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Tuesday, September 26, 2023

Geometry

From Wikipedia, the free encyclopedia
https://en.wikipedia.org/wiki/Geometry

Geometry (from Ancient Greek γεωμετρία (geōmetría) 'land measurement'; from γῆ () 'earth, land', and μέτρον (métron) 'a measure') is a branch of mathematics concerned with properties of space such as the distance, shape, size, and relative position of figures. Geometry is, along with arithmetic, one of the oldest branches of mathematics. A mathematician who works in the field of geometry is called a geometer. Until the 19th century, geometry was almost exclusively devoted to Euclidean geometry, which includes the notions of point, line, plane, distance, angle, surface, and curve, as fundamental concepts.

Originally developed to model the physical world, geometry has applications in almost all sciences, and also in art, architecture, and other activities that are related to graphics. Geometry also has applications in areas of mathematics that are apparently unrelated. For example, methods of algebraic geometry are fundamental in Wiles's proof of Fermat's Last Theorem, a problem that was stated in terms of elementary arithmetic, and remained unsolved for several centuries.

During the 19th century several discoveries enlarged dramatically the scope of geometry. One of the oldest such discoveries is Carl Friedrich Gauss' Theorema Egregium ("remarkable theorem") that asserts roughly that the Gaussian curvature of a surface is independent from any specific embedding in a Euclidean space. This implies that surfaces can be studied intrinsically, that is, as stand-alone spaces, and has been expanded into the theory of manifolds and Riemannian geometry. Later in the 19th century, it appeared that geometries without the parallel postulate (non-Euclidean geometries) can be developed without introducing any contradiction. The geometry that underlies general relativity is a famous application of non-Euclidean geometry.

Since the late 19th century, the scope of geometry has been greatly expanded, and the field has been split in many subfields that depend on the underlying methods—differential geometry, algebraic geometry, computational geometry, algebraic topology, discrete geometry (also known as combinatorial geometry), etc.—or on the properties of Euclidean spaces that are disregarded—projective geometry that consider only alignment of points but not distance and parallelism, affine geometry that omits the concept of angle and distance, finite geometry that omits continuity, and others. This enlargement of the scope of geometry led to a change of meaning of the word "space", which originally referred to the three-dimensional space of the physical world and its model provided by Euclidean geometry; presently a geometric space, or simply a space is a mathematical structure on which some geometry is defined.

History

A European and an Arab practicing geometry in the 15th century

The earliest recorded beginnings of geometry can be traced to ancient Mesopotamia and Egypt in the 2nd millennium BC. Early geometry was a collection of empirically discovered principles concerning lengths, angles, areas, and volumes, which were developed to meet some practical need in surveying, construction, astronomy, and various crafts. The earliest known texts on geometry are the Egyptian Rhind Papyrus (2000–1800 BC) and Moscow Papyrus (c. 1890 BC), and the Babylonian clay tablets, such as Plimpton 322 (1900 BC). For example, the Moscow Papyrus gives a formula for calculating the volume of a truncated pyramid, or frustum. Later clay tablets (350–50 BC) demonstrate that Babylonian astronomers implemented trapezoid procedures for computing Jupiter's position and motion within time-velocity space. These geometric procedures anticipated the Oxford Calculators, including the mean speed theorem, by 14 centuries. South of Egypt the ancient Nubians established a system of geometry including early versions of sun clocks.

In the 7th century BC, the Greek mathematician Thales of Miletus used geometry to solve problems such as calculating the height of pyramids and the distance of ships from the shore. He is credited with the first use of deductive reasoning applied to geometry, by deriving four corollaries to Thales's theorem. Pythagoras established the Pythagorean School, which is credited with the first proof of the Pythagorean theorem, though the statement of the theorem has a long history. Eudoxus (408–c. 355 BC) developed the method of exhaustion, which allowed the calculation of areas and volumes of curvilinear figures, as well as a theory of ratios that avoided the problem of incommensurable magnitudes, which enabled subsequent geometers to make significant advances. Around 300 BC, geometry was revolutionized by Euclid, whose Elements, widely considered the most successful and influential textbook of all time, introduced mathematical rigor through the axiomatic method and is the earliest example of the format still used in mathematics today, that of definition, axiom, theorem, and proof. Although most of the contents of the Elements were already known, Euclid arranged them into a single, coherent logical framework. The Elements was known to all educated people in the West until the middle of the 20th century and its contents are still taught in geometry classes today. Archimedes (c. 287–212 BC) of Syracuse, Italy used the method of exhaustion to calculate the area under the arc of a parabola with the summation of an infinite series, and gave remarkably accurate approximations of pi. He also studied the spiral bearing his name and obtained formulas for the volumes of surfaces of revolution.

Woman teaching geometry. Illustration at the beginning of a medieval translation of Euclid's Elements, (c. 1310).

