λν = c λ ν Electromagnetic spectrum classification of light based on the values of λ and ν

Similar documents
Chemistry 102 Summary June 24 th. Properties of Light

Name Date Class ELECTRONS IN ATOMS. Standard Curriculum Core content Extension topics

Atomic Structure: Chapter Problems

Wave Function, ψ. Chapter 28 Atomic Physics. The Heisenberg Uncertainty Principle. Line Spectrum

TIME OF COMPLETION NAME SOLUTION DEPARTMENT OF NATURAL SCIENCES. PHYS 3650, Exam 2 Section 1 Version 1 October 31, 2005 Total Weight: 100 points

DO PHYSICS ONLINE FROM QUANTA TO QUARKS QUANTUM (WAVE) MECHANICS

Chapter 18: The Structure of the Atom

The Phenomenon of Photoelectric Emission:

Arrangement of Electrons in Atoms

Light as a Wave. The Nature of Light. EM Radiation Spectrum. EM Radiation Spectrum. Electromagnetic Radiation

13- What is the maximum number of electrons that can occupy the subshell 3d? a) 1 b) 3 c) 5 d) 2

Photons. ConcepTest ) red light 2) yellow light 3) green light 4) blue light 5) all have the same energy. Which has more energy, a photon of:

How To Understand Light And Color

Atomic Structure Ron Robertson

5. The Nature of Light. Does Light Travel Infinitely Fast? EMR Travels At Finite Speed. EMR: Electric & Magnetic Waves

PHOTOELECTRIC EFFECT AND DUAL NATURE OF MATTER AND RADIATIONS

AP* Atomic Structure & Periodicity Free Response Questions KEY page 1

Quantum Mechanics and Atomic Structure 1

WAVES AND ELECTROMAGNETIC RADIATION

Chemistry 2 Chapter 13: Electrons in Atoms Please do not write on the test Use an answer sheet! 1 point/problem 45 points total

Review of the isotope effect in the hydrogen spectrum

ATOMIC SPECTRA. Apparatus: Optical spectrometer, spectral tubes, power supply, incandescent lamp, bottles of dyed water, elevating jack or block.

Nanoelectronics. Chapter 2 Classical Particles, Classical Waves, and Quantum Particles. Q.Li@Physics.WHU@2015.3

Chem 1A Exam 2 Review Problems

CHAPTER - 1. Chapter ONE: WAVES CHAPTER - 2. Chapter TWO: RAY OPTICS AND OPTICAL INSTRUMENTS. CHAPTER - 3 Chapter THREE: WAVE OPTICS PERIODS PERIODS

CHEM 1411 Chapter 5 Homework Answers

Atoms Absorb & Emit Light

Unit 2: Chemical Bonding and Organic Chemistry

Electron Orbits. Binding Energy. centrifugal force: electrostatic force: stability criterion: kinetic energy of the electron on its orbit:

Experiment #5: Qualitative Absorption Spectroscopy

CHEMSITRY NOTES Chapter 13. Electrons in Atoms

Level 3 Achievement Scale

Sample Exercise 6.1 Concepts of Wavelength and Frequency

Does Quantum Mechanics Make Sense? Size

Experiment #12: The Bohr Atom. Equipment: Spectroscope Hydrogen and Helium Gas Discharge Tubes, Holder, and Variac Flashlight

Chapter 2. Quantum Theory

Electron Arrangements

The quantum understanding of pre-university physics students

Chapter 7. Electron Structure of the Atom. Chapter 7 Topics

Chapters Magnetic Force. for a moving charge. F=BQvsinΘ. F=BIlsinΘ. for a current

Homework #10 (749508)

Atomic Calculations. 2.1 Composition of the Atom. number of protons + number of neutrons = mass number

Electromagnetic Radiation

From lowest energy to highest energy, which of the following correctly orders the different categories of electromagnetic radiation?

