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Diagonal

In , a is a straight that connects two nonconsecutive vertices of a or , excluding the sides or edges of the figure. This concept is fundamental to understanding the internal structure of polygonal shapes, where diagonals divide the interior into triangles and facilitate calculations such as area determination for specific quadrilaterals like rhombi and kites. For an n-sided , the total number of diagonals is given by the \frac{n(n-3)}{2}, which accounts for the fact that each vertex connects to n-3 other non-adjacent vertices, avoiding double-counting. In linear algebra, the term "diagonal" also describes a square where all off-diagonal entries are zero, leaving only the (from the top-left to bottom-right) potentially nonzero. Diagonal matrices simplify computations, such as matrix powers and , because multiplying them involves only scaling by their diagonal elements, and they play a central role in processes that transform general matrices into easier-to-analyze forms. Beyond and , diagonals appear in through , a demonstrating the uncountability of the real numbers by constructing a number differing from each in an assumed countable list along its diagonal position. This technique has broader applications in logic and computability, including , highlighting the diagonal's role in foundational .

Basic Concepts

Definition

In , a refers to a straight that connects two non-adjacent vertices of a or . For in the , a diagonal joins vertices that do not share an , thereby lying entirely within the polygon's interior for cases. This distinguishes diagonals from sides, which connect adjacent vertices. In the context of polyhedra, diagonals are categorized into face diagonals and space diagonals. A face diagonal lies on one of the polyhedron's polygonal faces and connects non-adjacent vertices within that face, analogous to a two-dimensional diagonal. In contrast, a space diagonal connects two vertices that do not share a common face, passing through the interior of the polyhedron. These space diagonals highlight the three-dimensional structure, unlike face diagonals which remain planar.

Properties in Plane Geometry

In plane geometry, a diagonal is a line segment connecting two non-adjacent vertices of a , lying entirely within the of the figure. This distinguishes diagonals from sides, which connect adjacent vertices, and enables the decomposition of polygons into simpler triangular regions through . For instance, drawing all non-intersecting diagonals from one vertex divides an n-gon into n-2 triangles, facilitating proofs of properties like the sum of interior angles equaling (n-2)\pi radians. In , the simplest polygons with diagonals, each figure has exactly two diagonals that connect opposite and generally intersect at a single interior point unless the quadrilateral is degenerate. The properties of these diagonals vary by quadrilateral type. In a , the diagonals bisect each other, meaning they intersect at their midpoints, a consequence of the vector equality of opposite sides. Extending this, the diagonals of a are congruent in length and bisect each other, while in a , they are perpendicular and bisect the vertex angles. For a square, combining these traits, the diagonals are equal, perpendicular, and each bisects the angles at 45 degrees. Key theorems highlight the role of diagonals in relating geometric elements. Varignon's theorem states that connecting the midpoints of the sides of any forms a , whose sides are parallel to the diagonals of the original and half their lengths; this Varignon is a if the original diagonals are equal in length, and a if they are . For cyclic quadrilaterals inscribed in a , Ptolemy's theorem provides a multiplicative relation: the product of the lengths of the diagonals equals the sum of the products of the lengths of the opposite sides, expressed as AC \cdot BD = AB \cdot CD + AD \cdot BC, where AB, BC, CD, DA are the sides and AC, BD the diagonals. This theorem, attributed to the ancient mathematician , underscores the interplay between diagonals and cyclic properties in plane figures. Diagonals also influence angle and area measures. In a , one diagonal is the of and bisects the other, while both are . The area of a can be computed using the diagonals and the angle \theta between them via \frac{1}{2} d_1 d_2 \sin \theta, applicable to any convex where the diagonals intersect. These properties extend conceptually to higher polygons, where diagonals may intersect to form additional vertices and edges, but in plane geometry, they fundamentally aid in classifying and analyzing polygonal structures.

In Polygons

Number of Diagonals

The number of diagonals in a with n vertices (or sides) is given by the formula \frac{n(n-3)}{2}. This expression arises because the total number of line segments connecting any two vertices is the combination \binom{n}{2} = \frac{n(n-1)}{2}, which includes both the n sides of the and the diagonals; subtracting the sides yields the diagonals: \frac{n(n-1)}{2} - n = \frac{n(n-3)}{2}. This formula applies specifically to simple polygons, where no three diagonals intersect at a single interior point, ensuring all diagonals are distinct and lie within the . For non- polygons, the count remains the same in terms of connections between vertices, but some diagonals may lie outside the . The derivation assumes vertices are in position, as is standard in basic . To illustrate, consider small polygons:
PolygonnNumber of Diagonals
30
42
55
69
These values follow directly from substituting into the formula, highlighting how the number grows quadratically with n, reflecting the increasing connectivity among vertices.

