Thermal and statistical physics has established the principles and procedures needed to understand and explain the properties of systems consisting of macroscopically large numbers of particles. By developing microscopic statistical physics and macroscopic classical thermodynamic descriptions in tandem, Statistical and Thermal Physics: An Introduction provides insight into basic concepts and relationships at an advanced undergraduate level. This second edition is updated throughout, providing a highly detailed, profoundly thorough, and comprehensive introduction to the subject and features exercises within the text as well as end-of-chapter problems. Part I of this book consists of nine chapters, the first three of which deal with the basics of equilibrium thermodynamics, including the fundamental relation. The following three chapters introduce microstates and lead to the Boltzmann definition of the entropy using the microcanonical ensemble approach. In developing the subject, the ideal gas and the ideal spin system are introduced as models for discussion. The laws of thermodynamics are compactly stated. The final three chapters in Part I introduce the thermodynamic potentials and the Maxwell relations. Applications of thermodynamics to gases, condensed matter, and phase transitions and critical phenomena are dealt with in detail. Initial chapters in Part II present the elements of probability theory and establish the thermodynamic equivalence of the three statistical ensembles that are used in determining probabilities. The canonical and the grand canonical distributions are obtained and discussed. Chapters 12-15 are concerned with quantum distributions. By making use of the grand canonical distribution, the Fermi–Dirac and Bose–Einstein quantum distribution functions are derived and then used to explain the properties of ideal Fermi and Bose gases. The Planck distribution is introduced and applied to photons in radiation and to phonons on solids. The last five chapters cover a variety of topics: the ideal gas revisited, nonideal systems, the density matrix, reactions, and irreversible thermodynamics. A flowchart is provided to assist instructors on planning a course. Key Features: Fully updated throughout, with new content on exciting topics, including black hole thermodynamics, Heisenberg antiferromagnetic chains, entropy and information theory, renewable and nonrenewable energy sources, and the mean field theory of antiferromagnetic systems Additional problem exercises with solutions provide further learning opportunities Suitable for advanced undergraduate students in physics or applied physics. Michael J.R. Hoch spent many years as a visiting scientist at the National High Magnetic Field Laboratory at Florida State University, USA. Prior to this, he was a professor of physics and the director of the Condensed Matter Physics Research Unit at the University of the Witwatersrand, Johannesburg, where he is currently professor emeritus in the School of Physics.

Thermal and statistical physics has established the principles and procedures needed to understand and explain the properties of systems consisting of macroscopically large numbers of particles. By developing microscopic statistical physics and macroscopic classical thermodynamic descriptions in tandem, Statistical and Thermal Physics: An Introduction provides insight into basic concepts and relationships at an advanced undergraduate level. This second edition is updated throughout, providing a highly detailed, profoundly thorough, and comprehensive introduction to the subject and features exercises within the text as well as end-of-chapter problems. Part I of this book consists of nine chapters, the first three of which deal with the basics of equilibrium thermodynamics, including the fundamental relation. The following three chapters introduce microstates and lead to the Boltzmann definition of the entropy using the microcanonical ensemble approach. In developing the subject, the ideal gas and the ideal spin system are introduced as models for discussion. The laws of thermodynamics are compactly stated. The final three chapters in Part I introduce the thermodynamic potentials and the Maxwell relations. Applications of thermodynamics to gases, condensed matter, and phase transitions and critical phenomena are dealt with in detail. Initial chapters in Part II present the elements of probability theory and establish the thermodynamic equivalence of the three statistical ensembles that are used in determining probabilities. The canonical and the grand canonical distributions are obtained and discussed. Chapters 12-15 are concerned with quantum distributions. By making use of the grand canonical distribution, the Fermi–Dirac and Bose–Einstein quantum distribution functions are derived and then used to explain the properties of ideal Fermi and Bose gases. The Planck distribution is introduced and applied to photons in radiation and to phonons on solids. The last five chapters cover a variety of topics: the ideal gas revisited, nonideal systems, the density matrix, reactions, and irreversible thermodynamics. A flowchart is provided to assist instructors on planning a course. Key Features: Fully updated throughout, with new content on exciting topics, including black hole thermodynamics, Heisenberg antiferromagnetic chains, entropy and information theory, renewable and nonrenewable energy sources, and the mean field theory of antiferromagnetic systems Additional problem exercises with solutions provide further learning opportunities Suitable for advanced undergraduate students in physics or applied physics. Michael J.R. Hoch spent many years as a visiting scientist at the National High Magnetic Field Laboratory at Florida State University, USA. Prior to this, he was a professor of physics and the director of the Condensed Matter Physics Research Unit at the University of the Witwatersrand, Johannesburg, where he is currently professor emeritus in the School of Physics.