Indian mathematicians also made many important contributions in geometry. The Shatapatha Brahmana (3rd century BC) contains rules for ritual geometric constructions that are similar to the Sulba Sutras. According to (Hayashi 2005, p. 363), the Śulba Sūtras contain "the earliest extant verbal expression of the Pythagorean Theorem in the world, although it had already been known to the Old Babylonians. They contain lists of Pythagorean triples, which are particular cases of Diophantine equations. In the Bakhshali manuscript, there are a handful of geometric problems (including problems about volumes of irregular solids). The Bakhshali manuscript also "employs a decimal place value system with a dot for zero." Aryabhata's Aryabhatiya (499) includes the computation of areas and volumes. Brahmagupta wrote his astronomical work Brāhmasphuṭasiddhānta in 628. Chapter 12, containing 66 Sanskrit verses, was divided into two sections: "basic operations" (including cube roots, fractions, ratio and proportion, and barter) and "practical mathematics" (including mixture, mathematical series, plane figures, stacking bricks, sawing of timber, and piling of grain). In the latter section, he stated his famous theorem on the diagonals of a cyclic quadrilateral. Chapter 12 also included a formula for the area of a cyclic quadrilateral (a generalization of Heron's formula), as well as a complete description of rational triangles (i.e. triangles with rational sides and rational areas).

In the Middle Ages, mathematics in medieval Islam contributed to the development of geometry, especially algebraic geometry. Al-Mahani (b. 853) conceived the idea of reducing geometrical problems such as duplicating the cube to problems in algebra. Thābit ibn Qurra (known as Thebit in Latin) (836–901) dealt with arithmetic operations applied to ratios of geometrical quantities, and contributed to the development of analytic geometry. Omar Khayyam (1048–1131) found geometric solutions to cubic equations. The theorems of Ibn al-Haytham (Alhazen), Omar Khayyam and Nasir al-Din al-Tusi on quadrilaterals, including the Lambert quadrilateral and Saccheri quadrilateral, were early results in hyperbolic geometry, and along with their alternative postulates, such as Playfair's axiom, these works had a considerable influence on the development of non-Euclidean geometry among later European geometers, including Vitello (c. 1230 – c. 1314), Gersonides (1288–1344), Alfonso, John Wallis, and Giovanni Girolamo Saccheri.

In the early 17th century, there were two important developments in geometry. The first was the creation of analytic geometry, or geometry with coordinates and equations, by René Descartes (1596–1650) and Pierre de Fermat (1601–1665). This was a necessary precursor to the development of calculus and a precise quantitative science of physics. The second geometric development of this period was the systematic study of projective geometry by Girard Desargues (1591–1661). Projective geometry studies properties of shapes which are unchanged under projections and sections, especially as they relate to artistic perspective.

Two developments in geometry in the 19th century changed the way it had been studied previously. These were the discovery of non-Euclidean geometries by Nikolai Ivanovich Lobachevsky, János Bolyai and Carl Friedrich Gauss and of the formulation of symmetry as the central consideration in the Erlangen programme of Felix Klein (which generalized the Euclidean and non-Euclidean geometries). Two of the master geometers of the time were Bernhard Riemann (1826–1866), working primarily with tools from mathematical analysis, and introducing the Riemann surface, and Henri Poincaré, the founder of algebraic topology and the geometric theory of dynamical systems. As a consequence of these major changes in the conception of geometry, the concept of "space" became something rich and varied, and the natural background for theories as different as complex analysis and classical mechanics.

Main concepts

The following are some of the most important concepts in geometry.

Axioms

An illustration of Euclid's parallel postulate

Euclid took an abstract approach to geometry in his Elements, one of the most influential books ever written. Euclid introduced certain axioms, or postulates, expressing primary or self-evident properties of points, lines, and planes. He proceeded to rigorously deduce other properties by mathematical reasoning. The characteristic feature of Euclid's approach to geometry was its rigor, and it has come to be known as axiomatic or synthetic geometry. At the start of the 19th century, the discovery of non-Euclidean geometries by Nikolai Ivanovich Lobachevsky (1792–1856), János Bolyai (1802–1860), Carl Friedrich Gauss (1777–1855) and others led to a revival of interest in this discipline, and in the 20th century, David Hilbert (1862–1943) employed axiomatic reasoning in an attempt to provide a modern foundation of geometry.

Objects

Points

Points are generally considered fundamental objects for building geometry. They may be defined by the properties that they must have, as in Euclid's definition as "that which has no part", or in synthetic geometry. In modern mathematics, they are generally defined as elements of a set called space, which is itself axiomatically defined.

With these modern definitions, every geometric shape is defined as a set of points; this is not the case in synthetic geometry, where a line is another fundamental object that is not viewed as the set of the points through which it passes.

However, there are modern geometries in which points are not primitive objects, or even without points. One of the oldest such geometries is Whitehead's point-free geometry, formulated by Alfred North Whitehead in 1919–1920.

Lines

Euclid described a line as "breadthless length" which "lies equally with respect to the points on itself". In modern mathematics, given the multitude of geometries, the concept of a line is closely tied to the way the geometry is described. For instance, in analytic geometry, a line in the plane is often defined as the set of points whose coordinates satisfy a given linear equation, but in a more abstract setting, such as incidence geometry, a line may be an independent object, distinct from the set of points which lie on it. In differential geometry, a geodesic is a generalization of the notion of a line to curved spaces.

Planes

In Euclidean geometry a plane is a flat, two-dimensional surface that extends infinitely; the definitions for other types of geometries are generalizations of that. Planes are used in many areas of geometry. For instance, planes can be studied as a topological surface without reference to distances or angles; it can be studied as an affine space, where collinearity and ratios can be studied but not distances; it can be studied as the complex plane using techniques of complex analysis; and so on.

Angles

Euclid defines a plane angle as the inclination to each other, in a plane, of two lines which meet each other, and do not lie straight with respect to each other. In modern terms, an angle is the figure formed by two rays, called the sides of the angle, sharing a common endpoint, called the vertex of the angle.

Acute (a), obtuse (b), and straight (c) angles. The acute and obtuse angles are also known as oblique angles.