Regions and Intersections

In a with n \geq 4 vertices, the diagonals intersect exclusively in the interior, provided the polygon is in where no three diagonals meet at a single interior point. Each such arises from the crossing of two diagonals that connect four distinct vertices, forming a whose diagonals intersect at one point. Consequently, the total number of interior intersection points is \dbinom{n}{4}, as every set of four vertices determines exactly one such crossing. These intersection points, combined with the polygon's n vertices and its \frac{n(n-3)}{2} diagonals, subdivide the interior into multiple regions. Applying for planar graphs (V - E + F = 2, where V is vertices including intersections, E is edges including diagonal segments, and F is faces including the exterior), or through direct combinatorial , the number of interior regions r(n) is given by r(n) = \dbinom{n}{4} + \dbinom{n-1}{2}. This can also be expressed in expanded form as r(n) = \frac{n^4 - 6n^3 + 23n^2 - 42n + 24}{24}. The formula accounts for the initial polygonal face, the additions from diagonals and their segments, and the splits at intersections. For small values of n, the results illustrate the growth: a (n=4) has \dbinom{4}{4} = [1](/page/1) intersection and r(4) = 4 regions; a (n=5) has 5 intersections and r(5) = 11 regions; a (n=6) has 15 intersections and r(6) = 25 regions. These configurations maximize the number of regions under the no-three-concurrent assumption, emphasizing the combinatorial complexity introduced by diagonal crossings. If the polygon is or otherwise positioned such that multiple diagonals concur at interior points, the number of intersections decreases and the regions are fewer than in the general case, as shared points reduce the splitting effect. For example, in a , three long diagonals intersect at the center, yielding 24 regions rather than 25, though adjusted counts depend on the specific concurrencies. Such cases highlight the role of geometric constraints in altering the topological division.

Diagonals in Regular Polygons

In a regular n-gon inscribed in a circle of circumradius R, the diagonals connect non-adjacent vertices and subtend central angles that are multiples of $2\pi/n. The length of a diagonal spanning k vertices (where $2 \leq k \leq \lfloor n/2 \rfloor) is d_k = 2R \sin\left(\frac{k\pi}{n}\right). This formula arises from the chord length in a circle, where the central angle is \theta = 2\pi k / n, and the chord length is $2R \sin(\theta/2). If expressed in terms of the side length s = 2R \sin(\pi/n), the diagonal length becomes d_k = s \frac{\sin(k\pi/n)}{\sin(\pi/n)}. Due to rotational symmetry, there are \lfloor n/2 \rfloor - 1 distinct diagonal lengths, corresponding to the unique values of k excluding sides and diameters (when n is even). A prominent example occurs in the regular (n=5), where all diagonals are equal in and form a when connected. For a side of , each diagonal has \phi = \frac{[1](/page/1) + \sqrt{5}}{2}, the , satisfying \phi^2 = \phi + [1](/page/1). This ratio emerges from solving the of intersecting diagonals, as the diagonal d satisfies d = [1](/page/1) + 2 \cdot \frac{[1](/page/1)}{d} by considering isosceles triangles formed within the . In the regular hexagon (n=6), there are two distinct diagonal s: the shorter ones (spanning two vertices) measure s\sqrt{3}, and the longer ones (spanning three vertices) are diameters of $2s, all intersecting at . The intersections of diagonals in a regular n-gon exhibit rotational and reflectional , with each interior crossing typically involving exactly two diagonals, except in cases of higher concurrency (e.g., at for even n). Every set of four vertices determines a unique intersection point inside the , but symmetries reduce the total count. The number of such interior intersection points is given by the formula I(n) = \binom{n}{4} + \frac{n}{24} \left( \binom{m}{2} (m^2 + 5) - 3(-1)^m \right), where m = n \mod 24, adjusted as a based on n modulo 24; this counts points with multiplicity for concurrent diagonals. In the regular , each pair of diagonals intersects at a single point, dividing the into 11 regions, with each intersection segment ratio equal to the \phi : 1 : \phi. For larger n, such as the , intersections form complex symmetric patterns without triple points except at vertices.

