Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE...

48
Chapter 42 Part III: Modern Physics Dr. Saif M. H. Qaid Atomic Physics 1 Dr. Saif Qaid PHYS 111 - KSU

Transcript of Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE...

Page 1: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Chapter 42

Part III: Modern Physics

Dr. Saif M. H. Qaid

Atomic Physics

1 Dr. Saif QaidPHYS 111 - KSU

Page 2: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

LECTURE OUTLINE

• 42.1 Atomic Spectra of Gases

• 42.2 Early Models of the Atom

• 42.3 Bohr’s Model of the Hydrogen Atom

• 42.8 More on Atomic Spectra: Visible and X-Ray

• 42.9 Spontaneous and Stimulated Transitions

• 42.10 Lasers

2 Dr. Saif QaidPHYS 111 - KSU

Page 3: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Need for Quantum Physics

•Problems remained from classical mechanics that the special theory of relativity didn’t explain.

•Attempts to apply the laws of classical physics to explain the behavior of matter on the atomic scale were consistently unsuccessful.

•Problems included:

– Blackbody radiation

• The electromagnetic radiation emitted by a heated object

– Photoelectric effect

• Emission of electrons by an illuminated metal

Introduction

Page 4: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Hydrogen

Atomic Spectra

Nitrogen

Page 5: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Fig 42-1, p.1353

Page 6: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Balmer’s Realization

Page 7: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s
Page 8: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Fig 42-4, p.1355

J.J. Thompson Model

Page 9: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Fig 42-5a, p.1355

Page 10: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

2sin 4

Rutherford Scattering of -particles

Page 11: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s
Page 12: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s
Page 13: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Fig 42-5b, p.1355

Page 14: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Fig 42-6, p.1356

Page 15: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Fig 42-7, p.1356

Page 16: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Fig 42-8, p.1358

Page 17: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Connection between Bohr and de Broglie

Page 18: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Fig 42-10, p.1362

Express S. E. in spherical coordinates,

solutions separate into two parts, radial

Part and an angular part

Page 19: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Fig 42-12a, p.1365

Radial solution for H

in its ground state.

<r> = a0

Page 20: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Probability per unit volume for finding the electron in the n = 1,

2 and 3 states of the hydrogen atom.

Electron Probability Density for H

0/

3

0

1

1 ar

s ea

02/

3

0

02

24

2 ar

s ea

ar

03/

3

0

2

0

2

03

381

21827 ar

s ea

arar

Page 21: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

The Quantum Theory of Lightالنظرية الكمية للضوء

األطياف الخطيةLine spectra

وجد العلماء أن لكل عنصر طيف خطي مميز له واستطاعوا قياس أطوالها الموجية

. ولكنهم لم يعرفوا في ذلك الوقت سبب وجودها

حزوز فعند مرور تيار كهربائي على غاز فإنه ينبعث ضوء، إذا مر خالل موشور أو م

.حيود تتكون منه خطوط طيفية منفصلة لكل منها طول موجي محدد

ألجل غاز الهيدروجين•

(:طيف مرئي)متسلسلة پالمر

ثابت رايدبرج

,.....5,4,3),1

2

1(R

122

nnn

17101.09737R, m

Page 22: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

The Quantum Theory of Lightالنظرية الكمية للضوء

:أما متسلسالت األطياف غير المرئية فهي

متسلسلة ليمان:

باشنمتسلسلة:

براكيتمتسلسلة:

,.....5,4,3,2),1

1

1(R

122

nnn

.....6,5,4),1

3

1(R

122

nnn

.....7,6,5),1

4

1(R

122

nnn

Page 23: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

The Quantum Theory of Lightالنظرية الكمية للضوء

أطياف األشعة السينيةX-ray spectra

عندماتنبعثمجهولةطبيعةذاتالموادتخترققويةإشعاعاتأنرونتجنالعالموجد

بيعتهابطمعرفتهولعدمثقيلة،معدنيةمادةمنهدفعلىسريعةإلكتروناتتصطدم

.x-rayأسماءهاانبعاثهاوسبب

موجاتهاأطوالكهرومغناطيسيةموجاتبأنهااألشعةهذهطبيعةذلكبعدوعرفت

0.01حدودفيجداقصيرة nm10و nm.

Page 24: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

The Quantum Theory of Lightالنظرية الكمية للضوء

لالشكفيكماخطيوطيفمستمرطيفمنالناتجةاإلشعاعاتهذهطيفيتكون

.المجاور

Page 25: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

The Quantum Theory of Lightالنظرية الكمية للضوء

السينيةاألشعةإنتاج

Page 26: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

The Quantum Theory of Lightالنظرية الكمية للضوء

:الطاقة الحركية لإللكترون المعجل

تعمل الطول الموجي لبداية الطيف المستمر وهو يعتمد فقط على الجهد المسλoحيث

.لتعجيل االلكترون

meterVeV

hchchfeV

eVK

6

0

0

0

1024.1

(:الطول الموجي للفوتون المنبعث11

(RZ1

22

2

if nn

kk

K

K

)13(

)12(

Page 27: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

The Quantum Theory of Lightالنظرية الكمية للضوء

لذرة عديدة اإللكترونات يمكن Kαلقد وجد تجريبيا أن طول موجة الخط المميز

:معرفته من العالقة

.المستعمل كهدفالفعال للعنصر العدد الذري Zeffحيث

يجد إلكترونا سالبا واحدا في نفس (K)حيث أن اإللكترون العائد إلى المستوى األول

وشحنة االلكترون Zeالمستوى فتكون الشحنة الكلية هي مجموع شحنة النواة الموجبة

:وبالتالي الشحنة الكلية. e-السالب

1Z,

Z4

3)

