 (ii) Pb 2 (b) (i) kinetic energy [or electrostatic potential energy] (ii) m = 8.6 E 2 c 1 10 = 8 2 (10 ) = 9.6 10 0 kg [5]
More informationNuclear Chemistry. Radioactivity. In this chapter we will look at two types of nuclear reactions.
1 Nuclear Chemistry In this chapter we will look at two types of nuclear reactions. Radioactive decay is the process in which a nucleus spontaneously disintegrates, giving off radiation. Nuclear bombardment
More information25.1. Nuclear Radiation
Nuclear Radiation Marie Curie was a Polish scientist whose research led to many discoveries about radiation and radioactive elements. In 1934 she died from leukemia caused by her long-term exposure to
More informationAtoms, nuclei, particles
Atoms, nuclei, particles Nikolaos Kidonakis Physics for Georgia Academic Decathlon September 2016 Age-old questions What are the fundamental particles of matter? What are the fundamental forces of nature?
More informationThe diagram below shows a radioactive isotope going through several half-lives as it decays.
By what process do most stars release energy? A. Electromagnetic induction resulting from strong magnetic fields B. Radioactivity in the interior of the star C. Nuclear fusion in the interior of the star
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 informationNuclear Properties. Thornton and Rex, Ch. 12
Nuclear Properties Thornton and Rex, Ch. 12 A pre-history 1896 Radioactivity discovered - Becquerel a rays + (Helium) b rays - (electrons) g rays 0 (EM waves) 1902 Transmutation observed - Rutherford and
More informationAnswerIT! Atoms and isotopes. Structure of an atom Mass number, atomic number and isotopes Development of the model of the atom.
AnswerIT! Atoms and isotopes Structure of an atom Mass number, atomic number and isotopes Development of the model of the atom. Atoms and isotopes - AnswerIT 1. The diameter of an atom is about 0.000 000
More informationThe Atom. Result for Hydrogen. For example: the emission spectrum of Hydrogen: Screen. light. Hydrogen gas. Diffraction grating (or prism)
The Atom What was know about the atom in 1900? First, the existence of atoms was not universally accepted at this time, but for those who did think atoms existed, they knew: 1. Atoms are small, but they
More informationChapter 3 Radioactivity
Chapter 3 Radioactivity Marie Curie 1867 1934 Discovered new radioactive elements Shared Nobel Prize in physics in 1903 Nobel Prize in Chemistry in 1911 Radioactivity Radioactivity is the spontaneous emission
More informationGreek Philosophers (cont.)
Greek Philosophers (cont.) Many ancient scholars believed matter was composed of such things as earth, water, air, and fire. Many believed matter could be endlessly divided into smaller and smaller pieces.
More informationPhysics 107 Final Exam December 13, Your Name: Questions
Physics 107 Final Exam December 13, 1993 Your Name: Questions 1. 11. 21. 31. 41. 2. 12. 22. 32. 42. 3. 13. 23. 33. 43. 4. 14. 24. 34. 44. 5. 15. 25. 35. 45. 6. 16. 26. 36. 46. 7. 17. 27. 37. 47. 8. 18.
More informationPHY293 Lecture #15. November 27, Quantum Mechanics and the Atom
PHY293 Lecture #15 November 27, 2017 1. Quantum Mechanics and the Atom The Thompson/Plum Pudding Model Thompson discovered the electron in 1894 (Nobel Prize in 1906) Heating materials (metals) causes corpuscles
More informationDownloaded from
constant UNIT VIII- ATOMS & NUCLEI FORMULAE ANDSHORTCUT FORMULAE. Rutherford s -Particle scattering experiment (Geiger Marsden experiment) IMPOTANT OBSERVATION Scattering of -particles by heavy nuclei
More informationPARTICLE PHYSICS :Higher Level Long Questions
PARTICLE PHYSICS :Higher Level Long Questions Particle Accelerators (including Cockcroft and Walton experiment) 2013 Question 10 (a) In 1932 J.D. Cockroft and E.T.S. Walton accelerated protons to energies
More information5. The Bernoulli Equation
5. The Bernolli Eqation [This material relates predominantly to modles ELP034, ELP035] 5. Work and Energy 5. Bernolli s Eqation 5.3 An example of the se of Bernolli s eqation 5.4 Pressre head, velocity
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 informationThe Hydrogen Atom According to Bohr
The Hydrogen Atom According to Bohr The atom We ve already talked about how tiny systems behave in strange ways. Now let s s talk about how a more complicated system behaves. The atom! Physics 9 4 Early
More information6. Atomic and Nuclear Physics
6. Atomic and Nuclear Physics Chapter 6.2 Radioactivity From IB OCC, prepared by J. Domingues based on Tsokos Physics book Warm Up Define: nucleon atomic number mass number isotope. Radioactivity In 1896,
More informationChapter 28. Atomic Physics
Chapter 28 Atomic Physics Sir Joseph John Thomson J. J. Thomson 1856-1940 Discovered the electron Did extensive work with cathode ray deflections 1906 Nobel Prize for discovery of electron Early Models