In Euclidean geometry, angles are used to study polygons and triangles, as well as forming an object of study in their own right. The study of the angles of a triangle or of angles in a unit circle forms the basis of trigonometry.

In differential geometry and calculus, the angles between plane curves or space curves or surfaces can be calculated using the derivative.

Curves

A curve is a 1-dimensional object that may be straight (like a line) or not; curves in 2-dimensional space are called plane curves and those in 3-dimensional space are called space curves.

In topology, a curve is defined by a function from an interval of the real numbers to another space. In differential geometry, the same definition is used, but the defining function is required to be differentiable  Algebraic geometry studies algebraic curves, which are defined as algebraic varieties of dimension one.

Surfaces

A sphere is a surface that can be defined parametrically (by x = r sin θ cos φ, y = r sin θ sin φ, z = r cos θ) or implicitly (by x2 + y2 + z2r2 = 0.)

A surface is a two-dimensional object, such as a sphere or paraboloid. In differential geometry and topology, surfaces are described by two-dimensional 'patches' (or neighborhoods) that are assembled by diffeomorphisms or homeomorphisms, respectively. In algebraic geometry, surfaces are described by polynomial equations.

Solids

In Euclidean space, a ball is the volume bounded by a sphere

A solid is a three-dimensional object bounded by a closed surface; for example, a ball is the volume bounded by a sphere.

Manifolds

A manifold is a generalization of the concepts of curve and surface. In topology, a manifold is a topological space where every point has a neighborhood that is homeomorphic to Euclidean space. In differential geometry, a differentiable manifold is a space where each neighborhood is diffeomorphic to Euclidean space.

Manifolds are used extensively in physics, including in general relativity and string theory.

Measures: length, area, and volume

Length, area, and volume describe the size or extent of an object in one dimension, two dimension, and three dimensions respectively.

In Euclidean geometry and analytic geometry, the length of a line segment can often be calculated by the Pythagorean theorem.

Area and volume can be defined as fundamental quantities separate from length, or they can be described and calculated in terms of lengths in a plane or 3-dimensional space. Mathematicians have found many explicit formulas for area and formulas for volume of various geometric objects. In calculus, area and volume can be defined in terms of integrals, such as the Riemann integral or the Lebesgue integral.

Other geometrical measures include the angular measure, curvature, compactness measures.

Metrics and measures

Visual checking of the Pythagorean theorem for the (3, 4, 5) triangle as in the Zhoubi Suanjing 500–200 BC. The Pythagorean theorem is a consequence of the Euclidean metric.

The concept of length or distance can be generalized, leading to the idea of metrics. For instance, the Euclidean metric measures the distance between points in the Euclidean plane, while the hyperbolic metric measures the distance in the hyperbolic plane. Other important examples of metrics include the Lorentz metric of special relativity and the semi-Riemannian metrics of general relativity.

In a different direction, the concepts of length, area and volume are extended by measure theory, which studies methods of assigning a size or measure to sets, where the measures follow rules similar to those of classical area and volume.

Congruence and similarity

Congruence and similarity are concepts that describe when two shapes have similar characteristics. In Euclidean geometry, similarity is used to describe objects that have the same shape, while congruence is used to describe objects that are the same in both size and shape. Hilbert, in his work on creating a more rigorous foundation for geometry, treated congruence as an undefined term whose properties are defined by axioms.

Congruence and similarity are generalized in transformation geometry, which studies the properties of geometric objects that are preserved by different kinds of transformations.

Compass and straightedge constructions

Classical geometers paid special attention to constructing geometric objects that had been described in some other way. Classically, the only instruments used in most geometric constructions are the compass and straightedge. Also, every construction had to be complete in a finite number of steps. However, some problems turned out to be difficult or impossible to solve by these means alone, and ingenious constructions using neusis, parabolas and other curves, or mechanical devices, were found.

Rotation and orientation

The geometrical concepts of rotation and orientation define part of the placement of objects embedded in the plane or in space.

Dimension

The Koch snowflake, with fractal dimension=log4/log3 and topological dimension=1

Where the traditional geometry allowed dimensions 1 (a line), 2 (a plane) and 3 (our ambient world conceived of as three-dimensional space), mathematicians and physicists have used higher dimensions for nearly two centuries. One example of a mathematical use for higher dimensions is the configuration space of a physical system, which has a dimension equal to the system's degrees of freedom. For instance, the configuration of a screw can be described by five coordinates.

In general topology, the concept of dimension has been extended from natural numbers, to infinite dimension (Hilbert spaces, for example) and positive real numbers (in fractal geometry). In algebraic geometry, the dimension of an algebraic variety has received a number of apparently different definitions, which are all equivalent in the most common cases.

Symmetry

A tiling of the hyperbolic plane

The theme of symmetry in geometry is nearly as old as the science of geometry itself. Symmetric shapes such as the circle, regular polygons and platonic solids held deep significance for many ancient philosophers and were investigated in detail before the time of Euclid. Symmetric patterns occur in nature and were artistically rendered in a multitude of forms, including the graphics of Leonardo da Vinci, M. C. Escher, and others. In the second half of the 19th century, the relationship between symmetry and geometry came under intense scrutiny. Felix Klein's Erlangen program proclaimed that, in a very precise sense, symmetry, expressed via the notion of a transformation group, determines what geometry is. Symmetry in classical Euclidean geometry is represented by congruences and rigid motions, whereas in projective geometry an analogous role is played by collineations, geometric transformations that take straight lines into straight lines. However it was in the new geometries of Bolyai and Lobachevsky, Riemann, Clifford and Klein, and Sophus Lie that Klein's idea to 'define a geometry via its symmetry group' found its inspiration. Both discrete and continuous symmetries play prominent roles in geometry, the former in topology and geometric group theory, the latter in Lie theory and Riemannian geometry.

