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Transcript
Cambridge University Press
978-0-521-70820-3 - Physics for the IB Diploma, Fifth Edition
K. A. Tsokos
Frontmatter
More information
Physics for the
IB Diploma
Fifth edition
K. A. Tsokos
© in this web service Cambridge University Press
www.cambridge.org
Cambridge University Press
978-0-521-70820-3 - Physics for the IB Diploma, Fifth Edition
K. A. Tsokos
Frontmatter
More information
CAMBRIDGE UNIVERSITY PRESS
Cambridge, New York, Melbourne, Madrid, Cape Town, Singapore,
São Paulo, Delhi, Dubai, Tokyo
Cambridge University Press
The Edinburgh Building, Cambridge CB2 8RU, UK
www.cambridge.org
Information on this title: www.cambridge.org/9780521708203
First, second and third editions © K. A. Tsokos 1998, 1999, 2001
Fourth edition © Cambridge University Press 2005
Fifth edition © Cambridge University Press 2005, 2008
This publication is in copyright. Subject to statutory exception
and to the provisions of relevant collective licensing agreements,
no reproduction of any part may take place without the written
permission of Cambridge University Press.
First published by K. A. Tsokos 1998
Second edition 1999
Third edition 2001
Fourth edition published by Cambridge University Press 2005
Fifth edition 2008
5th printing with corrections 2009
Printed in the United Kingdom by Latimer Trend
A catalogue record for this publication is available from the British Library
ISBN 978-0-521-70820-3 Paperback
Cambridge University Press has no responsibility for the persistence or
accuracy of URLs for external or third-party internet websites referred to in
this publication, and does not guarantee that any content on such websites is,
or will remain, accurate or appropriate. Information regarding prices, travel
timetables and other factual information given in this work are correct at
the time of first printing but Cambridge University Press does not guarantee
the accuracy of such information thereafter.
ACKNOWLEDGEMENTS
We are grateful to the following for permission to reproduce photographs:
76, 526(t), 644 Science Photo Library; 89 Harold Edgerton/Science Photo Library; 255,
Bettmann/CORBIS; 256 Reuters; 276 Sheila Terry/Science Photo Library; 315 Richard Megna/Science
Photo Library; 400 (Francis Simon), 403 (Segre Collection), 526(b), 725 (Physics Today Collection)
American Institute of Physics/Science Photo Library; 464(l) Robert Gendler/Science Photo Library; 464(r)
John Walsh/Science Photo Library; 492, 535c Anglo-Australian Observatory/David Malin Images; 535a, b
NOAO/Science Photo Library; 733 Stanford Linear Accelerator Center/Science Photo Library; 737a CERN
PHOTO/ Frédéric Pitchal/Sygma/CORBIS; 737b David Parker/Science Photo Library; 741 Goronwy Tudor
Jones/University of Birmingham/Science Photo Library; 742 CERN/Science Photo Library; 747 Klaus
Guldbranden/Science Photo Library
© in this web service Cambridge University Press
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Cambridge University Press
978-0-521-70820-3 - Physics for the IB Diploma, Fifth Edition
K. A. Tsokos
Frontmatter
More information
Contents
Preface
A note to the reader
xi
xii
2.2
Motion with constant
acceleration – Core
Acceleration
Measuring speed and acceleration
More on graphs
48
48
54
56
Part I Core and AHL
1
Topic 1: Physics and physical
measurement
2
2.3
2
2
5
The concept of force – Core
Forces and their direction
Hooke’s law
63
64
67
2.4
Newton’s first law – Core
Newton’s first law
Equilibrium
69
69
70
2.5
Newton’s second and
third laws – Core
Newton’s second law
The inclined plane
Newton’s third law
76
77
82
83
1.1
1.2
1.3
1.4
The realm of physics – Core
Orders of magnitude and units
Fundamental interactions
Uncertainties and errors – Core
Errors of measurement
Significant digits
Line of best fit
8
8
11
12
Mathematical and graphical
techniques – Core
Multiplicative changes
Straight-line graphs
Getting a linear graph
Interpreting graphs
Sine curves
Making assumptions
14
14
15
16
17
18
18
Vectors and scalars – Core
Vectors
Multiplication of a vector by a scalar
Addition of vectors
Subtraction of vectors
Components of a vector
21
21
22
22
24
25
2.6
Linear momentum – Core
The concept of momentum
Impulse
The law of conservation of
momentum
Proof of momentum conservation
Two-dimensional collisions
91
93
95
2.7
Work, energy and power – Core
Work done by a force
Gravitational potential energy
The work–kinetic energy relation
Conservation of energy
Frictional forces
Power
Kinetic energy and momentum
The problem of least time
99
99
102
103
104
107
108
110
112
2.8
Circular motion – Core
Circular motion and centripetal
acceleration
Centripetal forces
Angular momentum
119
1.5 Graphical analysis and
uncertainties – Core
Logarithmic functions
Propagation of errors
31
31
33
Topic 2: Mechanics
38
2.1
38
38
42
44
Kinematic concepts – Core
Displacement and velocity
Frames of reference
Graphs for uniform motion
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87
87
89
119
122
123
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K. A. Tsokos
Frontmatter
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iv Contents
2.9
The law of gravitation – Core
Newton’s law of gravitation
Gravitational field strength
127
127
129
2.10 Projectile motion – AHL
Parabolic motion
Launch at an arbitrary angle
Effect of air resistance forces
132
132
134
138
2.11 Motion in a gravitational field – AHL
Gravitational potential energy
Escape velocity
Orbital motion
Equipotential surfaces
The binary star system
142
143
145
146
149
151
4.2
Travelling-wave characteristics – Core
What is a wave?