Thermal and statistical physics has established the principles and procedures needed to understand and explain the properties of systems consisting of macroscopically large numbers of particles. By developing microscopic statistical physics and macroscopic classical thermodynamic descriptions in tandem, Statistical and Thermal Physics: An Introduction provides insight into basic concepts and relationships at an advanced undergraduate level. This second edition is updated throughout, providing a highly detailed, profoundly thorough, and comprehensive introduction to the subject and features exercises within the text as well as end-of-chapter problems.

Part I of this book consists of nine chapters, the first three of which deal with the basics of equilibrium thermodynamics, including the fundamental relation. The following three chapters introduce microstates and lead to the Boltzmann definition of the entropy using the microcanonical ensemble approach. In developing the subject, the ideal gas and the ideal spin system are introduced as models for discussion. The laws of thermodynamics are compactly stated. The final three chapters in Part I introduce the thermodynamic potentials and the Maxwell relations. Applications of thermodynamics to gases, condensed matter, and phase transitions and critical phenomena are dealt with in detail.

Initial chapters in Part II present the elements of probability theory and establish the thermodynamic equivalence of the three statistical ensembles that are used in determining probabilities. The canonical and the grand canonical distributions are obtained and discussed. Chapters 12-15 are concerned with quantum distributions. By making use of the grand canonical distribution, the Fermi–Dirac and Bose–Einstein quantum distribution functions are derived and then used to explain the properties of ideal Fermi and Bose gases. The Planck distribution is introduced and applied to photons in radiation and to phonons on solids. The last five chapters cover a variety of topics: the ideal gas revisited, nonideal systems, the density matrix, reactions, and irreversible thermodynamics. A flowchart is provided to assist instructors on planning a course.

Key Features:

Fully updated throughout, with new content on exciting topics, including black hole thermodynamics, Heisenberg antiferromagnetic chains, entropy and information theory, renewable and nonrenewable energy sources, and the mean field theory of antiferromagnetic systems

Additional problem exercises with solutions provide further learning opportunities

Suitable for advanced undergraduate students in physics or applied physics.

Michael J.R. Hoch spent many years as a visiting scientist at the National High Magnetic Field Laboratory at Florida State University, USA. Prior to this, he was a professor of physics and the director of the Condensed Matter Physics Research Unit at the University of the Witwatersrand, Johannesburg, where he is currently professor emeritus in the School of Physics.

Thermal and statistical physics has established the principles and procedures needed to understand and explain the properties of systems consisting of macroscopically large numbers of particles. By developing microscopic statistical physics and macroscopic classical thermodynamic descriptions in tandem, Statistical and Thermal Physics: An Introduction provides insight into basic concepts and relationships at an advanced undergraduate level. This second edition is updated throughout, providing a highly detailed, profoundly thorough, and comprehensive introduction to the subject and features exercises within the text as well as end-of-chapter problems.

Part I of this book consists of nine chapters, the first three of which deal with the basics of equilibrium thermodynamics, including the fundamental relation. The following three chapters introduce microstates and lead to the Boltzmann definition of the entropy using the microcanonical ensemble approach. In developing the subject, the ideal gas and the ideal spin system are introduced as models for discussion. The laws of thermodynamics are compactly stated. The final three chapters in Part I introduce the thermodynamic potentials and the Maxwell relations. Applications of thermodynamics to gases, condensed matter, and phase transitions and critical phenomena are dealt with in detail.