A different type of symmetry is the principle of duality in projective geometry, among other fields. This meta-phenomenon can roughly be described as follows: in any theorem, exchange point with plane, join with meet, lies in with contains, and the result is an equally true theorem. A similar and closely related form of duality exists between a vector space and its dual space.

Contemporary geometry

Euclidean geometry

Euclidean geometry is geometry in its classical sense. As it models the space of the physical world, it is used in many scientific areas, such as mechanics, astronomy, crystallography, and many technical fields, such as engineering, architecture, geodesy, aerodynamics, and navigation. The mandatory educational curriculum of the majority of nations includes the study of Euclidean concepts such as points, lines, planes, angles, triangles, congruence, similarity, solid figures, circles, and analytic geometry.

Euclidean vectors

Euclidean vectors are used for a myriad of applications in physics and engineering, such as position, displacement, deformation, velocity, acceleration, force, etc.

Differential geometry

Differential geometry uses tools from calculus to study problems involving curvature.

Differential geometry uses techniques of calculus and linear algebra to study problems in geometry. It has applications in physics, econometrics, and bioinformatics, among others.

In particular, differential geometry is of importance to mathematical physics due to Albert Einstein's general relativity postulation that the universe is curved. Differential geometry can either be intrinsic (meaning that the spaces it considers are smooth manifolds whose geometric structure is governed by a Riemannian metric, which determines how distances are measured near each point) or extrinsic (where the object under study is a part of some ambient flat Euclidean space).

Non-Euclidean geometry

Behavior of lines with a common perpendicular in each of the three types of geometry
In mathematics, non-Euclidean geometry consists of two geometries based on axioms closely related to those that specify Euclidean geometry. As Euclidean geometry lies at the intersection of metric geometry and affine geometry, non-Euclidean geometry arises by either replacing the parallel postulate with an alternative, or relaxing the metric requirement. In the former case, one obtains hyperbolic geometry and elliptic geometry, the traditional non-Euclidean geometries. When the metric requirement is relaxed, then there are affine planes associated with the planar algebras, which give rise to kinematic geometries that have also been called non-Euclidean geometry.

Topology

A thickening of the trefoil knot

Topology is the field concerned with the properties of continuous mappings, and can be considered a generalization of Euclidean geometry. In practice, topology often means dealing with large-scale properties of spaces, such as connectedness and compactness.

The field of topology, which saw massive development in the 20th century, is in a technical sense a type of transformation geometry, in which transformations are homeomorphisms. This has often been expressed in the form of the saying 'topology is rubber-sheet geometry'. Subfields of topology include geometric topology, differential topology, algebraic topology and general topology.

Algebraic geometry

Quintic Calabi–Yau threefold

Algebraic geometry is fundamentally the study by means of algebraic methods of some geometrical shapes, called algebraic sets, and defined as common zeros of multivariate polynomials. Algebraic geometry became an autonomous subfield of geometry c. 1900, with a theorem called Hilbert's Nullstellensatz that establishes a strong correspondence between algebraic sets and ideals of polynomial rings. This led to a parallel development of algebraic geometry, and its algebraic counterpart, called commutative algebra. From the late 1950s through the mid-1970s algebraic geometry had undergone major foundational development, with the introduction by Alexander Grothendieck of scheme theory, which allows using topological methods, including cohomology theories in a purely algebraic context. Scheme theory allowed to solve many difficult problems not only in geometry, but also in number theory. Wiles' proof of Fermat's Last Theorem is a famous example of a long-standing problem of number theory whose solution uses scheme theory and its extensions such as stack theory. One of seven Millennium Prize problems, the Hodge conjecture, is a question in algebraic geometry.

Algebraic geometry has applications in many areas, including cryptography and string theory.

Complex geometry

Complex geometry studies the nature of geometric structures modelled on, or arising out of, the complex plane. Complex geometry lies at the intersection of differential geometry, algebraic geometry, and analysis of several complex variables, and has found applications to string theory and mirror symmetry.

Complex geometry first appeared as a distinct area of study in the work of Bernhard Riemann in his study of Riemann surfaces. Work in the spirit of Riemann was carried out by the Italian school of algebraic geometry in the early 1900s. Contemporary treatment of complex geometry began with the work of Jean-Pierre Serre, who introduced the concept of sheaves to the subject, and illuminated the relations between complex geometry and algebraic geometry. The primary objects of study in complex geometry are complex manifolds, complex algebraic varieties, and complex analytic varieties, and holomorphic vector bundles and coherent sheaves over these spaces. Special examples of spaces studied in complex geometry include Riemann surfaces, and Calabi–Yau manifolds, and these spaces find uses in string theory. In particular, worldsheets of strings are modelled by Riemann surfaces, and superstring theory predicts that the extra 6 dimensions of 10 dimensional spacetime may be modelled by Calabi–Yau manifolds.

Discrete geometry

Discrete geometry includes the study of various sphere packings.