Transverse and longitudinal waves
Wave pulses
Travelling waves
Wavefronts
216
216
217
218
218
224
4.3
Wave phenomena I: reflection and
refraction – Core
The principle of superposition
Reflection and refraction of waves
Huygens’ principle
228
228
231
234
Wave phenomena II: diffraction and
interference – Core
Diffraction
Interference
238
238
240
4.4
Topic 3: Thermal properties of matter 158
3.1
3.2
3.3
3.4
Thermal concepts – Core
Temperature
Heat as energy
The atomic model of matter
158
158
159
160
Thermal properties – Core
Specific heat capacity
Change of state
Measuring specific heats
Evaporation
The kinetic theory of gases
163
163
165
167
168
169
Ideal gases – AHL
Pressure
The Boyle–Mariotte law
The volume–temperature law
The pressure–temperature law
The equation of state
174
174
175
176
177
178
Thermodynamics – AHL
Internal energy
Work done on or by a gas
The first law of thermodynamics
The second law of thermodynamics
Degradation of energy
183
183
184
187
189
192
Topic 4: Oscillations and waves
195
4.1
195
195
196
204
207
208
Simple harmonic motion – Core
Oscillations
Kinematics of simple harmonic motion
Energy in simple harmonic motion
Damping
Forced oscillations and resonance
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4.5
The Doppler effect – AHL /
SL Option A
The Doppler effect
244
244
4.6
Standing waves – AHL / SL Option A
Standing waves on strings and tubes
Resonance and the speed of sound
251
251
255
4.7
Diffraction – AHL / SL Option A
Diffraction
Single-slit diffraction
259
259
261
4.8
Resolution – AHL / SL Option A
The Rayleigh criterion
267
267
4.9
Polarization – AHL / SL Option A
What is polarization?
Malus’s law
Polarizers and analysers
Polarization by reflection
Optical activity
Practical applications of
polarization
271
271
272
273
274
275
Topic 5: Electricity and magnetism
280
5.1
Electric charge – Core
Properties of electric charge
Coulomb’s law for the electric force
280
280
285
5.2
Electric field and electric
potential – Core
Electric field
Electric potential
The electronvolt
289
289
292
295
276
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K. A. Tsokos
Frontmatter
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Contents v
5.3
5.4
5.5
5.6
5.7
5.8
Electric field and electric
potential – AHL
Electric fields
Electric potential and energy
Equipotential surfaces
The connection between electric
potential and electric field
Similarities between electricity
and gravitation
Electric current and electric
resistance – Core
Electric current
Electric resistance
Electric power
299
299
300
304
Radioactivity – Core
The nature of alpha, beta and
gamma radiations
Radioactive decay equations
The law of radioactive decay
373
373
376
377
6.3
Nuclear reactions – Core
The unified mass unit
The mass defect and binding energy
Nuclear reactions
Nuclear fission
Nuclear fusion
380
380
381
384
385
385
6.4
Interactions of matter with
energy – AHL / SL Option B
The photoelectric effect
De Broglie’s wavelength
389
389
394
Quantum theory and the uncertainty
principle – AHL / SL Option B
Atomic spectra
The ‘electron in a box’ model
The Schrödinger theory
The Heisenberg uncertainty principle
398
398
399
400
402
6.2
306
310
310
312
314
318
318
320
325
Magnetic fields – Core
Magnetic field
The magnetic force on a current
The magnetic force on a
moving charge
Ørsted’s discovery
The force between two
current-carrying wires
336
336
338
Electromagnetic induction – AHL
A wire moving in a magnetic field
Faraday’s law
Lenz’s law
Faraday’s disc
350
350
351
354
356
Alternating current – AHL
The AC generator
Power in AC circuits
The transformer
Transformers and power
transmission
360
360
361
363
327
339
341
6.5
6.6
343
365
Topic 6: Atomic and nuclear physics
367
6.1
367
367
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369
369
370
371
305
Electric circuits – Core
Emf
Simple electric circuits
Ammeters and voltmeters
Sensors based on the potential
divider
The atom and its nucleus – Core
The discovery of the nuclear atom
Consequences of the Rutherford
(Geiger–Marsden) experiment
The Rutherford model of the atom
The Bohr model
Nuclear structure
The forces within the nucleus
368
Nuclear physics – AHL / SL Option B
Scattering experiments and distance
of closest approach
The mass spectrometer