Chapter 9: ELECTRONS IN ATOMS AND THE PERIODIC TABLE

Flame Tests & Electron Configuration

Multi-electron atoms

Boardworks AS Physics

CHAPTER 11: MODERN ATOMIC THEORY

Calculating particle properties of a wave

Bohr model of hydrogen

THE CURRENT-VOLTAGE CHARACTERISTICS OF AN LED AND A MEASUREMENT OF PLANCK S CONSTANT Physics 258/259

Physics 30 Worksheet # 14: Michelson Experiment

Department of Physics and Geology The Elements and the Periodic Table

Quantum Phenomena and the Theory of Quantum Mechanics

Bohr's Theory of the Hydrogen Atom

2. Molecular stucture/basic

D.S. Boyd School of Earth Sciences and Geography, Kingston University, U.K.

Waves - Transverse and Longitudinal Waves

Molecular Spectroscopy:

G482 Electrons, Waves and Photons; Revision Notes Module 1: Electric Current

The Advanced Placement Examination in Chemistry. Part I Multiple Choice Questions Part II Free Response Questions Selected Questions from1970 to 2010

PHYSICS PAPER 1 (THEORY)

Preview of Period 3: Electromagnetic Waves Radiant Energy II

Curriculum for Excellence. Higher Physics. Success Guide

Solar Energy. Outline. Solar radiation. What is light?-- Electromagnetic Radiation. Light - Electromagnetic wave spectrum. Electromagnetic Radiation

3) Of the following, radiation has the shortest wavelength. A) X-ray B) radio C) microwave D) ultraviolet E) infrared Answer: A

Assessment Plan for Learning Outcomes for BA/BS in Physics

Physical Science Study Guide Unit 7 Wave properties and behaviors, electromagnetic spectrum, Doppler Effect

Elements in the periodic table are indicated by SYMBOLS. To the left of the symbol we find the atomic mass (A) at the upper corner, and the atomic num

Electrons In Atoms Mr. O Brien (SFHS) Chapter 5 Standard 1D

MASS DEFECT AND BINDING ENERGY

Question: Do all electrons in the same level have the same energy?

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

A-level PHYSICS (7408/1)

GRID AND PRISM SPECTROMETERS

Physics 9e/Cutnell. correlated to the. College Board AP Physics 1 Course Objectives

Energy. Mechanical Energy

Physics 111 Homework Solutions Week #9 - Tuesday

Electrons in Atoms & Periodic Table Chapter 13 & 14 Assignment & Problem Set

Blackbody Radiation References INTRODUCTION

Blackbody radiation derivation of Planck s radiation low

Use the following image to answer the next question. 1. Which of the following rows identifies the electrical charge on A and B shown above?

Chapter 28 Atomic Physics

Austin Peay State University Department of Chemistry Chem The Use of the Spectrophotometer and Beer's Law

Code number given on the right hand side of the question paper should be written on the title page of the answerbook by the candidate.

The rate of change of velocity with respect to time. The average rate of change of distance/displacement with respect to time.

MODERN ATOMIC THEORY AND THE PERIODIC TABLE

Determination of Molecular Structure by MOLECULAR SPECTROSCOPY

Arrangement of Electrons in Atoms

Basic Nuclear Concepts

THE BOHR QUANTUM MODEL

Unit 1, Lesson 03: Answers to Homework 1, 0, +1 2, 1, 0, +1, +2 1, 0, +1 2, 1, 0, +1, +2 3, 2, 1, 0, +1, +2, +3. n = 3 l = 2 m l = -2 m s = -½

Infrared Spectroscopy: Theory

Unamended Quantum Mechanics Rigorously Implies Awareness Is Not Based in the Physical Brain

The Hydrogen Atom Is a Magnet.

Treasure Hunt. Lecture 2 How does Light Interact with the Environment? EMR Principles and Properties. EMR and Remote Sensing

Section 11.3 Atomic Orbitals Objectives

Objectives. PAM1014 Introduction to Radiation Physics. Constituents of Atoms. Atoms. Atoms. Atoms. Basic Atomic Theory

FLAP P11.2 The quantum harmonic oscillator

Transcription:

Quantum Theory and Atomic Structure Nuclear atom small, heavy, positive nucleus surrounded by a negative electron cloud Electronic structure arrangement of the electrons around the nucleus Classical mechanics fails in describing the electronic motion Quantum mechanics designed to describe the motion of microscopic particles 7.1 The Nature of Light Light is electromagnetic radiation a stream of energy in the form waves Electromagnetic waves periodic oscillations (cycles) of the electric and magnetic fields in space Wavelength (λ) distance between two adjacent minima or maxima of the wave Frequency (ν) number of oscillations of the electric (or magnetic) field per second units - hertz (Hz) 1 Hz = 1 s -1 Amplitude strength of the oscillation (related to the intensity of the radiation) Speed of light (c) rate of travel of all types of electromagnetic radiation (3. 1 8 m/s) λν = c λ ν Electromagnetic spectrum classification of light based on the values of λ and ν Example: What is the wavelength of light with frequency 98.9 MHz. 98.9 MHz = 98.9 1 6 Hz = 98.9 1 6 s -1 8 c 3. 1 m/s λ = = = 3.3 m ν 6-1 98.9 1 s

Differences between waves and particles Refraction, diffraction and interference of waves The particle nature of light Blackbody radiation light emitted from solid objects heated to incandescence The energy profile of the emitted light could not be explained by the classical mechanics which assumes that the energy of an object can be continuously changed Plank (19) explained the energy profiles by assuming that the energy of an object can be changed only in discrete amounts (quanta) quantization of energy E = n(hν) h Planck s constant h = 6.626 1-34 J s ν frequency of the emitted light n quantum number (positive integer 1, 2, 3, ) hν the energy of one quantum Photoelectric effect ejection of e - from metals by irradiation with light Ejection of e - begins only above a certain threshold frequency (below this frequency, no ejection occurs no mater how intense the light is) Ejection of e - begins with no time delay Can t be explained by treating light as waves Explanation (Einstein, 195) the ejection of e - is caused by particles (photons) with energy proportional to the frequency of the radiation Only photons with enough energy and therefore high enough frequency can eject electrons Ejection results from an encounter of an e - with a single photon (not several photons), so no time delay is observed Energy of the photon (E ph ): E ph = hν ν = c/λ E ph = hc/λ The photon is the electromagnetic quantum the smallest amount of energy atoms can emit or absorb Dual nature of light light has both wave and particle like properties wave (refraction, interference, diffraction) particle (photoelectric effect) Example: Calculate the energy of a photon of light with wavelength 514 nm. 8 c 34 3. 1 m/s 19 Eph = h = 6.626 1 J s = 3.87 1 J λ -9 514 1 m 7.2 Atomic Spectra Spectroscopy studies the interaction of light with matter (emission, absorption, scattering, ) Spectrometer instrument that separates the different colors of light and records their intensities Spectrum intensity of light as a function of its color (wavelength or frequency) Atomic emission spectrum the spectrum emitted by the atoms of an element when they are excited by heating to high temperatures (very characteristic for each element; used for identification of elements)

Spectral lines images of the spectrometer entrance slit produced by the different colors in the spectrum Atomic emission spectra are line spectra consist of discrete frequencies (lines) Can t be explained by classical physics The Rydberg equation fits the observed lines in the hydrogen atomic emission spectrum 1 1 1 = R λ n 2 2 1 n 2 n 1, n 2 positive integers (1, 2, 3,...) and n 1 < n 2 R the Rydberg constant (1.96776 1 7 m -1 ) Lyman series (UV) n 1 = 1 and n 2 = 2, 3, 4,... Balmer series (VIS) n 1 = 2 and n 2 = 3, 4, 5, Paschen series (IR) n 1 = 3 and n 2 = 4, 5, 6,... The Bohr model of the H atom (1913) Explains the hydrogen atomic emission spectrum by using the idea of quantization Postulates: The electron travels around the nucleus in circular orbits without loss of energy The angular momentum of the electron is quantized only certain orbits are allowed Consequences: The energy of the H atom is quantized only certain discrete energy levels (stationary states) are allowed Each circular orbit corresponds to one E-level Consequences (cont.): A transition between two energy states generates a photon with energy equal to the difference between the two levels ( E) E ph = E state 2 E state 1 = hν E = hν A photon with a specific (discrete) frequency is emitted for each transition from a higher to a lower E-level Atomic emission spectra consist of discrete lines Each orbit is labeled with a number, n, starting from the orbit closest to the nucleus (n = 1, 2, ) The same number is used to label the energy levels n is the quantum number