Initial chapters in Part II present the elements of probability theory and establish the thermodynamic equivalence of the three statistical ensembles that are used in determining probabilities. The canonical and the grand canonical distributions are obtained and discussed. Chapters 12-15 are concerned with quantum distributions. By making use of the grand canonical distribution, the Fermi–Dirac and Bose–Einstein quantum distribution functions are derived and then used to explain the properties of ideal Fermi and Bose gases. The Planck distribution is introduced and applied to photons in radiation and to phonons on solids. The last five chapters cover a variety of topics: the ideal gas revisited, nonideal systems, the density matrix, reactions, and irreversible thermodynamics. A flowchart is provided to assist instructors on planning a course.

Key Features:

Fully updated throughout, with new content on exciting topics, including black hole thermodynamics, Heisenberg antiferromagnetic chains, entropy and information theory, renewable and nonrenewable energy sources, and the mean field theory of antiferromagnetic systems

Additional problem exercises with solutions provide further learning opportunities

Suitable for advanced undergraduate students in physics or applied physics.

Michael J.R. Hoch spent many years as a visiting scientist at the National High Magnetic Field Laboratory at Florida State University, USA. Prior to this, he was a professor of physics and the director of the Condensed Matter Physics Research Unit at the University of the Witwatersrand, Johannesburg, where he is currently professor emeritus in the School of Physics.

Physics: An Introduction to Physical Dynamics provides an accessible introduction to the fundamentals of physics for science and engineering undergraduates who are studying elementary physics.This textbook contains 12 chapters with accompanying problem sets and explains the dynamical properties of a variety of physical systems. The first six chapters intro- duce Newton’s laws of motion, followed by the concepts of mechanical work and mechanical energy, with illustrative applications to the translational and/or rotational motion of inflexible objects such as particles and 3D objects of fixed shape. The next four chapters generalize the application of Newton’s laws and mechanical energy to flexible systems, including flowing fluids, waves on strings, and oscillating springs. The last two chapters elucidate the laws of thermodynamics, especially heat energy transfer between systems at different temperatures.Some familiarity with topics in elementary mathematics, including calculus, is assumed. A wide variety of situations are explored, by means of which a student should acquire an enhanced understanding of the properties of physical systems from the astronomic scale to the microscopic.Key FeaturesCovers the classical mechanics of both single particles and assemblies of particles subject to forcesContains wide-ranging sets of examples and worked problemsCovers much of the material that a student might expect to encounter during the first year of a university physics course

Physics: An Introduction to Physical Dynamics provides an accessible introduction to the fundamentals of physics for science and engineering undergraduates who are studying elementary physics.This textbook contains 12 chapters with accompanying problem sets and explains the dynamical properties of a variety of physical systems. The first six chapters intro- duce Newton’s laws of motion, followed by the concepts of mechanical work and mechanical energy, with illustrative applications to the translational and/or rotational motion of inflexible objects such as particles and 3D objects of fixed shape. The next four chapters generalize the application of Newton’s laws and mechanical energy to flexible systems, including flowing fluids, waves on strings, and oscillating springs. The last two chapters elucidate the laws of thermodynamics, especially heat energy transfer between systems at different temperatures.Some familiarity with topics in elementary mathematics, including calculus, is assumed. A wide variety of situations are explored, by means of which a student should acquire an enhanced understanding of the properties of physical systems from the astronomic scale to the microscopic.Key FeaturesCovers the classical mechanics of both single particles and assemblies of particles subject to forcesContains wide-ranging sets of examples and worked problemsCovers much of the material that a student might expect to encounter during the first year of a university physics course

Physics: An Introduction to Physical Dynamics provides an accessible introduction to the fundamentals of physics for science and engineering undergraduates who are studying elementary physics.

