Wednesday, Sept. 26, 2012 PHYS 3313-001, Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #9 Wednesday, Sept. 26, 2012 Dr. Jaehoon Yu The Bohr.

Slides:



Advertisements
Similar presentations
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
Advertisements

Cphys351 c4:1 Chapter 4: Atomic Structure The Nuclear Atom The Atom as the smallest division of an element quantization of electric charge oil drop experiments.
1 My Chapter 27 Lecture. 2 Chapter 27: Early Quantum Physics and the Photon Blackbody Radiation The Photoelectric Effect Compton Scattering Early Models.
Quantum Physics ISAT 241 Analytical Methods III Fall 2003 David J. Lawrence.
Early Quantum Theory and Models of the Atom
1 Light as a Particle The photoelectric effect. In 1888, Heinrich Hertz discovered that electrons could be ejected from a sample by shining light on it.
Monday, Oct. 1, 2012PHYS , Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #10 Monday, Oct. 1, 2012 Dr. Jaehoon Yu Importance of Bohr’s.
 When a gas in a tube is subjected to a voltage, the gas ionizes, and emits light.  We can analyze that light by looking at it through a spectroscope.
Monday, Sept. 24, 2012PHYS , Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #8 Monday, Sept. 24, 2012 Dr. Jaehoon Yu Atomic Model of.
Physics Lecture 9 2/23/ Andrew Brandt Monday February 23, 2009 Dr. Andrew Brandt 1.The Electron 2.Rutherford Scattering 3.Bohr Model of.
1 Light as a Particle In 1888, Heinrich Hertz discovered that electrons could be ejected from a sample by shining light on it. This is known as the photoelectric.
Physics at the end of XIX Century Major Discoveries of XX Century
1.The Atomic Models of Thomson and Rutherford 2.Rutherford Scattering 3.The Classical Atomic Model 4.The Bohr Model of the Hydrogen Atom 5.Successes &
Spectra of Atoms When an atom is excited, it emits light. But not in the continuous spectrum as blackbody radiation! The light is emitted at discrete wavelengths.
Dr. Jie ZouPHY Chapter 42 Atomic Physics. Dr. Jie ZouPHY Outline Atomic spectra of gases Early models of the atom Bohr’s model of the hydrogen.
Quantum Physics. Black Body Radiation Intensity of blackbody radiation Classical Rayleigh-Jeans law for radiation emission Planck’s expression h =
4.1The Atomic Models of Thomson and Rutherford 4.2Rutherford Scattering 4.3The Classic Atomic Model 4.4The Bohr Model of the Hydrogen Atom 4.5Successes.
Cutnell/Johnson Physics 7 th edition Classroom Response System Questions Chapter 39 More about Matter Waves Reading Quiz Questions.
4.1The Atomic Models of Thomson and Rutherford 4.2Rutherford Scattering 4.3The Classic Atomic Model 4.4The Bohr Model of the Hydrogen Atom 4.5Successes.
Physics 1C Lecture 29A.
CHAPTER 4 Structure of the Atom
Chapter 39 Particles Behaving as Waves
PA 114 Waves and Quanta Unit 4: Revision PA1140 Waves and Quanta Unit 4: Revision Dr Matt Burleigh (S4)
Chapter 10: Modern atomic theory Chemistry 1020: Interpretive chemistry Andy Aspaas, Instructor.
Young/Freeman University Physics 11e. Ch 38 Photons, Electrons, and Atoms © 2005 Pearson Education.
Midterm results will be posted downstairs (by the labs) this afternoon No office hours today.
1 PHYS 3313 – Section 001 Lecture #11 Wednesday, Feb. 19, 2014 Dr. Jaehoon Yu Pair production/Pair annihilation Atomic Model of Thomson Rutherford Scattering.
1 PHYS 3313 – Section 001 Lecture #10 Monday, Feb. 17, 2014 Dr. Jaehoon Yu Photoelectric Effect Compton Effect Pair production/Pair annihilation Monday,
CHAPTER 4 Structure of the Atom
1 PHYS 3313 – Section 001 Lecture #9 Wednesday, Feb. 12, 2014 Dr. Jaehoon Yu Determination of Electron Charge Line Spectra Blackbody Radiation Wednesday,
Monday, March 23, 2015PHYS , Spring 2014 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #13 Monday, March 23, 2015 Dr. Jaehoon Yu Bohr Radius.
