Cambridge Library Collection - Physical Sciences – serie
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140 produkter
140 produkter
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Astronomer and philosopher J. F. W. Herschel's A Preliminary Discourse on the Study of Natural Philosophy, originally published in 1830, can be regarded as the first modern work on the philosophy of science. In this book, Herschel carefully sets out what he regards as the principles and methods of scientific investigation, both at a theoretical level and at the level of experiment or observation. He describes nature as being governed by laws which are difficult to discern by mere observation and so deduces that theoretical science requires analogical reasoning. In the Discourses, written as the first in a series called Cabinet Cyclopaedia, he covers a wide range of methodological, scientific and philosophical subjects that include discussions of contemporary astronomy, atomism and chemistry. His writing on light is heavily influenced by Newton. Herschel also ponders the differences between human beings and animals and the relationship between religious faith and scientific enquiry.
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Published in 1831, this work forms part of a collection of introductory volumes suggested by Henry, Lord Brougham and Vaux, the Lord Chancellor, for the Society of the Diffusion of Useful Knowledge. Due to the exceptional mathematical ability of its author, however, it outgrew its original plan and has since been seen as a rather more ambitious project. Praised by Somerville's contemporary Sir John Herschel for its presentation of general astronomical theories and the mechanical principles employed in their derivation, the work was a tour de force of scientific and technical exposition. It is especially remarkable both for its author's firm grasp of the subject, especially given her lack of formal mathematical training, and for its clear outline of Newtonian philosophy for a popular audience.
The Scientific Papers of Sir George Darwin
Oceanic Tides and Lunar Disturbance of Gravity
Häftad, Engelska, 2009
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Sir George Darwin (1845-1912) was the second son and fifth child of Charles Darwin. After studying mathematics at Cambridge he read for the Bar, but soon returned to science and to Cambridge, where in 1883 he was appointed Plumian Professor of Astronomy and Experimental Philosophy. His family home is now the location of Darwin College. His work was concerned primarily with the effect of the sun and moon on tidal forces on Earth, and with the theoretical cosmogony which evolved from practical observation: he formulated the fission theory of the formation of the moon (that the moon was formed from still-molten matter pulled away from the Earth by solar tides). He also developed a theory of evolution for the Sun-Earth-Moon system based on mathematical analysis in geophysical theory. This volume of his collected papers covers oceanic tides and lunar disturbances of gravity.
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Sir George Darwin (1845-1912) was the second son and fifth child of Charles Darwin. After studying mathematics at Cambridge he read for the Bar, but soon returned to science and to Cambridge, where in 1883 he was appointed Plumian Professor of Astronomy and Experimental Philosophy. His family home is now the location of Darwin College. His work was concerned primarily with the effect of the sun and moon on tidal forces on Earth, and with the theoretical cosmogony which evolved from practical observation: he formulated the fission theory of the formation of the moon (that the moon was formed from still-molten matter pulled away from the Earth by solar tides). He also developed a theory of evolution for the Sun-Earth-Moon system based on mathematical analysis in geophysical theory. This volume of his collected papers covers tidal friction and cosmogony.
The Scientific Papers of Sir George Darwin
Figures of Equilibrium of Rotating Liquid and Geophysical Investigations
Häftad, Engelska, 2009
654 kr
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Sir George Darwin (1845-1912) was the second son and fifth child of Charles Darwin. After studying mathematics at Cambridge he read for the Bar, but soon returned to science and to Cambridge, where in 1883 he was appointed Plumian Professor of Astronomy and Experimental Philosophy. His family home is now the location of Darwin College. His work was concerned primarily with the effect of the sun and moon on tidal forces on Earth, and with the theoretical cosmogony which evolved from practical observation: he formulated the fission theory of the formation of the moon (that the moon was formed from still-molten matter pulled away from the Earth by solar tides). He also developed a theory of evolution for the Sun-Earth-Moon system based on mathematical analysis in geophysical theory. This volume of his collected papers covers figures of equilibrium of rotating liquid and geophysical investigations.