This textbook contains 12 chapters with accompanying problem sets and explains the dynamical properties of a variety of physical systems. The first six chapters intro- duce Newton’s laws of motion, followed by the concepts of mechanical work and mechanical energy, with illustrative applications to the translational and/or rotational motion of inflexible objects such as particles and 3D objects of fixed shape. The next four chapters generalize the application of Newton’s laws and mechanical energy to flexible systems, including flowing fluids, waves on strings, and oscillating springs. The last two chapters elucidate the laws of thermodynamics, especially heat energy transfer between systems at different temperatures.

Some familiarity with topics in elementary mathematics, including calculus, is assumed. A wide variety of situations are explored, by means of which a student should acquire an enhanced understanding of the properties of physical systems from the astronomic scale to the microscopic.

Key Features

Covers the classical mechanics of both single particles and assemblies of particles subject to forces Contains wide-ranging sets of examples and worked problems Covers much of the material that a student might expect to encounter during the first year of a university physics course

Physics: An Introduction to Physical Dynamics provides an accessible introduction to the fundamentals of physics for science and engineering undergraduates who are studying elementary physics.

This textbook contains 12 chapters with accompanying problem sets and explains the dynamical properties of a variety of physical systems. The first six chapters intro- duce Newton’s laws of motion, followed by the concepts of mechanical work and mechanical energy, with illustrative applications to the translational and/or rotational motion of inflexible objects such as particles and 3D objects of fixed shape. The next four chapters generalize the application of Newton’s laws and mechanical energy to flexible systems, including flowing fluids, waves on strings, and oscillating springs. The last two chapters elucidate the laws of thermodynamics, especially heat energy transfer between systems at different temperatures.

Some familiarity with topics in elementary mathematics, including calculus, is assumed. A wide variety of situations are explored, by means of which a student should acquire an enhanced understanding of the properties of physical systems from the astronomic scale to the microscopic.

Key Features

Covers the classical mechanics of both single particles and assemblies of particles subject to forces Contains wide-ranging sets of examples and worked problems Covers much of the material that a student might expect to encounter during the first year of a university physics course

Thermal and statistical physics has established the principles and procedures needed to understand and explain the properties of systems consisting of macroscopically large numbers of particles. By developing microscopic statistical physics and macroscopic classical thermodynamic descriptions in tandem, Statistical and Thermal Physics: An Introduction provides insight into basic concepts and relationships at an advanced undergraduate level. This second edition is updated throughout, providing a highly detailed, profoundly thorough, and comprehensive introduction to the subject and features exercises within the text as well as end-of-chapter problems. Part I of this book consists of nine chapters, the first three of which deal with the basics of equilibrium thermodynamics, including the fundamental relation. The following three chapters introduce microstates and lead to the Boltzmann definition of the entropy using the microcanonical ensemble approach. In developing the subject, the ideal gas and the ideal spin system are introduced as models for discussion. The laws of thermodynamics are compactly stated. The final three chapters in Part I introduce the thermodynamic potentials and the Maxwell relations. Applications of thermodynamics to gases, condensed matter, and phase transitions and critical phenomena are dealt with in detail. Initial chapters in Part II present the elements of probability theory and establish the thermodynamic equivalence of the three statistical ensembles that are used in determining probabilities. The canonical and the grand canonical distributions are obtained and discussed. Chapters 12-15 are concerned with quantum distributions. By making use of the grand canonical distribution, the Fermi–Dirac and Bose–Einstein quantum distribution functions are derived and then used to explain the properties of ideal Fermi and Bose gases. The Planck distribution is introduced and applied to photons in radiation and to phonons on solids. The last five chapters cover a variety of topics: the ideal gas revisited, nonideal systems, the density matrix, reactions, and irreversible thermodynamics. A flowchart is provided to assist instructors on planning a course. Key Features: Fully updated throughout, with new content on exciting topics, including black hole thermodynamics, Heisenberg antiferromagnetic chains, entropy and information theory, renewable and nonrenewable energy sources, and the mean field theory of antiferromagnetic systems Additional problem exercises with solutions provide further learning opportunities Suitable for advanced undergraduate students in physics or applied physics. Michael J.R. Hoch spent many years as a visiting scientist at the National High Magnetic Field Laboratory at Florida State University, USA. Prior to this, he was a professor of physics and the director of the Condensed Matter Physics Research Unit at the University of the Witwatersrand, Johannesburg, where he is currently professor emeritus in the School of Physics.