28.3 THE BOHR THEORY OF HYDROGEN At the beginning of the 20th century, scientists were puzzled by the failure of classical physics to explain the characteristics.
Nuclear Atom and Atomic Spectra Physics Montwood High School R. Casao.
Chapter 28:Atomic Physics
Rutherford’s Model: Conclusion Massive nucleus of diameter m and combined proton mass equal to half of the nuclear mass Planetary model: Electrons.
Chapter 7. Electromagnetic Radiation  aka. Radiant energy or light  A form of energy having both wave and particle characteristics  Moves through a.
1 PHYS 3313 – Section 001 Lecture #15 Monday, Mar. 17, 2014 Dr. Jaehoon Yu Atomic Excitation by Electrons X-ray Scattering Bragg’s Law De Broglie Waves.
Physics Lecture 7 Wednesday February 10, 2010 Dr. Andrew Brandt
1 PHYS 3313 – Section 001 Lecture #14 Monday, Mar. 3, 2014 Dr. Jaehoon Yu Bohr’s Hydrogen Model and Its Limitations Characteristic X-ray Spectra Hydrogen.
4: Introduction to Quantum Physics
Electrons in Atoms Light is a kind of electromagnetic radiation. All forms of electromagnetic radiation move at 3.00 x 10 8 m/s. The origin is the baseline.
Wednesday, Feb. 25, 2015 PHYS , Spring 2014 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #10 Wednesday, Feb. 25, 2015 Dr. Jaehoon Yu Blackbody.
PHYS 3313 – Section 001 Lecture #11
Chapter 38C - Atomic Physics © 2007 Properties of Atoms Atoms are stable and electrically neutral.Atoms are stable and electrically neutral. Atoms have.
Wednesday, Oct. 2, 2013PHYS , Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #11 Wednesday, Oct. 2, 2013 Dr. Amir Farbin Importance.
Monday, March 16, 2015PHYS , Spring 2014 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #12 Monday, March 16, 2015 Dr. Jaehoon Yu Rutherford.
Atomic Spectra and Electron Orbitals. The Classical Atom Electrons orbited the nucleus. Electrons orbited the nucleus. Problem!! Problem!! Accelerating.
Atomic Structure. Model A: The plum pudding model J.J. Thompson Negative charges like raisins in plumb pudding Positive charge is spread out like the.
Ch2 Bohr’s atomic model Four puzzles –Blackbody radiation –The photoelectric effect –Compton effect –Atomic spectra Balmer formula Bohr’s model Frank-Hertz.
Unit 12: Part 2 Quantum Physics. Overview Quantization: Planck’s Hypothesis Quanta of Light: Photons and the Photoelectric Effect Quantum “Particles”:
QUANTUM AND NUCLEAR PHYSICS. Wave Particle Duality In some situations light exhibits properties that are wave-like or particle like. Light does not show.
1 PHYS 3313 – Section 001 Lecture #9 Wednesday, Sept. 25, 2013 Dr. Jae Yu Compton Effect Pair production/Pair annihilation Atomic Model of Thomson Rutherford.
1© Manhattan Press (H.K.) Ltd Continuous spectra Spectra Sun’s spectrum and Fraunhofer lines.
The Atomic Models of Thomson and Rutherford Rutherford Scattering The Classic Atomic Model The Bohr Model of the Hydrogen Atom Successes & Failures of.
PHYS 3313 – Section 001 Lecture #15
PHYS 3313 – Section 001 Lecture #14
PHYS 3313 – Section 001 Lecture #12
Lecture 12: The Atom & X-Rays
CHAPTER 6 Structure of the Atom
PHYS 3313 – Section 001 Lecture #13
PHYS 3313 – Section 001 Lecture #9
What value of wavelength is associated with the Lyman series for {image} {image} 1. {image}
CHAPTER 4 Structure of the Atom
Chapter 4 The Nuclear Atom.
General Physics (PHY 2140) Lecture 33 Modern Physics Atomic Physics
The Bohr Model of the Atom
CHAPTER 4 Structure of the Atom
PHYS 3313 – Section 001 Lecture #14
Bohr Model Rutherford established the atomic nucleus as a positive charge of radius ~ 1F At the same time, the radius of an atom was known to be ~ 10-10m.
PHYS 3313 – Section 001 Lecture #10
Presentation transcript:

Wednesday, Sept. 26, 2012 PHYS , Fall 2012 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #9 Wednesday, Sept. 26, 2012 Dr. Jaehoon Yu The Bohr Model of the Hydrogen Atom Bohr Radius Fine Structure Constant The Correspondence Principle Characteristic X-ray Spectra Atomic Excitation by Electrons

Wednesday, Sept. 26, 2012 PHYS , Fall 2012 Dr. Jaehoon Yu 2 Announcements Reading assignments: CH4.6 and CH4.7 Mid-term exam –In class on Wednesday, Oct. 10, in PKH107 –Covers: CH1.1 to what we finish Wednesday Oct. 3 –Style: Mixture of multiple choices and free response problems which are more heavily weighted –Mid-term exam constitutes 20% of the total Conference volunteers, please send to Dr. Jackson –Extra credit of 3 points per each hour served, as good as attending the class!! Colloquium today –4pm, SH101 –Dr. Kaushik De on latest LHC results

Special Project #3 A total of Ni Ni incident projectile particles of atomic number Z1 Z1 kinetic energy KE scatter on a target of thickness t, atomic number Z2 Z2 and with n atoms per volume. What is the total number of scattered projectile particles at an angle  ? (20 points) Please be sure to define all the variables used in your derivation! Points will be deducted for missing variable definitions. This derivation must be done on your own. Please do not copy the book or your friends’. Due is Monday, Oct. 8. Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

The Bohr Model of the Hydrogen Atom – The assumptions “Stationary” states or orbits must exist in atoms, i.e., orbiting electrons do not radiate energy in these orbits. These orbits or stationary states are of a fixed definite energy E. The emission or absorption of electromagnetic radiation can occur only in conjunction with a transition between two stationary states. The frequency, f, of this radiation is proportional to the difference in energy of the two stationary states: E = E1 E1 − E2 E2 = hf where h is Planck’s Constant – Bohr thought this has to do with fundamental length of order ~ m Classical laws of physics do not apply to transitions between stationary states. The mean kinetic energy of the electron-nucleus system is quantized as K = nhf orb /2, where f orb is the frequency of rotation. This is equivalent to the angular momentum of a stationary state to be an integral multiple of h/2  Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

How did Bohr Arrived at the angular momentum quantization? The mean kinetic energy of the electron-nucleus system is quantized as K = nhf orb /2, where f orb is the frequency of rotation. This is equivalent to the angular momentum of a stationary state to be an integral multiple of h/2 . Kinetic energy can be written Angular momentum is defined as The relationship between linear and angular quantifies Thus, we can rewrite Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

Bohr’s Quantized Radius of Hydrogen The angular momentum is So the speed of an orbiting e can be written From the Newton’s law for a circular motion So from above two equations, we can get Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

Bohr Radius The radius of the hydrogen atom for stationary states is Where the Bohr radius for a given stationary state is: The smallest diameter of the hydrogen atom is –OMG!! The fundamental length!! n = 1 gives its lowest energy state (called the “ground” state) Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

Emission of light occurs when the atom is in an excited state and decays to a lower energy state (nu (nu → n ℓ ). where f is the frequency of a photon. R∞ R∞ is the Rydberg constant. The Hydrogen Atom The energies of the stationary states where E0 E0 is the ground state energy Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

Transitions in the Hydrogen Atom Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu Lyman series: The atom will remain in the excited state for a short time before emitting a photon and returning to a lower stationary state. All hydrogen atoms exist in n = 1 (invisible). Balmer series: When sunlight passes through the atmosphere, hydrogen atoms in water vapor absorb the wavelengths (visible).