Discrete geometry is a subject that has close connections with convex geometry. It is concerned mainly with questions of relative position of simple geometric objects, such as points, lines and circles. Examples include the study of sphere packings, triangulations, the Kneser-Poulsen conjecture, etc. It shares many methods and principles with combinatorics.

Computational geometry

Computational geometry deals with algorithms and their implementations for manipulating geometrical objects. Important problems historically have included the travelling salesman problem, minimum spanning trees, hidden-line removal, and linear programming.

Although being a young area of geometry, it has many applications in computer vision, image processing, computer-aided design, medical imaging, etc.

Geometric group theory

The Cayley graph of the free group on two generators a and b

Geometric group theory uses large-scale geometric techniques to study finitely generated groups. It is closely connected to low-dimensional topology, such as in Grigori Perelman's proof of the Geometrization conjecture, which included the proof of the Poincaré conjecture, a Millennium Prize Problem.

Geometric group theory often revolves around the Cayley graph, which is a geometric representation of a group. Other important topics include quasi-isometries, Gromov-hyperbolic groups, and right angled Artin groups.

Convex geometry

Convex geometry investigates convex shapes in the Euclidean space and its more abstract analogues, often using techniques of real analysis and discrete mathematics. It has close connections to convex analysis, optimization and functional analysis and important applications in number theory.

Convex geometry dates back to antiquity. Archimedes gave the first known precise definition of convexity. The isoperimetric problem, a recurring concept in convex geometry, was studied by the Greeks as well, including Zenodorus. Archimedes, Plato, Euclid, and later Kepler and Coxeter all studied convex polytopes and their properties. From the 19th century on, mathematicians have studied other areas of convex mathematics, including higher-dimensional polytopes, volume and surface area of convex bodies, Gaussian curvature, algorithms, tilings and lattices.

Applications

Geometry has found applications in many fields, some of which are described below.

Art

Bou Inania Madrasa, Fes, Morocco, zellige mosaic tiles forming elaborate geometric tessellations

Mathematics and art are related in a variety of ways. For instance, the theory of perspective showed that there is more to geometry than just the metric properties of figures: perspective is the origin of projective geometry.

Artists have long used concepts of proportion in design. Vitruvius developed a complicated theory of ideal proportions for the human figure. These concepts have been used and adapted by artists from Michelangelo to modern comic book artists.

The golden ratio is a particular proportion that has had a controversial role in art. Often claimed to be the most aesthetically pleasing ratio of lengths, it is frequently stated to be incorporated into famous works of art, though the most reliable and unambiguous examples were made deliberately by artists aware of this legend.

Tilings, or tessellations, have been used in art throughout history. Islamic art makes frequent use of tessellations, as did the art of M. C. Escher. Escher's work also made use of hyperbolic geometry.

Cézanne advanced the theory that all images can be built up from the sphere, the cone, and the cylinder. This is still used in art theory today, although the exact list of shapes varies from author to author.

Architecture

Geometry has many applications in architecture. In fact, it has been said that geometry lies at the core of architectural design. Applications of geometry to architecture include the use of projective geometry to create forced perspective, the use of conic sections in constructing domes and similar objects, the use of tessellations, and the use of symmetry.

Physics

The field of astronomy, especially as it relates to mapping the positions of stars and planets on the celestial sphere and describing the relationship between movements of celestial bodies, have served as an important source of geometric problems throughout history.

Riemannian geometry and pseudo-Riemannian geometry are used in general relativity. String theory makes use of several variants of geometry, as does quantum information theory.

Other fields of mathematics

The Pythagoreans discovered that the sides of a triangle could have incommensurable lengths.

Calculus was strongly influenced by geometry. For instance, the introduction of coordinates by René Descartes and the concurrent developments of algebra marked a new stage for geometry, since geometric figures such as plane curves could now be represented analytically in the form of functions and equations. This played a key role in the emergence of infinitesimal calculus in the 17th century. Analytic geometry continues to be a mainstay of pre-calculus and calculus curriculum.

Another important area of application is number theory. In ancient Greece the Pythagoreans considered the role of numbers in geometry. However, the discovery of incommensurable lengths contradicted their philosophical views. Since the 19th century, geometry has been used for solving problems in number theory, for example through the geometry of numbers or, more recently, scheme theory, which is used in Wiles's proof of Fermat's Last Theorem.

Critique of the Schopenhauerian philosophy

From Wikipedia, the free encyclopedia
https://en.wikipedia.org/wiki/Critique_of_the_Schopenhauerian_philosophy

Schopenhauer in 1852, 64 years old
 
Mainländer c. 1867, 26 years old

Critique of the Schopenhaurian philosophy is a literary work by Philipp Mainländer appended to Die Philosophie der Erlösung (The Philosophy of Redemption or The Philosophy of Salvation), offering a criticism of the philosophy of Arthur Schopenhauer. Mainländer saw the purification of Schopenhauer's philosophy as the primary task of his life. The criticism had an important impact on Nietzsche's philosophical development.

General overview

The Critique of the Schopenhauerian philosophy is generally seen as offering a position closer to realism than the idealism of Kant and Schopenhauer. Mainländer aims to free the philosophy of Schopenhauer from its metaphysical tendencies.

It is the longest criticism of Schopenhauer's work, and it earned him the praise of Frauenstädt, "apostle primarie" of Schopenhauer, Max Seiling and Frederick C. Beiser for being one of the most talented followers of Schopenhauer.