The Scientific Papers of Sir George Darwin
Periodic Orbits and Miscellaneous Papers
Häftad, Engelska, 2009
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Sir George Darwin (1845-1912) was the second son and fifth child of Charles Darwin. After studying mathematics at Cambridge he read for the Bar, but soon returned to science and to Cambridge, where in 1883 he was appointed Plumian Professor of Astronomy and Experimental Philosophy. His family home is now the location of Darwin College. His work was concerned primarily with the effect of the sun and moon on tidal forces on Earth, and with the theoretical cosmogony which evolved from practical observation: he formulated the fission theory of the formation of the moon (that the moon was formed from still-molten matter pulled away from the Earth by solar tides). This volume of his collected papers covers periodic orbits and some miscellaneous papers, including two investigating the health statistics of the marriage of first cousins - of interest to a member of a dynasty in which such marriages were common.
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Sir George Darwin (1845-1912) was the second son of Charles Darwin. After studying mathematics at Cambridge he read for the Bar, but soon returned to science and to Cambridge, where in 1883 he was appointed Plumian Professor of Astronomy and Experimental Philosophy. His work was concerned primarily with the effect of the sun and moon on tidal forces on Earth, and with the theoretical cosmogony which evolved from practical observation: he formulated the fission theory of the formation of the moon (that the moon was formed from still-molten matter pulled away from the Earth by solar tides). He also developed a theory of evolution for the Sun-Earth-Moon system based on mathematical analysis in geophysical theory. This volume, published in 1916 after the author's death, includes a biographical memoir by his brother Sir Francis Darwin, his inaugural lecture and his lectures on George W. Hill's lunar theory.
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Mary Somerville (1780-1872) would have been a remarkable woman in any age, but as an acknowledged leading mathematician and astronomer at a time when the education of most women was extremely restricted, her achievement was extraordinary. Laplace famously told her that 'There have been only three women who have understood me. These are yourself, Mrs Somerville, Caroline Herschel and a Mrs Greig of whom I know nothing.' Mary Somerville was in fact Mrs Greig. After (as she herself said) translating Laplace's work 'from algebra into common language', she wrote On the Connexion of the Physical Sciences (1834). Her intention was to demonstrate the remarkable tendency of modern scientific discoveries 'to simplify the laws of nature, and to unite detached branches by general principles.' This and her next book, the two-volume Physical Geography, also reissued in this series, were enormously influential both within the scientific community and beyond.
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This book can be described as a student's edition of the author's Dynamical Theory of Gases. It is written, however, with the needs of the student of physics and physical chemistry in mind, and those parts of which the interest was mainly mathematical have been discarded. This does not mean that the book contains no serious mathematical discussion; the discussion in particular of the distribution law is quite detailed; but in the main the mathematics is concerned with the discussion of particular phenomena rather than with the discussion of fundamentals.
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Sir James Jeans' well-known treatise covers the topics in electromagnetic theory required by every non-specialist physicist. It provides the relevant mathematical analysis and is therefore useful to those whose mathematical knowledge is limited, as well as to the more advanced physicists, engineers and applied mathematicians. A large number of examples are given.
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This is the full text of James Jeans's Rouse Ball Lecture given in 1925 at Cambridge University, and surveys the field of atomic and subatomic physics in the early days of quantum mechanics, with a brief historical perspective on measurement.
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Jeans's primary aim with the first edition of his book, originally published in 1904, was to 'develop the theory of gases upon as exact a mathematical basis as possible'. Twenty years later and those theories were being revolutionised by Quantum Theory. In this fourth edition, Jeans does not attempt to avoid the discoveries of this topical science, but rather exposes the many difficulties that classical theory was experiencing, and how those problems disappeared with Quantum Theory. This edition therefore offers a fascinating insight into a field of physics in transition between two great models of physical science.
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The Growth of Physical Science is a detailed but very accessible survey of what began as natural philosophy and culminated in the mid-twentieth century as quantum physical science. From the earliest physical investigations of nature made by the various civilisations of Babylonia, Phoenicia and Egypt (a period covering 5000-600 BC), through the remarkable mathematical and philosophical achievements of the ancient Greeks, to the ages of Newton and then Einstein, Rutherford and Bohr, Jeans has written a comprehensive history of this tremendous advancement in our understanding of the universe, one that will appeal to a broad range of readers interested in this subject.