More informationCHEMISTRY. Matter and Change. Table Of Contents. Section 4.1 Early Ideas About Matter. Unstable Nuclei and Radioactive Decay
CHEMISTRY 4 Table Of Contents Matter and Change Section 4.1 Early Ideas About Matter Chapter 4: The Structure of the Atom Section 4.2 Section 4.3 Section 4.4 Defining the Atom How Atoms Differ Unstable
More informationAtomic Theory. Developing the Nuclear Model of the Atom. Saturday, January 20, 18
Atomic Theory Developing the Nuclear Model of the Atom Democritus Theory: Atom, the indivisible particle c. 300 BC Democritus Problem: No scientific evidence c. 300 BC Dalton Theory: The solid sphere model
More informationLECTURE 23 NUCLEI. Instructor: Kazumi Tolich
LECTURE 23 NUCLEI Instructor: Kazumi Tolich Lecture 23 2 Reading chapter 32.1 to 32.2 Nucleus Radioactivity Mass and energy 3 The famous equation by Einstein tells us that mass is a form of energy. E =
More information7.1 Atomic Theory and Radioactive Decay
7.1 Atomic Theory and Radioactive Decay exists all around us. This radiation consists of high energy particles or waves being emitted from a variety of materials. is the release of high energy particles
More informationAn Interpretation of the Black Energy in Universe by Using a Hydro-Dynamical Analogy with Newton Gravity
An Interpretation of the Black nergy in Universe by Using a Hydro-Dynamical Analogy with Newton Gravity Corneli BRBNT*,1, Sorin BRBNT *Corresponding athor *,1 POLITHNICA University of Bcharest, Faclty
More informationPhysics 30: Chapter 8 Exam Nuclear
Physics 30: Chapter 8 Exam Nuclear Name: Date: Mark: /34 Numeric Response. Place your answers to the numeric response questions, with units, in the blanks at the side of the page. (1 mark each) 1. A 100
More informationConcepTest PowerPoints
ConcepTest PowerPoints Chapter 30 Physics: Principles with Applications, 6 th edition Giancoli 2005 Pearson Prentice Hall This work is protected by United States copyright laws and is provided solely for
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 informationQuestions Q1. * Rutherford designed an experiment to see what happened when alpha particles were directed at a piece of gold foil. Summarise the observations and state the conclusions Rutherford reached
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 informationEMISSION AND ABSORPTION SPECTRUM
EMISSION AND ABSORPTION SPECTRUM Topic 7: Atomic, nuclear and particle physics 7.1 Discrete energy and radioactivity Essential idea: In the microscopic world energy is discrete. Nature of science: Accidental
More informationAstro 1010 Planetary Astronomy Sample Questions for Exam 2
Astro 1010 Planetary Astronomy Sample Questions for Exam 2 Chapter 4 1. The Universal Law of Gravitation says that every particle of matter in the universe attracts every other particle with a force that
More informationNuclear Chemistry. The Nucleus. Isotopes. Slide 1 / 43. Slide 2 / 43. Slide 3 / 43
Slide 1 / 43 Nuclear Chemistry The Nucleus Slide 2 / 43 Remember that the nucleus is comprised of the two nucleons, protons and neutrons. The number of protons is the atomic number. The number of protons
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 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 informationSCIENCE 10: (7.1) ATOMIC THEORY, ISOTOPES AND RADIOACTIVE DECAY Name: Date: Block: (Textbook Reference pp in BC Science 10) into an
SCIENCE 10: (7.1) ATOMIC THEORY, ISOTOPES AND RADIOACTIVE DECAY Name: Date: Block: (Textbook Reference pp. 286-301 in BC Science 10) Natural background radiation: It has the ability to interact with an
More informationOverview of particle physics
Overview of particle physics The big qestions of particle physics are 1. What is the niverse mae of? 2. How is it hel together? We can start at orinary istances an work or way own. Macroscopic stff is
More informationComplete nomenclature for electron orbitals
Complete nomenclature for electron orbitals Bohr s model worked but it lacked a satisfactory reason why. De Broglie suggested that all particles have a wave nature. u l=h/p Enter de Broglie again It was
More informationPhysics 107: Ideas of Modern Physics
Physics 107: Ideas of Modern Physics Exam 3 Apr. 19, 2006 Name ID # Section # On the Scantron sheet, 1) Fill in your name 2) Fill in your student ID # (not your social security #) 3) Fill in your section
More informationPhysics 107: Ideas of Modern Physics
Physics 107: Ideas of Modern Physics Exam 3 Apr. 19, 2006 Name ID # Section # On the Scantron sheet, 1) Fill in your name 2) Fill in your student ID # (not your social security #) 3) Fill in your section
More informationThe birth of atomic physics and quantum mechanics. Honors Physics Don Rhine
The birth of atomic physics and quantum mechanics Honors Physics Don Rhine Constants & Atomic Data Look inside back cover of book! Speed of Light (vacuum): c = 3.00 x 10 8 m/s Elementary Charge: e - =
More information