Energy states of the H atom 2 Z En = B 2 n= 1, 2, 3,..., n B is a constant (B = 2.18 1-18 J) Z is the nuclear charge (For H: Z = 1 E n = -B/n 2 ) Ground state the lowest energy state (n = 1) E 1 = -B/1 2 = -B = 2.18 1-18 J Excited states higher energy levels (n > 1) The energy increases with increasing n The highest possible energy is for n = (the electron is completely separated from the nucleus) E = -B/ 2 = A transition between two E-levels with quantum numbers n 1 and n 2 will produce a photon with energy equal to the E-difference between the levels, E: B B 1 1 E= En E 2 n = 1 2 2 = B 2 2 n2 n1 n1 n2 hc 1 1 E= Eph = hν = = B n 2 2 λ 1 n 2 1 B 1 1 B = Rydberg eq. 2 2 = R λ hc n1 n 2 hc Ionization energy (I) of the H atom the energy needed to completely remove the electron from a H atom in its ground state (can be viewed as the energy change from E 1 to E ) B B E = E E1 = ( B) B 2 2 1 = = 18 I = B= 2.18 1 J/atom Limitations of the Bohr Model Applicable only to H-like atoms and ions (having a single electron) in the absence of strong electric or magnetic fields (H, He +, Li 2+, ) 7.3 The Wave-Particle Duality of Matter and Energy Mass-energy equivalency (Einstein) E = mc 2 For a photon with energy E = hν = hc/λ: E = mc 2 = hc/λ mc = h/λ λ = h/mc λ = h/p p photon momentum The equation shows that the wave-like photons have particle-like mass and momentum Experimental evidence (Compton, 1923) De Broglie s hypothesis (1924) all matter has wave-like properties (just as waves have particle-like properties) For a particle with mass, m, and velocity, u, the wavelength is: λ = h/mu De Broglie s equation is equivalent to that for a photon (λ = h/mc) De Broglie s equation combines particle properties (m, u) with wave properties (λ) Matter and energy exhibit wave-particle duality Example: Calculate the wavelengths of an electron (m = 9.19 1-31 kg) with velocity 2.2 1 6 m/s and a bullet (m = 5. g) traveling at 7. m/s. 34 h 6.626 1 J s λ( e ) = = -31 6 mu 9.19 1 kg 2.2 1 m/s 1 = 3.3 1 m =.33 nm comparable to atomic sizes 34 h 6.626 1 J s λ( bul) = = -3 mu 5. 1 kg 7. m/s 34 = 1.9 1 m very short, undetectable

Experimental evidence (Davisson and Germer, 1927) Diffraction of electrons by crystal surfaces Diffraction patterns are consistent with the wavelength predicted by de Broglie s relation The electron can be treated as a wave with a very short wavelength (similar to the wavelength of x-rays) The electron confined in the H atom can be treated as a standing wave having discrete frequencies (energies) like a guitar string Heisenberg s uncertainty principle (1927) the exact position and momentum (velocity) of a particle can not be known simultaneously x p h/4π x and p= m u uncertainty in position and momentum, respectively A consequence of the wave-particle duality of matter The exact location of very small particles is not well known due to their wave-like properties The probability to find a particle at a particular location depends on the amplitude (intensity) of the wave at this location 7.4 The Quantum-Mechanical Model of the Atom Bohr s model of the H atom Assumes the quantization without explanation Does not take into account Heisenberg s uncertainty principle Limited success only for the H atom Schrödinger s model Based on the wave-particle duality of the electron The quantization is logically derived from the wave properties of the electron Formalism applicable to other atoms Atomic Orbitals The Schrödinger equation The electron wave is described by a wavefunction (Ψ) a mathematical function of the wave s amplitude at different points (x, y, z) in space The equation provides solutions for the possible wavefunctions and energies of the electron Only certain solutions for the energy are allowed (waves fit in the atom only for certain energy values) 2 2 2 h Ψ Ψ Ψ + + V E 2 2 2 + Ψ = Ψ 2 m x y z The solutions for the wavefunction, Ψ, in the H atom are called atomic orbitals Born s interpretation of the wavefunction the probability to find the electron at a certain point (x, y, z) in space is proportional to the square of the wave function, Ψ 2, in this point Electron density diagrams three-dimensional plots of the probability to find the electron (Ψ 2 ) around the nucleus electron clouds Contour diagrams surround the densest regions of the electron cloud usually 9% of the total probability 9% probability contour