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Originating from the Rede Lecture delivered at the University of Cambridge in November 1930, this book is based upon the conviction that the teachings and findings of astronomy and physical science are destined to produce an immense change on our outlook on the universe as a whole, and on views about the significance of human life. The author contends that the questions at issue are ultimately one for philosophical discussion, but that before philosophers can speak, science should present ascertained facts and provisional hypotheses. The book is therefore written with these thoughts in mind while broadly presenting the fundamental physical ideas and findings relevant for a wider philosophical inquiry.
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Originally published in 1942, this book discusses an emerging physical science that brought with it a fresh message as to the fundamental nature of the world, and of the possibilities of human free will in particular. The aim of the book is to explore that territory, which forms a borderland between physics and philosophy. The author seeks to estimate the philosophical significance of physical developments, and the interest of his enquiry extends far beyond technical physics and philosophy. Some of the questions raised touch everyday human life closely: can we have knowledge of the world outside us other than that what we can gain by observation and experiment? Is the world spiritual and psychological or material in its ultimate essence; is it better likened to a thought or to a machine? Are we endowed with free will, or are we part of a vast machine that must follow its course until it finally runs down?
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Through Space and Time is based upon the 1933 Christmas Lectures that James Jeans gave at the Royal Institution, London. Intended to appeal to a wide readership and presenting a broad understanding of the Earth, solar system and the universe, the book begins its journey with the history, structure and main features of our planet, and ends in the vast expanses of space among the nebulae.
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Published in 1934 as a second edition to James Jeans' popular work on the general understanding of the physical universe, The New Background of Science took advantage of a comparatively 'quiescent' period in physical investigation when fundamental theories and findings gained wide acceptance. Jeans' aim in writing this book was to depict this 'situation in broad outline and in the simplest possible terms. I have drawn my picture against a roughly sketched background of rudimentary philosophy... because I believe, in common with most scientific workers, that without a background of this kind we can neither see our fresh knowledge as a consistent whole, nor appreciate its significance to the full.'
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The mathematical physicist and engineer William Thomson, 1st Baron Kelvin (1824-1904) is best known for devising the Kelvin scale of absolute temperature and for his work on the first and second laws of thermodynamics. The lectures in this collection demonstrate an attempt by Baron Kelvin to formulate a physical model for the existence of ether. This concept of a medium for light propagation became prominent in the late nineteenth century, arising from the combination of Maxwell's equations stating that light is an electromagnetic wave with the demands of Newtonian physics that light must move in a unique reference frame. First published in 1904, Kelvin's lectures describe the difficulties inherent in this model. These problems with the concept of ether are credited for inspiring Einstein to devise the theory of special relativity and the photoelectric effect, both of which are central to modern physics.
Memoir and Scientific Correspondence of the Late Sir George Gabriel Stokes, Bart.
Selected and Arranged by Joseph Larmor
Häftad, Engelska, 2010
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Lucasian Professor of Mathematics at Cambridge and President of the Royal Society, Sir George Gabriel Stokes (1819-1904) made substantial contributions to the fields of fluid dynamics, optics, physics, and geodesy, in which numerous discoveries still bear his name. The Memoir and Scientific Correspondence of the Late Sir George Gabriel Stokes, Bart., edited by Joseph Larmor, offers rare insight into this capacious scientific mind, with letters attesting to the careful, engaged experimentation that earned him international acclaim. Volume 1 (1907) includes a memoir - culled from the reminiscences of family, friends, and colleagues - and letters, including early correspondence with Lady Stokes during the time of their engagement and early marriage. Professional correspondence covers Stokes' discoveries in the areas of spectroscopy, fluorescence, and colour vision. The result is an intimate portrait of a brilliant mathematician - both in the early stages of his career and at the height of his intellectual powers.
Memoir and Scientific Correspondence of the Late Sir George Gabriel Stokes, Bart.
Selected and Arranged by Joseph Larmor
Häftad, Engelska, 2010
666 kr
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Lucasian Professor of Mathematics at Cambridge and President of the Royal Society, Sir George Gabriel Stokes (1819-1904) made substantial contributions to the fields of fluid dynamics, optics, physics, and geodesy, in which numerous discoveries still bear his name. The Memoir and Scientific Correspondence of the Late Sir George Gabriel Stokes, Bart., edited by Joseph Larmor, offers rare insight into this capacious scientific mind, with letters attesting to the careful, engaged experimentation that earned him international acclaim. Volume 2 (1907) includes important professional correspondence with James Clerk Maxwell, James Prescott Joule, and many others, with particular attention given to Stokes' activities with the British Meteorological Society. Many of his foundational innovations in optics are also explicated in these letters, serving in place of the authoritative volume he unfortunately never had the opportunity to complete.