Beta decay and the neutrino
Nuclear energy levels
The radioactive decay law
Topic 7: Energy, power and climate
change
7.1
Energy degradation and power
generation – Core
Degradation of energy
Electricity production
Energy sources
Fossil fuels
Nuclear power
Solar power
Hydroelectric power
Wind power
Wave power
407
407
408
409
410
411
415
415
415
417
417
418
420
423
425
427
428
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vi Contents
7.2
The greenhouse effect and global
warming – Core
The black-body law
Solar radiation
The greenhouse effect
Global warming
Sea level
Effects of global warming on climate
434
434
436
438
444
447
448
8.2
Analogue and digital signals – AHL /
SL Option C / SL and HL Option F
Binary numbers
Analogue and digital signals
Compact disks
Other storage devices
Advantages of digital storage
454
454
455
458
459
461
Digital imaging with charge-coupled
devices – AHL / SL Option C
Capacitance
The charge-coupled device
CCD imaging characteristics
Medical uses of CCDs
463
463
464
466
467
Part II Options
Resolution – SL
481
A6
Polarization – SL
481
SL Option B – Quantum physics
B1
Quantum physics – SL
482
B2
Nuclear physics – SL
482
SL Option C – Digital technology
C1
Topic 8: Digital technology
8.1
A5
471
The content of Options A–D (except
Option A1) is identical to that in the
appropriate chapter in the Core and
AHL material, to which the reader is
referred (details are given in the text).
Analogue and digital
signals – SL
483
Data capture and imaging using
CCDs – SL
483
C3
Electronics – SL
484
C4
The mobile phone system – SL
484
C2
SL Option D – Relativity and particle
physics
D1
Introduction to relativity – SL
485
D2
Concepts and postulates of special
relativity – SL
485
D3
Relativistic kinematics – SL
485
D4
Particles and interactions – SL
486
D5
Quarks – SL
486
SL and HL Option E – Astrophysics
E1
Introduction to the universe – SL
and HL
The solar system
Beyond the solar system
The motion of the stars
487
487
489
491
E2
Stellar radiation – SL and HL
The energy source of stars
Luminosity
Black-body radiation
Stellar spectra
The Hertzsprung–Russell diagram
Types of stars
494
494
495
496
498
499
500
E3
Stellar objects – SL and HL
The parallax method
Absolute and apparent magnitudes
Spectroscopic parallax
The Cepheids
506
506
507
510
511
SL Option A – Sight and wave phenomena
A1
A2
The eye and sight – SL
The structure of the human eye
Depth of vision
Accommodation
Scotopic and photopic vision
Colour
Colour blindness
Colour addition
Colour subtraction
Perception of colour and light
472
472
473
474
474
475
476
476
477
478
The Doppler effect – SL
480
A3 Standing waves – SL
480
A4 Diffraction – SL
480
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Contents vii
E4
E5
E6
Cosmology – SL and HL
Olbers’ paradox
The expanding universe
The Big Bang: the creation of space
and time
The development of the universe
514
514
516
Stellar evolution – Extension HL
Nucleosynthesis
Evolutionary paths and stellar
processes
Pulsars and quasars
521
521
Galaxies – Extension HL
Types of galaxy
Galactic motion
Hubble’s law
The evolution of the
universe
517
517
525
529
F2
F3
Radio communication – SL
and HL
Modulation
Amplitude modulation (AM)
Frequency modulation (FM)
Comparing AM and FM
The AM radio receiver
Analogue and digital signals – SL
and HL
Binary numbers
Analogue and digital signals
Bit rate of a digital signal
The transmission and reception of
digital signals
Time division multiplexing
The advantages of digital
communication
Optic fibre transmission – SL
and HL
Total internal reflection
Optical fibres
Dispersion
Attenuation
Detection
Noise
Regeneration
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F5
533
533
536
537
F6
539
Channels of communication – SL
and HL
Copper wires
Wire pairs
Coaxial cables
Optic fibres
Radio waves
Microwave transmission through
free space
Satellite communications
Electronics – Extension HL
The operational amplifier (op-amp)
The non-inverting amplifier
Reshaping digital pulses – the
Schmitt trigger
The mobile phone
system – Extension HL
574
574
575
575
575
576
577
578
584
584
588
590
596
SL and HL Option G – Electromagnetic
waves
SL and HL Option F – Communications
F1
F4
544
544
546
548
550
550
554
554
554
554
G1
Light – SL and HL