Epistemology

Background of the critical philosophy

Locke had referred all philosophical research to the domain of experience. He argued that the mind is empty at birth, and that all knowledge stems from experience. This was an important step in philosophy, yet, by accepting this important problems arise. The most famous challenge came from Hume, namely, if all knowledge is derived from experience we have no right to claim things are caused, we can only perceive that they follow after each other. Berkeley also noted that all that is given to us are subjective sensations, and Thomas Reid expounded this further by demonstrating that the mere sensations of the senses bear no resemblance to objective qualities, such as extension, figure, and number.

Kant determined that although Locke was right to assert that all knowledge begins with experience, it does not follow that all knowledge arises from experience. Cognition has a priori structures (the categories and the form of intuition) that structure experience, that is, are constitutive of experience as ordered and intelligible. (Kant notes that without the categories experience would be less than a great roar of sound). These forms that lie in us are causality (amongst other categories), space and time.

G.E. Schulze had argued that Kant's proof that causality must be an inborn concept is invalid. Schopenhauer and Mainländer agreed with Schulze that the attempt of Kant was totally unsuccessful.

Causality

It was therefore up to those who were loyal to Kant’s project to secure the validity of causality. As Hume’s skepticism is based on the assumption that causality is a concept drawn from successive external representations, Schopenhauer started to investigate how we actually come to know external representations. After all, all that is given to me are subjective sensations, sense data that go not beyond my skin. So how is it possible to perceive something beyond my skin, outside of me? Mainländer praises this as an exceptional sign of prudence.

The senses merely deliver the data, which is processed by the brain into the objective world by means of the understanding, which conceives every change in a sense organ as the effect of an external cause, and seeks the cause in space. Hereby, for the first time it is shown how the visible world arises from sense data. Schopenhauer called this comprehension of a change in the sense organ having a cause in space, the causal law (German: Kausalitätsgesetz).

Schopenhauer deemed that he had thereby disproven Hume’s skepticism, since representations presuppose the causal law. Causality is consequently not a concept drawn from successive representations, but representations presuppose knowledge of causality.

The causal law does not cover causality in general.

This reasoning is too hastily made (a subreption). Schopenhauer has indeed shown that the causal law is needed for objective perception and consequently lies a priori in us, but not that causality in general must lie a priori in us. The causal law merely says: every change in my sense organ is the effect of a cause. It is a one-sided relation (the outer world affects me) of the subject that says nothing about objects affecting each other. The causal law does not cover causality in general.

In order to do anything else than searching the cause of an effect, we need another mental faculty. Reason reflects and recognizes that I am not a privileged subject but an object amongst objects, so with help of experience it subjects all appearances to the general law: wherever in nature a change takes place, it is the effect of a cause, which preceded it in time. Causality is therefore given a posteriori and not a priori, though it has an aprioristic ground.

Transcendental Analytic

According to Schopenhauer the only mental faculty needed for the creation of the outer world is the understanding. The reason merely draws concepts from the objective world, reflects on it, but in no way helps to construct it. Kant however, maintained that there are inborn concepts, categories, and that they are needed to make from “the chaos of appearances”, the manifold given in perception, an objectively valid connection called nature.

Schopenhauer has shown that only due to the understanding we can know external objects, by moving the sensation in the sense organ outwards. This is its only function. So the understanding gives us many external representations, though it does not know how they are connected amongst each other. Schopenhauer illegitimately claimed that causality in general is the function of the understanding. Consequently, his explanation that the understanding can know that different partial-representations come from one object does not hold. For example, if I stand before a lamppost and first behold its lower part, and then move my eyes to its top; then my understanding has first moved the sensation in my eye outwards to see its lower part, and has, after that, done the same with the top; but it does not deduce that the sensations come from one object, since its only function is moving the sensation outwards. It has merely given me partial-representations.

This observation forms, in the Critique of Pure Reason, the heart of the Transcendental Analytic. Kant writes:

It was assumed, that the senses deliver not only impressions, but also conjoin them and provide images of objects. But for this to happen something else, besides the receptivity of impressions, is needed, namely a function for the synthesis of these impressions. 

Since every appearance contains a manifold, and different perceptions are found in the mind scattered and singly, a conjoinment of them is needed, which they cannot have in the senses themselves.

For the unity of a manifold to become an objective perception (like something in the representation of space,) first the accession of the manifold and then the unification of this manifold are necessary, an act which I call the synthesis of apprehension.

The combination (conjunctio) of a manifold can never come to us through the senses.

This synthesis forms the main topic of the Analytic, and it is very important to never lose sight of the concerned issue, that partial-representations delivered by the senses need a mental faculty before appearing as connected in the mind:

The synthesis is a blind but indispensable function of the soul, without which we should have no cognition whatever, but of the working of which we are seldom even conscious.[10]: A78, B103 

And holding onto this important observation, it makes clear that the categories are a secondary issue in the Analytic. The categories are necessary as fixed rules for the subject in its conjoinment of partial-representations: otherwise the subject would arbitrarily conjoin whatever appears, and no sustained object could be perceived.

In other words, Kant needed the categories because there is (according to his teaching) no coercion coming from the reality-in-itself to perceive this or that object, to conjoin the lower and upper part of the lamppost into one object. So the coercion to see sustained objects (and a world with natural laws) comes according to Kant solely from the subject. This "absurd" reasoning which Kant had to make, is not needed when we comprehend the activity which brings forth homogenous partial-representations as coming from the same thing-in-itself. The activity of a tree-in-itself would, when we behold its lower part, provide us the sensation that leads to the partial-representation of its lower part, and when we behold the upper part the corresponding partial-representation. Judgement-power can determine that the activity originates from one unity (the tree-in-itself) and reason conjoins them. This way, the coercion stems from reality-in-itself instead of the subject.