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Sir Ernest Rutherford (1871-1937) was a New Zealand-born physicist who has become known as the 'father of nuclear physics' for his discovery of the so-called planetary structure of atoms. He was awarded the Nobel Prize in Chemistry in 1908. His co-authors, James Chadwick and Charles D. Ellis also made significant discoveries in the field of nuclear physics, with Chadwick discovering the neutron particle in 1932. Research in nuclear physics in the 1930s had become focused on investigating the natures of alpha, beta and gamma radiation and their effects on matter and atomic structure. This volume provides a definitive account of the state of research into these types of radiation in 1930, explaining the theory and process behind inferring the structure of the atom and the structure of the nucleus. The text of this volume is taken from a 1951 reissue of the 1930 edition.
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Henry Cavendish (1731-1810), the grandson of the second duke of Devonshire, wrote papers on electrical topics for the Royal Society, but the majority of his electrical experiments did not become known until they were collected and published by James Clerk Maxwell a century later, in 1879, long after other scientists had been credited with the same results. Among Cavendish's discoveries were the concept of electric potential, which he called the 'degree of electrification'; an early unit of capacitance, that of a sphere one inch in diameter; the formula for the capacitance of a plate capacitor; the concept of the dielectric constant of a material; the relationship between electric potential and current, now called Ohm's Law; laws for the division of current in parallel circuits, now attributed to Charles Wheatstone; and the inverse square law of variation of electric force with distance, now called Coulomb's Law.
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The publication in 1890 of the two-volume Scientific Papers of James Clerk Maxwell, edited by W. D. Niven, was one of the two objects of a committee formed 'for the purpose of securing a fitting memorial of him' (the other object being the commissioning of a marble bust for the Cavendish Laboratory). Before his death in 1879 at the age of 48, Clerk Maxwell had made major contributions to many areas of theoretical physics and mathematics, not least his discoveries in the fields of electromagnetism and of the kinetic theory of gases, which have been regarded as laying the foundations of all modern physics. He is generally considered the third most important physicist of all time, after Newton and Einstein. These collected shorter works, beginning with a paper written at the age of 15, show the wide range of Clerk Maxwell's interests across mathematics, physics and chemistry.
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Polymath Alexander von Humboldt (1769-1859), a self-described 'scientific traveller', was one of the most respected scientists of his time. Humboldt's wanderlust led him across Europe and to South America, Mexico, the U.S., and Russia, and his voyages and observations resulted in the discovery of many species previously unknown to Europeans. Originating as lectures delivered in Berlin and Paris (1827-1828), his multi-volume Cosmos: Sketch of a Physical Description of the Universe (1845-1860) represented the culmination of his lifelong interest in understanding the physical world. As Humboldt writes, 'I ever desired to discern physical phenomena in their widest mutual connection, and to comprehend Nature as a whole, animated and moved by inward forces.' Volume 1 (1846) investigates celestial and terrestrial phenomena, from nebulae to the temperature of the earth, as well as 'organic life'. Throughout, he stresses the method of, and limits to, describing the universe's physical nature.
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Polymath Alexander von Humboldt (1769-1859), a self-described 'scientific traveller', was one of the most respected scientists of his time. Humboldt's wanderlust led him across Europe and to South America, Mexico, the U.S. and Russia, and his voyages and observations resulted in the discovery of many species previously unknown to Europeans. Originating as lectures delivered in Berlin and Paris (1827-1828), his two-volume Cosmos: Sketch of a Physical Description of the Universe (1845-1860) represented the culmination of his lifelong interest in understanding the physical world. As Humboldt writes, 'I ever desired to discern physical phenomena in their widest mutual connection, and to comprehend Nature as a whole, animated and moved by inward forces'. Volume 2 (1848) reviews poetic descriptions of nature as well as landscape painting from antiquity through to modernity, before using the same time-span to examine a 'History of the Physical Contemplation of the Universe'.