2

1

1

1(RZ

1

eff

2

eff22

2

eff

Z

R

eZeZe )1(

Page 28: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Transition Probabilities of Atoms and Molecules

Page 29: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Stimulated Emission and Lasers

Laser:

•An acronym for “light amplification by the stimulated emission of radiation”

Masers:

•Microwaves are used instead of visible light.

•The first working laser by Theodore H. Maiman in 1960

helium-neon laser

Page 30: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Absorption and Spontaneous Emission

Consider a two-level system

En, Nn

Em, Nm

absorption

En, Nn

Em, Nm

emission

Light from bulbs are due to spontaneous emission

Page 31: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Absorption and Stimulated Emission

En, Nn

Em, Nm

absorption

stimulated emission

En, Nn

Em, Nm

Laser light results from stimulated emission

Page 32: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Stimulated vs Spontaneous Emission

Stimulated emission requires the presence of a photon. An “incoming” photon

stimulates a molecule in an excited state to decay to the ground state by emitting a

photon. The stimulated photons travel in the same direction as the incoming photon.

Spontaneous emission does not require the presence of a photon.

Instead a molecule in the excited state can relax to the ground state by spontaneously

emitting a photon. Spontaneously emitted photons are emitted in all directions.

Page 33: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

When light travels through an absorbing medium, the medium absorbs the light; the

amount of light absorbed is determined by Beer’s Law.

For a medium to operate as a lasing medium, the transmitted light intensity should be

greater than the intensity of light incident on the material.

Page 34: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

When an atom or molecule in the lasing medium absorbs light it is excited

The excited molecule then decays to a lower level either through emission of a photon

(stimulated or spontaneous) or via a non-radiative loss of the energy.

For lasing action, stimulated emission must dominate.

As determined by the Boltzmann factor, the population of the ground state > population

of excited state.

Hence, typically absorption dominates.

Page 35: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

For stimualted emission to be the dominant process, the excited state population must

be larger than the lower state population.

In other words, for a medium to produce laser light, there must be a “population

inversion” where Nupper > Nlower

How can a population inversion be created when the population in the ground state is

always greater that the population in the excited state?

What kinds of materials will “allow” for an inversion of population in its electronic

states?

Page 36: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

How can a population inversion be created?

By excitation of the lasing atoms or molecules - this is called PUMPING.

If the pump source is very intense, the number of atoms or molecules excited can

be large.

However, once excited, the atoms and molecules must say in the excited state long

enough to create an excited population > ground state population

Page 37: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Two-Level System

En, Nn

Em, Nm

En, Nn

Em, Nm

Even with very a intense pump source, the best one can achieve with a two-level

system is

excited state population = ground state population

Page 38: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Three-Level System

The first laser, the ruby laser, was a three-level system

lower lasing state

upper lasing

state

Laser light due to transition from 2E state to 4A2 state

Page 39: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Four-Level System

He-Ne laser

Page 40: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Four-Level System

Nd:YAG laser

upper laser state

lower laser state

Laser light due to transition from 4F to 4I

Page 41: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Dye Lasers: Four-level systems

Page 42: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Dye Tuning Curves

Page 43: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

effic

ient

pum

pin

g

slo

w r

ela

xation Metastable state

fast

slow Population

inversion

Fast relaxation

Requirements for Laser Action

Page 44: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Light Amplification

Create a laser cavity, which consists of the lasing medium and two highly reflective

mirrors.

Page 45: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Continuous vs Pulsed Lasers

Excitation of the lasing atoms or molecules is by using external sources of light,

examples flashlamps or another laser - PUMPING

The output of the laser light can be a continuous wave (cw) if the pumping is

continuous or pulsed if the pumping is pulsed.

Pulsed lasers have very high intensities because the laser intensity is concentrated in

a very short time duration.

Page 46: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Lasers in Chemistry

Lasers being monochromatic, with short pulse durations, and high intensity allow

detailed studies in chemical dynamics.

Can do very fast kinetic studies – femtosec (10-15 s) studies – “look” at bond

dissociation, bond formation, study kinetics in the liquid phase

Spectroscopy – monochromaticity allows detailed information on small molecules

High intensity – allows investigation of processes which which depend on light

intensity and have very small probabilities of occuring e.g. Raman scattering

Page 47: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

Thank You

47 Dr. Saif QaidPHYS 111 - KSU

Page 48: Chapter 42fac.ksu.edu.sa/sites/default/files/phys_111-_lec-3233_-atomic_physics.pdfLECTURE OUTLINE • 42.1 Atomic Spectra of Gases • 42.2 Early Models of the Atom • 42.3 Bohr’s

48 Dr. Saif QaidPHYS 111 - KSU