Thermal and statistical physics has established the principles and procedures needed to understand and explain the properties of systems consisting of macroscopically large numbers of particles. By developing microscopic statistical physics and macroscopic classical thermodynamic descriptions in tandem, Statistical and Thermal Physics: An Introduction provides insight into basic concepts and relationships at an advanced undergraduate level. This second edition is updated throughout, providing a highly detailed, profoundly thorough, and comprehensive introduction to the subject and features exercises within the text as well as end-of-chapter problems. Part I of this book consists of nine chapters, the first three of which deal with the basics of equilibrium thermodynamics, including the fundamental relation. The following three chapters introduce microstates and lead to the Boltzmann definition of the entropy using the microcanonical ensemble approach. In developing the subject, the ideal gas and the ideal spin system are introduced as models for discussion. The laws of thermodynamics are compactly stated. The final three chapters in Part I introduce the thermodynamic potentials and the Maxwell relations. Applications of thermodynamics to gases, condensed matter, and phase transitions and critical phenomena are dealt with in detail. Initial chapters in Part II present the elements of probability theory and establish the thermodynamic equivalence of the three statistical ensembles that are used in determining probabilities. The canonical and the grand canonical distributions are obtained and discussed. Chapters 12-15 are concerned with quantum distributions. By making use of the grand canonical distribution, the Fermi–Dirac and Bose–Einstein quantum distribution functions are derived and then used to explain the properties of ideal Fermi and Bose gases. The Planck distribution is introduced and applied to photons in radiation and to phonons on solids. The last five chapters cover a variety of topics: the ideal gas revisited, nonideal systems, the density matrix, reactions, and irreversible thermodynamics. A flowchart is provided to assist instructors on planning a course. Key Features: Fully updated throughout, with new content on exciting topics, including black hole thermodynamics, Heisenberg antiferromagnetic chains, entropy and information theory, renewable and nonrenewable energy sources, and the mean field theory of antiferromagnetic systems Additional problem exercises with solutions provide further learning opportunities Suitable for advanced undergraduate students in physics or applied physics. Michael J.R. Hoch spent many years as a visiting scientist at the National High Magnetic Field Laboratory at Florida State University, USA. Prior to this, he was a professor of physics and the director of the Condensed Matter Physics Research Unit at the University of the Witwatersrand, Johannesburg, where he is currently professor emeritus in the School of Physics.

Thermal and statistical physics has established the principles and procedures needed to understand and explain the properties of systems consisting of macroscopically large numbers of particles. By developing microscopic statistical physics and macroscopic classical thermodynamic descriptions in tandem, Statistical and Thermal Physics: An Introduction provides insight into basic concepts and relationships at an advanced undergraduate level. This second edition is updated throughout, providing a highly detailed, profoundly thorough, and comprehensive introduction to the subject and features exercises within the text as well as end-of-chapter problems.

Part I of this book consists of nine chapters, the first three of which deal with the basics of equilibrium thermodynamics, including the fundamental relation. The following three chapters introduce microstates and lead to the Boltzmann definition of the entropy using the microcanonical ensemble approach. In developing the subject, the ideal gas and the ideal spin system are introduced as models for discussion. The laws of thermodynamics are compactly stated. The final three chapters in Part I introduce the thermodynamic potentials and the Maxwell relations. Applications of thermodynamics to gases, condensed matter, and phase transitions and critical phenomena are dealt with in detail.