Space and time

Kant had argued that space and time lie as infinite magnitudes inborn in us, and are forms of our sensibility. Schopenhauer accepted this characterization of space and time, as did many neo-Kantians: it was frequently praised as one of the greatest events in philosophy. The theory of relativity eroded the value of the Aesthetic, as it proved to be incompatible with relativity, famously causing neo-Kantians to write A Hundred Authors against Einstein.

A few critical followers of Kant were skeptical from the beginning, Afrikan Spir and Mainländer noted, independently from each other, that the Aesthetic is self-contradicting, and Mainländer maintains that Kant was conscious of this, as Kant redefines the nature of space and time in the Analytic.

In the Analytic Kant makes a distinction between form of perception (German: Anschauung) and pure perception. Time and mathematical space are no longer forms of perception, but are the synthesis of a manifold which sensibility offers in its original receptivity. Kant is silent about what this manifold of the original receptivity of sensibility is. The investigation of Mainländer gives as result that these inborn forms are, instead, point-space and the present (point-time). Time and mathematical spaces are subjective creations a posteriori.

Mainländer saw it as the greatest merit of Kant to show that space and time are subjective. However, space and time do not readily lie in us, to bring forth properties such as extension and motion, but are subjective preconditions to cognize them.

Extension does not depend upon space. Because Kant and Schopenhauer automatically assumed that extension and space are equivalent concepts, by showing that space exists only for a perceiver, they had to deny that extension exists independently from a perceiver. Mainländer thus distinguished between proper length and length as it is perceived.

Here, Mainländer not only circumvented the contradiction with relativity of Kant-Schopenhauer, but also came to a result that surprisingly complies with special relativity, which teaches us that length as it is perceived is subjective: it is dependent on the velocity of the observer and the proper length of the object that is perceived.

where

L0 is the proper length,
L is the length observed by an observer in relative motion with respect to the object,
v is the relative velocity between the observer and the moving object,
c is the speed of light.

The separation of space as it is observed and proper length seemed to have no meaning before the discovery of relativity: in a time with only Newtonian mechanics it seemed to many as a superfluous distinction. As a consequence, not realizing why this would be of any importance, contemporaries of Mainländer accused his philosophy of simply being realism contrary to his own claims. (Plümacher, Von Hartmann)

Time is likewise subjective though nothing without its real underlay. It is its “subjective measuring rod.”

Ontology

According to Mainländer, Schopenhauer found the only path that leads to the thing-in-itself.

If we refer the concept of force to that of will, we have in fact referred the less known to what is infinitely better known; indeed, to the one thing that is really immediately and fully known to us, and have very greatly extended our knowledge. If, on the contrary, we subsume the concept of will under that of force, as has hitherto always been done, we renounce the only immediate knowledge which we have of the inner nature of the world, for we allow it to disappear in a concept which is abstracted from the phenomenal, and with which we can therefore never go beyond the phenomenal.

Yet, though we know the will without the forms of space and causality, under the influence of Kant's transcendental aesthetic, Schopenhauer deems that we know the will under the form of our inner sensibility, time, which implies that we know not the will as it is in itself. This would mean that we can never determine anything about the essence of the world, and Schopenhauer uses this result to continue with obscure metaphysics. Mainländer maintains that, since time is not a form of our inner sensibility, we can know the thing-in-itself completely and nakedly.

Aesthetics

Although Mainländer considers Schopenhauer's works on art to be brilliant and spirited, they are often based on pure metaphysics. Schopenhauer reintroduces Plato's theory of forms and calls Platonic Ideas the first and most universal form of objects without the subordinate forms of the phenomenon. Mainländer comments that this is a meaningless combination of words.

Head of Christ by Antonio da Correggio

Kant and Schopenhauer briefly discuss the sublime character, but only mention characteristics that explain not its essence. Just like how the feeling of the sublime stems from overcoming the fear of death in a situation where the individual normally would feel endangered, though it is merely self-deception, sublimity inheres the individual if it permanently has contempt of death.

Mainländer mentions three classes of sublime characters. To the first class belong those who still love life, but care no longer about their individual weal as they fight for a higher ideal (the freedom of a nation, social rights, emancipation), in a word, heroes. To the second class belong those who are convinced of the worthlessness of life, and this conviction has made them immune to all worldly affairs. Saints and wise philosophers such as Spinoza belong to this class. The third class belongs to those who are sublime in the highest degree: the ascetic human who returns to the world, without making any concession, only to free the world from suffering. That they gain thereby adulation during life and deification after death leaves them cold and indifferent. Buddha and Christ fill up this class.

Because the wise hero is the most sublime appearance in this world, the greatest geniuses have tried to portray it in art. Two exceptional works Mainländer highlights are Eschenbach’s Parzival and Corregio’s Head of Christ.

Ethics

Schopenhauer called Kant's distinction between the empirical and intelligible character "one of the most beautiful and most profound thought products of this great mind". It claims that although all appearances act in a determined manner, it is the subject who issued these laws of nature: they owe their existence and necessity to the subject. Therefore, as thing-in-itself, we must be free, though it is a transcendental freedom which we cannot comprehend. Mainländer argues that this distinction follows only because of errors in epistemology, since Kant and Schopenhauer believed that all coercion stems from the subject, instead of the things-in-themselves.