Personal Recollections, from Early Life to Old Age
With Selections from her Correspondence
Häftad, Engelska, 2010
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These Personal Recollections contain the memoirs and a selection of the correspondence of the nineteenth-century polymath Mary Somerville (1780-1872). The book was first published in 1873, a year after Mary's death, by her daughter Martha, who wrote brief introductions to the text. Mary Somerville is best known for her pioneering scientific publications which include her translation of Laplace's Mécanique Céleste (1831: also resissued in this series); On the Connection of the Physical Sciences (1834); Physical Geography (1848); and On Molecular and Microscopic Science (1869). Through these publications, Somerville made a lasting contribution to the dissemination of scientific knowledge. Somerville's correspondence deals primarily with her public life, while the memoirs offer insight into her private sphere: the discouragement she faced in pursuit of learning; her passion for women's education and suffrage; family life; and personal faith. Her story is compelling, and her experiences may resonate with many women today.
The Life of James Clerk Maxwell
With a Selection from his Correspondence and Occasional Writings and a Sketch of his Contributions to Science
Häftad, Engelska, 2010
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James Clerk Maxwell (1831-1879) was a Scottish physicist well-known for his extensive work with electromagnetism, colour analysis, and kinetic theory. Considered by many to be a giant in his field with significant influence on the physicists who would follow, Maxwell spent time as a professor at Aberdeen University, King's College, London, and Cambridge. This 1882 Life by his friend Lewis Campbell and natural philosopher William Garnett represents an important - and lengthy - investigation into Maxwell's life and thought. Part I is concerned with biographical matters while the second section focuses upon his scientific mind. A third part contains Maxwell's poetry, so included because the poems are 'characteristic of him' and have 'curious biographical interest'. At nearly 700 pages, the Life represents an important starting point for those curious about the state of theoretical physics and the person in whom it reached its culmination in the nineteenth century.
Biographical Memoir of James Dinwiddie, L.L.D., Astronomer in the British Embassy to China, 1792, '3, '4,
Afterwards Professor of Natural Philosophy in the College of Fort William, Bengal
Häftad, Engelska, 2010
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This is an account of the career of James Dinwiddie (1746-1815). First published in 1868 by Dinwiddie's grandson William Jardine Proudfoot, the work is based on Dinwiddie's own autobiographical notes, travel logbook and personal correspondence. The biography traces Dinwiddie's career from the scientific lectures he gave from 1781 and the journal series Queries and Hints, which he began in 1779, to his visit to the Chinese imperial court as official astronomer in Lord Macartney's mission (1792-1794); his residence in Beijing and Canton; and his move to India, where he was appointed Professor of Mathematics, Natural Philosophy and Chemistry at the College of Fort William, Bengal. Dinwiddie's career was marked by passionate commitment to the dissemination of scientific knowledge - his travels, lectures and publications were undertaken for this cause. His life is a fascinating account of a polymathic mind which will fascinate and entertain a modern-day readership.
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Published posthumously in 1888, this treatise by the first Cavendish Professor of Physics at Cambridge explores and explains the fundamental principles and laws that are the basis of elementary physics. Maxwell was at the forefront of physics and mathematics during the nineteenth century and his pioneering work brought together existing ideas to give 'a dynamical theory of the electromagnetic field'. This work inspired not only the applications of electromagnetic waves like fibre optics but also Einstein's theory of relativity. The text explains many of Newton's laws and the unifying concepts that govern a body and its motion. The increment in the complexity of topics allows one to build a solid understanding of the accepted laws of mathematical physics that explain topics like force, work, energy and the centre mass point of a material system. This logical guide and instruction is as timeless as the laws of physics that it explains.
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Arguably the most influential nineteenth-century scientist for twentieth-century physics, James Clerk Maxwell (1831-1879) demonstrated that electricity, magnetism and light are all manifestations of the same phenomenon: the electromagnetic field. A fellow of Trinity College Cambridge, Maxwell became, in 1871, the first Cavendish Professor of Physics at Cambridge. His famous equations - a set of four partial differential equations that relate the electric and magnetic fields to their sources, charge density and current density - first appeared in fully developed form in his 1873 Treatise on Electricity and Magnetism. This two-volume textbook brought together all the experimental and theoretical advances in the field of electricity and magnetism known at the time, and provided a methodical and graduated introduction to electromagnetism. Volume 1 covers the first elements of Maxwell's electromagnetic theory: electrostatics, and electrokinematics, including detailed analyses of electrolysis, conduction in three dimensions, and conduction through heterogeneous media.