Initial chapters in Part II present the elements of probability theory and establish the thermodynamic equivalence of the three statistical ensembles that are used in determining probabilities. The canonical and the grand canonical distributions are obtained and discussed. Chapters 12-15 are concerned with quantum distributions. By making use of the grand canonical distribution, the Fermi–Dirac and Bose–Einstein quantum distribution functions are derived and then used to explain the properties of ideal Fermi and Bose gases. The Planck distribution is introduced and applied to photons in radiation and to phonons on solids. The last five chapters cover a variety of topics: the ideal gas revisited, nonideal systems, the density matrix, reactions, and irreversible thermodynamics. A flowchart is provided to assist instructors on planning a course.

Key Features:

Fully updated throughout, with new content on exciting topics, including black hole thermodynamics, Heisenberg antiferromagnetic chains, entropy and information theory, renewable and nonrenewable energy sources, and the mean field theory of antiferromagnetic systems

Additional problem exercises with solutions provide further learning opportunities

Suitable for advanced undergraduate students in physics or applied physics.

Michael J.R. Hoch spent many years as a visiting scientist at the National High Magnetic Field Laboratory at Florida State University, USA. Prior to this, he was a professor of physics and the director of the Condensed Matter Physics Research Unit at the University of the Witwatersrand, Johannesburg, where he is currently professor emeritus in the School of Physics.

Thermal and statistical physics has established the principles and procedures needed to understand and explain the properties of systems consisting of macroscopically large numbers of particles. By developing microscopic statistical physics and macroscopic classical thermodynamic descriptions in tandem, Statistical and Thermal Physics: An Introduction provides insight into basic concepts and relationships at an advanced undergraduate level. This second edition is updated throughout, providing a highly detailed, profoundly thorough, and comprehensive introduction to the subject and features exercises within the text as well as end-of-chapter problems.

Part I of this book consists of nine chapters, the first three of which deal with the basics of equilibrium thermodynamics, including the fundamental relation. The following three chapters introduce microstates and lead to the Boltzmann definition of the entropy using the microcanonical ensemble approach. In developing the subject, the ideal gas and the ideal spin system are introduced as models for discussion. The laws of thermodynamics are compactly stated. The final three chapters in Part I introduce the thermodynamic potentials and the Maxwell relations. Applications of thermodynamics to gases, condensed matter, and phase transitions and critical phenomena are dealt with in detail.

Initial chapters in Part II present the elements of probability theory and establish the thermodynamic equivalence of the three statistical ensembles that are used in determining probabilities. The canonical and the grand canonical distributions are obtained and discussed. Chapters 12-15 are concerned with quantum distributions. By making use of the grand canonical distribution, the Fermi–Dirac and Bose–Einstein quantum distribution functions are derived and then used to explain the properties of ideal Fermi and Bose gases. The Planck distribution is introduced and applied to photons in radiation and to phonons on solids. The last five chapters cover a variety of topics: the ideal gas revisited, nonideal systems, the density matrix, reactions, and irreversible thermodynamics. A flowchart is provided to assist instructors on planning a course.

Key Features:

Fully updated throughout, with new content on exciting topics, including black hole thermodynamics, Heisenberg antiferromagnetic chains, entropy and information theory, renewable and nonrenewable energy sources, and the mean field theory of antiferromagnetic systems

Additional problem exercises with solutions provide further learning opportunities

Suitable for advanced undergraduate students in physics or applied physics.

Michael J.R. Hoch spent many years as a visiting scientist at the National High Magnetic Field Laboratory at Florida State University, USA. Prior to this, he was a professor of physics and the director of the Condensed Matter Physics Research Unit at the University of the Witwatersrand, Johannesburg, where he is currently professor emeritus in the School of Physics.