Schopenhauer used this transcendental freedom to legitimize the negation of motives, quietives, which finds its expression in asceticism. Hereby Schopenhauer shows that compassion is not the basis of morality, since saintliness is not motivated by compassion. A saint who is worried about his immortal soul and flees to deserts, is indeed no longer sensitive to worldly motives, but only because a stronger motive crushes them.

Metaphysics

As every aspect of Schopenhauer's metaphysics has been discussed throughout the critique, Mainländer ends instead with a selection of religious texts, that show that the essence of Schopenhauer’s philosophy, Christianity and Buddhism is one: the absolute truth.

Particle

From Wikipedia, the free encyclopedia
Arc welders need to protect themselves from welding sparks, which are heated metal particles that fly off the welding surface.

In the physical sciences, a particle (or corpuscule in older texts) is a small localized object which can be described by several physical or chemical properties, such as volume, density, or mass. They vary greatly in size or quantity, from subatomic particles like the electron, to microscopic particles like atoms and molecules, to macroscopic particles like powders and other granular materials. Particles can also be used to create scientific models of even larger objects depending on their density, such as humans moving in a crowd or celestial bodies in motion.

The term particle is rather general in meaning, and is refined as needed by various scientific fields. Anything that is composed of particles may be referred to as being particulate. However, the noun particulate is most frequently used to refer to pollutants in the Earth's atmosphere, which are a suspension of unconnected particles, rather than a connected particle aggregation.

Conceptual properties

Particles are often represented as dots. This figure could represent the movement of atoms in a gas, people in crowds or stars in the night sky.

The concept of particles is particularly useful when modelling nature, as the full treatment of many phenomena can be complex and also involve difficult computation. It can be used to make simplifying assumptions concerning the processes involved. Francis Sears and Mark Zemansky, in University Physics, give the example of calculating the landing location and speed of a baseball thrown in the air. They gradually strip the baseball of most of its properties, by first idealizing it as a rigid smooth sphere, then by neglecting rotation, buoyancy and friction, ultimately reducing the problem to the ballistics of a classical point particle. The treatment of large numbers of particles is the realm of statistical physics.

Size

Galaxies are so large that stars can be considered particles relative to them

The term "particle" is usually applied differently to three classes of sizes. The term macroscopic particle, usually refers to particles much larger than atoms and molecules. These are usually abstracted as point-like particles, even though they have volumes, shapes, structures, etc. Examples of macroscopic particles would include powder, dust, sand, pieces of debris during a car accident, or even objects as big as the stars of a galaxy.

Another type, microscopic particles usually refers to particles of sizes ranging from atoms to molecules, such as carbon dioxide, nanoparticles, and colloidal particles. These particles are studied in chemistry, as well as atomic and molecular physics. The smallest of particles are the subatomic particles, which refer to particles smaller than atoms. These would include particles such as the constituents of atoms – protons, neutrons, and electrons – as well as other types of particles which can only be produced in particle accelerators or cosmic rays. These particles are studied in particle physics.

Because of their extremely small size, the study of microscopic and subatomic particles falls in the realm of quantum mechanics. They will exhibit phenomena demonstrated in the particle in a box model, including wave–particle duality, and whether particles can be considered distinct or identical is an important question in many situations.

Composition

A proton is composed of three quarks.

Particles can also be classified according to composition. Composite particles refer to particles that have composition – that is particles which are made of other particles. For example, a carbon-14 atom is made of six protons, eight neutrons, and six electrons. By contrast, elementary particles (also called fundamental particles) refer to particles that are not made of other particles. According to our current understanding of the world, only a very small number of these exist, such as leptons, quarks, and gluons. However it is possible that some of these might turn up to be composite particles after all, and merely appear to be elementary for the moment. While composite particles can very often be considered point-like, elementary particles are truly punctual.

Stability

Both elementary (such as muons) and composite particles (such as uranium nuclei), are known to undergo particle decay. Those that do not are called stable particles, such as the electron or a helium-4 nucleus. The lifetime of stable particles can be either infinite or large enough to hinder attempts to observe such decays. In the latter case, those particles are called "observationally stable". In general, a particle decays from a high-energy state to a lower-energy state by emitting some form of radiation, such as the emission of photons.

N-body simulation

In computational physics, N-body simulations (also called N-particle simulations) are simulations of dynamical systems of particles under the influence of certain conditions, such as being subject to gravity. These simulations are very common in cosmology and computational fluid dynamics.

N refers to the number of particles considered. As simulations with higher N are more computationally intensive, systems with large numbers of actual particles will often be approximated to a smaller number of particles, and simulation algorithms need to be optimized through various methods.

Distribution of particles

Examples of a stable and of an unstable colloidal dispersion.

Colloidal particles are the components of a colloid. A colloid is a substance microscopically dispersed evenly throughout another substance. Such colloidal system can be solid, liquid, or gaseous; as well as continuous or dispersed. The dispersed-phase particles have a diameter of between approximately 5 and 200 nanometers. Soluble particles smaller than this will form a solution as opposed to a colloid. Colloidal systems (also called colloidal solutions or colloidal suspensions) are the subject of interface and colloid science. Suspended solids may be held in a liquid, while solid or liquid particles suspended in a gas together form an aerosol. Particles may also be suspended in the form of atmospheric particulate matter, which may constitute air pollution. Larger particles can similarly form marine debris or space debris. A conglomeration of discrete solid, macroscopic particles may be described as a granular material.

Inhalant

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