The speed of light
Electromagnetic waves
Properties of EM waves
The laser
598
598
599
601
603
G2
Optical instruments – SL and HL
Lenses
Optical instruments
Lens aberrations
607
607
617
620
G3
Interference and diffraction –
SL and HL
Two-source interference
Young’s two-slit experiment
Intensity in two-slit interference
Multiple-slit diffraction
The diffraction grating
624
624
626
628
629
631
G4
X-rays – Extension HL
The production of X-rays
X-ray diffraction
634
634
635
G5
Thin-film interference – Extension
HL
Parallel films
Thin air wedges
Measuring small distances
640
640
641
642
557
558
558
562
562
564
565
567
569
570
571
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978-0-521-70820-3 - Physics for the IB Diploma, Fifth Edition
K. A. Tsokos
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viii Contents
I3
HL Option H – Special and
general relativity
H1 The principle of special
relativity – HL
Frames of reference
The speed of light
The principle of special relativity
644
645
647
648
H2 The effects of special relativity – HL
Time dilation
Length contraction
Addition of velocities
652
652
657
659
H3 Consequences of and evidence for
special relativity – HL
Relativistic energy
Evidence for special relativity
The Michelson–Morley experiment
The constancy of the speed of
light
H4 Relativistic mechanics – HL
Momentum and energy
(momenergy)
A point about units
A free electron cannot absorb
(or emit) a photon
H5 General relativity – HL
The principle of equivalence
The tests of general relativity
The structure of the theory
Black holes
Time dilation in general
relativity
J1
718
718
719
720
720
721
J2
Detectors and accelerators – HL
The need for high energies
Resolution
Accelerators
Synchrotron radiation
Available energy
Detectors
731
731
732
733
738
738
740
J3
Quarks and leptons – HL
Hadrons – baryons and mesons
Baryon number
Strangeness
The spin of hadrons
Colour
Gluons
Confinement
The interaction between nucleons
Quarks, leptons and the standard
model
Lepton number
The Higgs particle
746
746
748
748
749
749
750
751
752
671
673
674
685
HL Option I – Biomedical physics
I1
The functioning of the ear – HL
The ear
Intensity of sound
Hearing defects
690
690
693
697
I2
Medical imaging – HL
Properties of radiation
X-ray imaging
Other imaging techniques
Ultrasound
Diagnostic uses of radioactive
sources
700
700
702
705
707
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709
712
716
Particles and interactions – HL
Particles and antiparticles
The elementary particles
Quantum numbers
Antiparticles
Spin
The Heisenberg uncertainty
principle for time and energy
Virtual particles
Interactions and exchange particles
Feynman diagrams
The range of an interaction
671
677
677
680
682
683
712
HL Option J – Particle physics
663
663
666
667
669
Radiation in medicine – HL
Biological effects of radiation
and dosimetry
Radiation therapy
J4
Experimental evidence for
the standard model – HL
Gell-Mann’s prediction of the
omega-minus
The direct evidence for quarks
Asymptotic freedom
The discovery of the Z0 and
neutral currents
722
723
723
725
728
752
753
753
758
758
758
761
761
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K. A. Tsokos
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Contents ix
J5
Cosmology and strings – HL
The Boltzmann equation
Matter and antimatter
Strings
Physics and the theory of
knowledge (TOK) – SL and HL
764
764
765
766
770
Appendices
1
Physical constants
2 Masses of elements and
selected isotopes
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3
Astronomical data
780
4 Some important mathematical
results
781
5
782
Nobel prize winners in physics
Answers to questions
788
Glossary of selected terms
819
Index
832
778
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For Alexios and Alkeos
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Preface
Physics is a fundamental science, and those
who study it will gain an understanding of the
basic laws that govern everything from the very
small subatomic to the very large cosmic scale.
The study of physics provides us with an
unparalleled power of analysis that is useful in
the study of the other sciences, engineering and
mathematics, as well as in daily life.
eye and sight, which is not part of the AHL core).
