Physics
1st Edition
Walker
ISBN: 9780133256925
Textbook solutions
Chapter 1: Introduction to Physics
Section 1.1: Physics and the Scientific Method
Section 1.2: Physics and Society
Section 1.3: Units and Dimensions
Section 1.4: Basic Math for Physics
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Chapter 2: Introduction to Motion
Section 2.1: Describing Motion
Section 2.2: Speed and Velocity
Section 2.3: Position-Time Graphs
Section 2.4: Equation of Motion
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Chapter 3: Acceleration and Acceleration Motion
Section 3.1: Acceleration
Section 3.2: Motion with Constant Acceleration
Section 3.3: Position-Time Graphs for Constant Acceleration
Section 3.4: Free Fall
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Chapter 4: Motion in Two Dimensions
Section 4.1: Vectors in Physics
Section 4.2: Adding and Subtracting Vectors
Section 4.3: Relative Motion
Section 4.4: Projectile Motion
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Chapter 5: Newton’s Laws of Motion
Section 5.1: Newton’s Laws of Motion
Section 5.2: Applying Newton’s Laws
Section 5.3: Friction
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Chapter 6: Work and Energy
Section 6.1: Work
Section 6.2: Work and Energy
Section 6.3: Conservation of Energy
Section 6.4: Power
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Chapter 7: Linear Momentum and Collisions
Section 7.1: Momentum
Section 7.2: Impulse
Section 7.3: Conservation of Momentum
Section 7.4: Collisions
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Chapter 8: Rotational Motion and Equilibrium
Section 8.1: Describing Angular Motion
Section 8.2: Rolling Motion and the Moment of Inertia
Section 8.3: Torque
Section 8.4: Static Equilibrium
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Chapter 9: Gravity and Circular Motion
Section 9.1: Newton’s Law of Universal Gravity
Section 9.2: Applications of Gravity
Section 9.3: Circular Motion
Section 9.4: Planetary Motion and Orbits
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Chapter 10: Temperature and Heat
Section 10.1: Temperature, Energy, and Heat
Section 10.2: Thermal Expansion and Energy Transfer
Section 10.3: Heat Capacity
Section 10.4: Phase Changes and Latent Heat
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Chapter 11: Thermodynamics
Section 11.1: The First Law of Thermodynamics
Section 11.2: Thermal Processes
Section 11.3: The Second and Third Laws of Thermodynamics
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Chapter 12: Gases, Liquids, and Solids
Section 12.1: Gases
Section 12.2: Fluids at Rest
Section 12.3: Fluids in Motion
Section 12.4: Solids
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Chapter 13: Oscillations and Waves
Section 13.1: Oscillations and Periodic Motion
Section 13.2: The Pendulum
Section 13.3: Waves and Wave Properties
Section 13.4: Interacting Waves
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Chapter 14: Sound
Section 14.1: Sound Waves and Beats
Section 14.2: Standing Sound Waves
Section 14.3: The Doppler Effect
Section 14.4: Human Perception of Sound
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Chapter 15: The Properties of Lights
Section 15.1: The Nature of Light
Section 15.2: Color and the Electromagnetic Spectrum
Section 15.3: Polarization and Scattering of Light
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Chapter 16: Reflection and Mirrors
Section 16.1: The Reflection of Light
Section 16.2: Plane Mirrors
Section 16.3: Curved Mirrors
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Chapter 17: Refraction and Lenses
Section 17.1: Refraction
Section 17.2: Applications of Refraction
Section 17.3: Lenses
Section 17.4: Applications of Lenses
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Chapter 18: Interference and Diffraction
Section 18.1: Interference
Section 18.2: Interference in Thin Films
Section 18.3: Diffraction
Section 18.4: Diffraction Gratings
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Chapter 19: Electric Charges and Forces
Section 19.1: Electric Charge
Section 19.2: Electric Force
Section 19.3: Combining Electric Forces
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Chapter 20: Electric Fields and Electric Energy
Section 20.1: The Electric Field
Section 20.2: Electric Potential Energy and Electric Potential
Section 20.3: Capacitance and Energy Storage
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Chapter 21: Electric Current and Electric Circuits
Section 21.1: Electric Current, Resistance, and Semiconductors
Section 21.2: Electric Circuits
Section 21.3: Power and Energy in Electric Circuits
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Chapter 22: Magnetism and Magnetic Fields
Section 22.1: Magnets and Magnetic Fields
Section 22.2: Magnetism and Electric Currents
Section 22.3: The Magnetic Force
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Chapter 23: Electromagnetic Induction
Section 23.1: Electricity from Magnetism
Section 23.2: Electric Generators and Motors
Section 23.3: AC Circuits and Transformers
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Chapter 24: Quantum Physics
Section 24.1: Quantized Energy and Photons
Section 24.2: Wave-Particle Duality
Section 24.3: The Heisenberg Uncertainty Principle
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Chapter 25: Atomic Physics
Section 25.1: Early Models of the Atom
Section 25.2: Bohr’s Model of the Hydrogen Atom
Section 25.3: The Quantum Physics of Atoms
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Chapter 26: Nuclear Physics
Section 26.1: The Nucleus
Section 26.2: Radioactivity
Section 26.3: Applications of Nuclear Physics
Section 26.4: Fundamental Forces and Elementary Particles
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Chapter 27: Relativity
Section 27.1: The Postulates of Relativity
Section 27.2: The Relativity of Time and Length
Section 27.3: E=mc^2
Section 27.4: General Relativity
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Chapter Appendix B: Appendix B
Section 1: Chapter 1
Section 10: Chapter 10
Section 11: Chapter 11
All Solutions
Section 25.1: Early Models of the Atom
Exercise 1
Step 1
1 of 2
It is similar to the solar system because it predicts that the electrons orbit the nucleus just as the planets orbit the Sun.
Result
2 of 2
Click here for the solution.
Exercise 2
Step 1
1 of 2
Sunlight is visible part of electromagnetic radiation the sun emits that comes to Earth. Sun radiates as a black body, thus giving off a continuous range of frequencies resulting in continuous range of colors in the visible part. On the other hand radiation coming from hydrogen atom is a result of predetermined atomic transitions (electrons are jumping from shell to shell) and thus produce discrete values of frequencies resulting in only certain colors making appearance in the spectrum.
Result
2 of 2
Click here for the answer.
Exercise 3
Step 1
1 of 2
Rutherford’s model predicts that electrons are moving around the nucleus in circular orbits. Since every circular motion is accelerated (due to centripetal acceleration) the electron would radiate energy in the form of electromagnetic waves as a charged particle that accelerates. This would result in two things:
1) The electron would loose energy and spiral down to the nucleus and thus atoms would be unstable.
2) While spiraling down it would radiate different frequencies (equal to the current orbiting frequency of the electron) which would result in continuous specter.
This does not meet the experimental data that firmly shows that atom is stable and specter is continuous.
Result
2 of 2
Click here for the answer.
Exercise 4
Step 1
1 of 2
The bright lines of emission spectrum exactly match dark lines on atom’s absorption spectrum.
Result
2 of 2
Click for answer.
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