Physics: An Introduction to Physical Dynamics provides an accessible introduction to the fundamentals of physics for science and engineering undergraduates who are studying elementary physics.This textbook contains 12 chapters with accompanying problem sets and explains the dynamical properties of a variety of physical systems. The first six chapters intro- duce Newton’s laws of motion, followed by the concepts of mechanical work and mechanical energy, with illustrative applications to the translational and/or rotational motion of inflexible objects such as particles and 3D objects of fixed shape. The next four chapters generalize the application of Newton’s laws and mechanical energy to flexible systems, including flowing fluids, waves on strings, and oscillating springs. The last two chapters elucidate the laws of thermodynamics, especially heat energy transfer between systems at different temperatures.Some familiarity with topics in elementary mathematics, including calculus, is assumed. A wide variety of situations are explored, by means of which a student should acquire an enhanced understanding of the properties of physical systems from the astronomic scale to the microscopic.Key FeaturesCovers the classical mechanics of both single particles and assemblies of particles subject to forcesContains wide-ranging sets of examples and worked problemsCovers much of the material that a student might expect to encounter during the first year of a university physics course

Physics: An Introduction to Physical Dynamics provides an accessible introduction to the fundamentals of physics for science and engineering undergraduates who are studying elementary physics.This textbook contains 12 chapters with accompanying problem sets and explains the dynamical properties of a variety of physical systems. The first six chapters intro- duce Newton’s laws of motion, followed by the concepts of mechanical work and mechanical energy, with illustrative applications to the translational and/or rotational motion of inflexible objects such as particles and 3D objects of fixed shape. The next four chapters generalize the application of Newton’s laws and mechanical energy to flexible systems, including flowing fluids, waves on strings, and oscillating springs. The last two chapters elucidate the laws of thermodynamics, especially heat energy transfer between systems at different temperatures.Some familiarity with topics in elementary mathematics, including calculus, is assumed. A wide variety of situations are explored, by means of which a student should acquire an enhanced understanding of the properties of physical systems from the astronomic scale to the microscopic.Key FeaturesCovers the classical mechanics of both single particles and assemblies of particles subject to forcesContains wide-ranging sets of examples and worked problemsCovers much of the material that a student might expect to encounter during the first year of a university physics course

Physics: An Introduction to Physical Dynamics provides an accessible introduction to the fundamentals of physics for science and engineering undergraduates who are studying elementary physics.

This textbook contains 12 chapters with accompanying problem sets and explains the dynamical properties of a variety of physical systems. The first six chapters intro- duce Newton’s laws of motion, followed by the concepts of mechanical work and mechanical energy, with illustrative applications to the translational and/or rotational motion of inflexible objects such as particles and 3D objects of fixed shape. The next four chapters generalize the application of Newton’s laws and mechanical energy to flexible systems, including flowing fluids, waves on strings, and oscillating springs. The last two chapters elucidate the laws of thermodynamics, especially heat energy transfer between systems at different temperatures.

Some familiarity with topics in elementary mathematics, including calculus, is assumed. A wide variety of situations are explored, by means of which a student should acquire an enhanced understanding of the properties of physical systems from the astronomic scale to the microscopic.

Key Features

Covers the classical mechanics of both single particles and assemblies of particles subject to forces Contains wide-ranging sets of examples and worked problems Covers much of the material that a student might expect to encounter during the first year of a university physics course

Physics: An Introduction to Physical Dynamics provides an accessible introduction to the fundamentals of physics for science and engineering undergraduates who are studying elementary physics.

This textbook contains 12 chapters with accompanying problem sets and explains the dynamical properties of a variety of physical systems. The first six chapters intro- duce Newton’s laws of motion, followed by the concepts of mechanical work and mechanical energy, with illustrative applications to the translational and/or rotational motion of inflexible objects such as particles and 3D objects of fixed shape. The next four chapters generalize the application of Newton’s laws and mechanical energy to flexible systems, including flowing fluids, waves on strings, and oscillating springs. The last two chapters elucidate the laws of thermodynamics, especially heat energy transfer between systems at different temperatures.

Some familiarity with topics in elementary mathematics, including calculus, is assumed. A wide variety of situations are explored, by means of which a student should acquire an enhanced understanding of the properties of physical systems from the astronomic scale to the microscopic.

Key Features

Covers the classical mechanics of both single particles and assemblies of particles subject to forces Contains wide-ranging sets of examples and worked problems Covers much of the material that a student might expect to encounter during the first year of a university physics course