Three options (Option E, Astrophysics; Option F,
Communications; and Option G, Electromagnetic
waves) are available to both SL and HL students.
Finally, there are three options (Option H, Special
and general relativity; Option I, Biomedical
physics; and Option J, Particle physics) that are
available to HL students only.
This fifth edition of Physics for the IB Diploma
follows the previous edition, but contains
material for the new syllabus that will be
examined for the first time in May 2009. It
covers the entire International Baccalaureate
(IB) syllabus, including all options at both
standard level (SL) and higher level (HL). It
includes a chapter on the role of physics in the
theory of knowledge (TOK), along with many
discussion questions for TOK. Each chapter
opens with a list of objectives, which include
the important formulae that will be covered in
that chapter. The questions at the end of each
chapter have been increased, and there are
answers at the end of the book for all those
involving calculation (and for some others too).
The division of this book into chapters and
sections usually follows quite closely the
syllabus published by the International
Baccalaureate Organization (IBO). This does not
mean, however, that this particular order
should be followed in teaching. Within reason,
the sections are fairly independent of each other,
and so alternative teaching sequences may be
used. It must also be stressed that this book is
not an official guide to the IB syllabus, nor is
this book connected with the IBO in any way.
Part I of the book covers the core material and the
additional higher level (AHL) material. The title
and running heads of each chapter clearly
indicate whether the chapter is part of the core or
AHL. Part II covers the optional subjects. There are
now four options that are available to SL students
only (Option A, Sight and wave phenomena;
Option B, Quantum physics; Option C, Digital
technology; and Option D, Relativity and particle
physics). The material for these is the same as the
corresponding AHL material, and so these four
SL options are neither repeated nor presented
separately (except for one chapter, Option A1, The
© in this web service Cambridge University Press
The book contains many example questions and
answers that are meant to make the student
more comfortable with solving problems. Some
are more involved than others. There are also
questions at the end of each chapter, which the
student should attempt to answer to test his or
her understanding. Even though the IB does not
require calculus for physics, I have used
calculus, on occasion, in the text and in the
questions for the benefit of those students
taking both physics and mathematics at higher
level. They can apply what they are learning in
mathematics in a concrete and well-defined
context. However, calculus is not essential for
following the book. It is assumed that a student
starting a physics course at this level knows the
basics of trigonometry and is comfortable with
simple algebraic manipulations.
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K. A. Tsokos
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xii Preface
In many questions and examples I have not
resisted the temptation to use 10 m s-2 as the
numerical value of the acceleration due to
gravity. I have also followed the conventions of
symbols used by the IBO in their Physics Data
Booklet, with one major exception. The Data
Booklet uses the symbol s for displacement.
Almost universally, the symbol s is reserved for
distance, and so s stands for distance in this
book, not displacement. Also, I have chosen to
call initial velocities, speeds, etc. by v0 rather
than the IBO’s u.
I wish to thank my wife, Ellie Tragakes, for her
great help and support. I am indebted to fellow
teacher Wim Reimert for his careful reading of
the book and his extensive comments that have
improved the book – I thank him sincerely. I
would like to thank Geoff Amor, who has edited
the new material for the fifth edition,
implemented my changes, and made many
suggestions for its improvement.
K. A. Tsokos
Athens
May 2007
A note to the reader
The main text of each chapter contains a
number of different features, which are clearly
identified by the use of headings or by other
typographical means, as outlined below.
Important results, laws, definitions and
significant formulae
Particularly important material, such as
important results, laws, definitions and
significant formulae, appear in a shaded box.
Example questions
These occur in nearly all of the chapters. They
are indicated by the heading ‘Example
question(s)’ and all have a full answer. It is a
good idea to attempt to solve these problems
before reading the answers. There are over 500
such example questions in this book.
Material for higher level students
This material is highlighted in a shaded box
that is labelled ‘HL only’.
Material that is outside the IB syllabus
Some material is included that is outside the IB
syllabus and will not be examined in the IB
exams. It is included here for two reasons. The
first is that I believe that it clarifies syllabus
material and in some cases it does so in
essential ways. The second is that it gives the
interested student a more rounded view of the
subject that is not bounded by the rigid
syllabus content. Such material is highlighted
in a shaded box that is labelled ‘Supplementary
material’. There is also a small amount of other
similar material with different labels.
Questions
Learning outcomes/objectives
These are provided as bullet lists at the
beginning of each chapter, and indicate what
you will have learned or be able to do when you
have finished studying the chapter.
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Each chapter ends with a set of numbered
questions. Answers to all those that involve
calculation are given at the end of the book.
Answers are also provided for some other
questions where it is useful for students to be
able to check their answers.
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