Fine Structure Constant The electron’s speed on an orbit in the Bohr model: On the ground state, v1 v1 = 2.2 × 10 6 m/s ~ less than 1% of the speed of light The ratio of v1 v1 to c is the fine structure constant, .. Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

The Correspondence Principle Need a principle to relate the new modern results with classical ones. Classical electrodynamics Bohr’s atomic model Determine the properties of radiation Bohr’s correspondence principle In the limits where classical and quantum theories should agree, the quantum theory must produce the classical results. + Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

The Correspondence Principle The frequency of the radiation emitted f classical is equal to the orbital frequency f orb of the electron around the nucleus. The frequency of the transition from n + 1 to n is For large n the classical limit, Substitute E0:E0: So the frequency of the radiated E between classical theory and Bohr model agrees in large n case!! Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

Importance of Bohr’s Model Demonstrated the need for Plank’s constant in understanding atomic structure Assumption of quantized angular momentum which led to quantization of other quantities, r, v and E as follows Orbital Radius: Orbital Speed: Energy levels: Wednesday, Sept. 26, 2012 PHYS , Fall 2012 Dr. Jaehoon Yu 13

Successes and Failures of the Bohr Model The electron and hydrogen nucleus actually revolved about their mutual center of mass  reduced mass correction!! All we need is to replace me me with atom’s reduced mass. The Rydberg constant for infinite nuclear mass, R ∞ is replaced by R.R. Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

Limitations of the Bohr Model The Bohr model was a great step of the new quantum theory, but it had its limitations. 1) Works only to single-electron atoms – Even for ions  What would change? – The charge of the nucleus 2) Could not account for the intensities or the fine structure of the spectral lines – Fine structure is caused by the electron spin 3) Could not explain the binding of atoms into molecules Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

Characteristic X-Ray Spectra and Atomic Number Shells have letter names: K shell for n = 1 L shell for n = 2 The atom is most stable in its ground state. When a transition occurs in a heavy atom, the radiation emitted is an x ray. It has the energy E (x ray) = Eu Eu − Eℓ.Eℓ. An electron from higher shells will fill the inner-shell vacancy at lower energy. Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

Atomic Number L shell to K shell Kα Kα x ray M shell to K shell Kβ Kβ x ray Atomic number Z = of protons in the nucleus Moseley found a relationship between the frequencies of the characteristic x ray and Z. This holds for the Kα Kα x ray Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

Moseley’s Empirical Results The x ray is produced from n = 2 to n = 1 transition. In general, the K series of x ray wavelengths are Moseley’s research clarified the importance of the electron shells for all the elements, not just for hydrogen. Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

Atomic Excitation by Electrons Franck and Hertz studied the phenomenon of ionization. Accelerating voltage is below 5 V electrons did not lose energy Accelerating voltage is above 5 V sudden drop in the current Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu

Atomic Excitation by Electrons Ground state has E0 E0 to be zero. First excited state has E1.E1. The energy difference E1 E1 − 0 = E1 E1 is the excitation energy. Above 4.88 eV, the current drops because scattered electrons no longer reach the collector until the accelerating voltage reaches 9.8 eV and so on. Wednesday, Sept. 26, PHYS , Fall 2012 Dr. Jaehoon Yu Hg has an excitation energy of 4.88 eV in the first excited state No energy can be transferred to Hg below 4.88 eV because not enough energy is available to excite an electron to the next energy level