Physics 213 General Physics

Slides:



Advertisements
Similar presentations
Aim: How can we explain energy transitions in an atom? Do Now: What were the limitations of the Rutherford model of the atom and how did the Bohr model.
Advertisements

e-e- E n eV n = 1 ground state n = 3 0 n = ∞ n = n = 4 ionisation N.B. All energies are NEGATIVE. REASON: The maximum energy.
1 My Chapter 27 Lecture. 2 Chapter 27: Early Quantum Physics and the Photon Blackbody Radiation The Photoelectric Effect Compton Scattering Early Models.
What do you see? Old woman? Or young girl?  Is turning a light on and off a chemical or physical change? ◦ Physical change  What creates light?
Electron Arrangement. Assessment statementTeacher’s notes 2.3.1Describe the electromagnetic spectrum.Students should be able to identify the ultraviolet,
Announcements First project is due in two weeks. In addition to a short (~10 minute) presentation you must turn in a written report on your project Homework.
The Hydrogen Spectrum Experiment 6 amplitude Wavelength -λ.
Review. The Wave Nature of Light Important: When a light wave travels from one medium to another, its frequency does not change, but its wavelength does.
Phys 102 – Lecture 25 The quantum mechanical model of light.
Chapter 45 The Nature of Light. Light Particle (photon) Wave (electromagnetic wave) Interference Diffraction Polarization.
Vacuum tube - V, only for shorter than certain wavelength Current V VoVo Fixed wavelength Varying intensity I2I 3I Maximum electron energy 0.
Classical vs Quantum Mechanics Rutherford’s model of the atom: electrons orbiting around a dense, massive positive nucleus Expected to be able to use classical.
Astronomy 100 Tuesday, Thursday 2:30 - 3:45 pm Tom Burbine
Assigned Reading Today’s assigned reading is: –Finish Chapter 7.
Wave Nature of Light and Quantum Theory
The Electromagnetic Spectrum and Light. Wavelength - The distance between two consecutive peaks of a wave.
HYDROGEN ATOM AND SPECTROSCOPY.. Energy Levels for the Hydrogen atom.
Section 5.3 Physics and the Quantum Mechanical Model
Astronomy Chapter 4 Review Game
the photoelectric effect. line spectra emitted by hydrogen gas
21 Sep 2000ASTR103, GMU, Dr. Correll1 Ch 04--Origin and Nature of Light.
Chapter 5: Light.
Sunbeds and stars... Ionization, excitation and line spectra.
In an experiment to demonstrate the photoelectric effect, you shine a beam of monochromatic blue light on a metal plate. As a result, electrons are emitted.
Wave property of light Waves can carry energy Wavelength ( ) : distance between successive crests (or troughs) Frequency (f): # of waves passing a point.
Spectra What determines the “color” of a beam of light? The answer is its frequency, or equivalently, its wavelength. We see different colors because.
Light l The study of light led to the development of the quantum mechanical model. l Light is a kind of electromagnetic radiation. l Electromagnetic radiation.
Light Waves and Particle Characteristics. Parts of a Wave = wavelength (lambda) =frequency(nu)
Modern Physics Quantum Effects 1773 – 1829 Objectives  Explain the photoelectric effect and recognize that quantum theory can explain it, but wave theory.
Problems with Rutherford’s Model Why do elements produce spectral lines instead of a continuous spectrum? And Why aren’t the negative electrons pulled.
Lecture 10: Light & Distance & Matter Astronomy 1143 – Spring 2014.
Electromagnetic radiation – transmission of energy through space in the form of oscillating waves wavelength, – distance between identical points on successive.
Quantum Theory and the Atom In the early 1900s, scientists observed certain elements emitted visible light when heated in a flame. Analysis of the emitted.
Light is a Particle Physics 12.
Chem-To-Go Lesson 7 Unit 2 ENERGY OF ELECTRONS. ENERGY BASICS All energy travels in the form of a wave. Scientists measure the wavelength of a wave to.
Examples A star radiates as a blackbody at a temperature of 1700 K. At what wavelength does the peak of the blackbody spectrum occur? If you were to look.
1© Manhattan Press (H.K.) Ltd Quantum theory.
Quantum Theory and the Electronic Structure of Atoms Chapter 7.
The Quantum-Mechanical
PHYS 172: Modern Mechanics Lecture 14 – Energy Quantization Read Summer 2012.
CH Explaining a Continuous Spectrum (called a blackbody spectrum)
Electrons in Atoms Chapter 4.
Plan for Today (AP Physics 2) Questions on HW (due tomorrow) Notes/Lecture on Blackbody Radiation.
The Solar System Lesson2 Q & A
Chapter 5 Electrons In Atoms 5.3 Atomic Emission Spectra
Still have a few registered iclickers (3 or 4
Chapter 6 Electronic Structure of Atoms
Chapter 6 Electronic Structure of Atoms
Bohr Model Of Atom.
Bohr Model Of Atom.
Quantum Theory and the Electronic Structure of Atoms
Atomic Structure.
Physics 213 General Physics
The Bohr Model (1913) revolve sun energy
Stars and Galaxies Lesson2 Q & A
Chapter 27 Early Quantum Theory
Chapter 4 Preview Multiple Choice Short Answer Extended Response
Light Practice Problems
I. Waves & Particles (p ) Ch. 4 - Electrons in Atoms I. Waves & Particles (p )
Orbits and Line Spectra
QM2 Concept Test 8.1 The total energy for distinguishable particles in a three dimensional harmonic oscillator potential
FLAME TEST.
Light and Matter Chapter 2.
The Quantum-Mechanical
Electromagnetic Radiation
Quantum Theory.
Chapter 5 Electrons In Atoms 5.3 Atomic Emission Spectra
5.1 – ELECTRONS IN ATOMS.
Ch. 5 - Electrons in Atoms Waves & Particles.
Light and EM Spectrum Light is all thanks to electrons…well… photons…but whatever. What do you REALLY know about light?
Presentation transcript:

Physics 213 General Physics Physics 213 General Physics Final Review 1 Demos: Model Door with Spring Meter; Rope Pulls Door Handle; Pivoting Rectangle with Strings; Falling Weight Rotates Pulley Videos: none Transparencies: Net Torque (Problem); Two Blocks and Pulley (Problem)

A hydrogen atom in the ground state absorbs a 12. 75-eV photon A hydrogen atom in the ground state absorbs a 12.75-eV photon. To what level is the electron promoted? (The ionization energy of hydrogen is 13.6-eV). n=2 n=3 n=4 n=5 n=6

The quantum mechanical model of the hydrogen atom requires that if the orbital quantum number = 5 for a specific principal quantum number state, how many possible substates exist for that specific orbital? 5 8 10 11 22

Which of the following transitions in hydrogen from an initial state (ni) to a final state (nf) results in the most energy emitted? (a) ni = 80, nf = 2 (b) ni = 3, nf = 95 (c) ni = 2, nf = 1 (d) ni = 1, nf = 3 (e) ni = 95, nf = 3

A flame emits light as an ideal blackbody A flame emits light as an ideal blackbody. When is the flame hotter; when it glows red or blue?

If the flame is at a temperature such that it is mostly emitting red visible light, we can assume all of the visible photons have a wavelength of approximately 630 nm. If the power of visible light emitted by the flame is 2 watts, approximately how many visible photons per second are emitted by the flame? (h = 6.63 x 10-34 Js = 4.14 x 10-15 eVs, c=3 x 108 m/s)

Surface #1 has work function j1, and when bombarded with photons of wavelength l1 emits photoelectrons with maximum energy KE1. Surface #2 has work function j2, and when bombarded by photons of wavelength l2 emits photoelectrons with maximum energy KE2. If j1 > j2, then which of the following must be true? KE1 > KE2 l1 > l2 lC for surface #1 is greater than lC for surface #2. lC for surface #2 is greater than lC for surface #1. None of the above.

As the temperature of a radiation emitting blackbody becomes higher, what happens to the peak wavelength of the radiation? Increases. Decreases. Remains constant. It is directly proportional to temperature. None of the above.

A mass is bouncing on the end of a spring with a period T when measured by a ground observer. What would the period of oscillation be (as measured by the same observer) if the mass and spring were moving past the ground observer at a speed of 0.80 c? 0.44 T 0.60 T 1.0 T 1.7 T 2.7 T

How fast would a rocket have to move past a ground observer if the latter were to observe a 4.0% length shrinkage in the rocket length? (c = 3.00  108 m/s) 0.12  108 m/s 0.28  108 m/s 0.85  108 m/s 1.2  108 m/s 3.1  108 m/s

A given individual is able to see objects clearly only when they are beyond 100 cm. If this person would like to be able to read text held as close as 25.0 cm from their eye, what focal length eye glasses should be used? 100 cm 25.0 cm 75.0 cm 100 cm 33.3 cm