Probability plot (ground state of H) Radial distribution plot (probability to find the electron in a given spherical layer) 9% probability contour Quantum Numbers Solutions of the Schrödinger equation for the wavefunction of the electron in the H atom: Atomic orbitals Ψn,l,m l Depend on three quantum numbers used as labels of each solution (n, l, m l ) Principal quantum number (n) specifies the energy (E n ) of the electron occupying the orbital and the average distance (r) of the electron from the nucleus (size of the orbital) n E n n r Angular momentum quantum number (l) specifies the shape of the orbital Magnetic quantum number (m l ) specifies the orientation of the orbital A set of three quantum numbers (n, l, m l ) unambiguously specifies an orbital (Ψn,l,m l ) Possible values of the quantum numbers: n = 1, 2, 3,, l =, 1, 2,, n-1 (restricted by n) m l = -l,, -1,, 1,, l (restricted by l) Ψ 3,2,-1 (possible) Ψ 2,2,2 and Ψ 3,,1 (impossible) All orbitals with the same value of n form a principal level (shell) All orbitals with the same value of l form a sublevel (subshell) within a principal shell Subshells are labeled with the value of n followed by a letter corresponding to the value of l l= s, l=1 p, l=2 d, l=3 f, l=4 g, Each value of m l specifies an orbital in a subshell Example: Label the subshell containing the orbital Ψ 3,2,-1 n = 3 l=2 d 3d-subshell Shells n=3 n=2 n=1 n Subshells l=2 l=1 l= l=1 l= l= Orbitals # of orbitals in a shell = n 2 # of orbitals in a subshell = 2l + 1 l -2-1 -1-1 +1 +1 m l +1 +2 3d-subshell 3p-subshell 3s-subshell 2p-subshell 2s-subshell 1s-subshell Example: What is the # of orbitals in the 4f subshell? Give the m l values of these orbitals. 4f n = 4, l = 3 2l + 1 = 7 orbitals l = 3 m l = -3, -2, -1,, +1, +2, +3 Solutions of the Schrödinger equation for the energy of the electron in the H atom: B En = n= 1, 2, 3,... 2 n The energy levels of H depend only on the principal quantum number, n Same as Bohr s energy levels (B = 2.18 1-18 J) E n increases with increasing n

Shapes of Orbitals s-orbitals l = Spherical shape The electron density is highest at the nucleus (density decreases away from the nucleus) The radial distribution has a maximum slightly away from the nucleus The orbital size increases with increasing the energy of the orbital (1s < 2s < 3s ) Higher energy orbitals have several maxima in the radial distribution and one or more spherical nodes (regions with zero probability to find the electron) 2s 2 max, 1 node; 3s 3 max, 2 nodes p-orbitals l = 1 Dumbbell-shaped (two-lobed) Positive sign of Ψ in one of the lobes of the orbital and negative in the other lobe Nodal plane going through the nucleus (surface with zero probability to find the electron) Three possible orientations in space: m l = -1,, +1 p x, p y, p z p-orbitals are possible only in the 2 nd and higher principal shells The orbital size increases with increasing the energy of the orbital (2p < 3p < 4p ) d-orbitals l = 2 Cloverleaf-shaped (four-lobed, except d z 2) Opposite signs of Ψ in the lobes laying beside each other Two perpendicular nodal planes going through the nucleus Five possible orientations in space: m l = -2, -1,, 1, 2 d z 2, d x 2 -y 2, d xy, d zx, d yz d-orbitals are possible only in the 3 rd and higher principal shells The orbital size increases with increasing the energy of the orbital (3d < 4d < 5d )

Energy levels of the H atom Electronic energy depends only on the principal quantum number (n) all subshells in a given shell have the same energy