In Polyhedra

Face Diagonals

In , a face diagonal of a is a connecting two non-adjacent vertices that lie on the same polygonal face, distinguishing it from edges and diagonals that pass through the interior. Unlike diagonals, which connect vertices on different faces, face diagonals remain entirely on the surface of the . The total number of face diagonals in a is determined by summing the diagonals across all its faces, where each face, being an n-gon, contributes \frac{n(n-3)}{2} diagonals. For example, a with six square faces (n=4) has $6 \times \frac{4(4-3)}{2} = 12 face diagonals, with two per face. In a square , the square base contributes 2 diagonals, while the four triangular faces (n=3) contribute none, yielding a total of 2 face diagonals. This approach highlights how face diagonals depend on the 's facial structure rather than its overall volume. Face diagonals play a key role in measuring surface distances and verifying polyhedral properties, such as in rectangular prisms where the lengths are \sqrt{l^2 + w^2}, \sqrt{l^2 + h^2}, and \sqrt{w^2 + h^2} for dimensions l, w, and h, with each type appearing on two opposite faces. In regular polyhedra like the , face diagonals on pentagonal faces follow the , \phi = \frac{1 + \sqrt{5}}{2}, scaled by the edge length, underscoring their geometric harmony.

Space Diagonals

In a , a space diagonal (also known as a body diagonal or interior diagonal) is a that connects two vertices not lying on the same face, passing through the interior of the . Unlike face diagonals, which lie entirely on one of the polyhedron's faces, space diagonals link vertices from distinct faces and do not coincide with any edges. This distinguishes them from the edges of the , which connect adjacent vertices. The is the only convex without space diagonals, as all pairs of vertices are either connected by an edge or lie on the same triangular face. The number of space diagonals in a polyhedron can be calculated by first determining the total number of line segments connecting any two vertices, which is the combination \binom{v}{2} = \frac{v(v-1)}{2} where v is the number of vertices, then subtracting the number of edges e and the total number of face diagonals. The number of face diagonals is the sum over all faces of \frac{n_f(n_f - 3)}{2}, where n_f is the number of sides of the f-th face. Thus, the formula for the number of space diagonals d_s is: d_s = \frac{v(v-1)}{2} - e - \sum_f \frac{n_f(n_f - 3)}{2}. This approach accounts for all possible connections while excluding surface elements. Using Euler's formula v - e + f = 2 for convex polyhedra, the total number of diagonals (face plus space) simplifies to \frac{v(v-3)}{2} + 2 - f, but space diagonals require the additional subtraction of face diagonals. For the Platonic solids, the numbers of space diagonals vary due to their symmetry and face structures, as shown in the table below. All faces are regular polygons, and triangular faces contribute no diagonals.
Platonic SolidVertices (v)Edges (e)Faces (f)Face DiagonalsSpace Diagonals
464 (triangles)00
8126 (squares)124
6128 (triangles)03
203012 (pentagons)60100
123020 (triangles)036
These counts are derived from the general formula applied to the known parameters of each solid. In a rectangular parallelepiped (or cuboid) with side lengths a, b, and c, each of the four space diagonals has length \sqrt{a^2 + b^2 + c^2}, obtained by applying the Pythagorean theorem in three dimensions: first finding the face diagonal on the base (\sqrt{a^2 + b^2}), then extending to the height (\sqrt{(\sqrt{a^2 + b^2})^2 + c^2}). For a cube with side length a, this simplifies to a\sqrt{3}. In more general regular polyhedra like the dodecahedron or icosahedron, space diagonals come in multiple lengths due to varying distances between non-adjacent vertices, related to the golden ratio \phi = \frac{1 + \sqrt{5}}{2} in their geometry.

In Higher Dimensions

In Simplices

In an n-dimensional , defined as the of n+1 affinely independent points, the 1-skeleton is the Kn+1 on its vertices, meaning every pair of distinct vertices is joined by an . As a result, there are no diagonals, since diagonals in a are line segments connecting non-adjacent vertices. This distinguishes simplices from other polytopes, such as hypercubes, where non-adjacent vertices exist and form various classes of diagonals. The absence of diagonals implies that any triangulation or subdivision of a simplex requires no additional internal connections between vertices; its structure is already fully edged. For instance, in a 3-simplex (tetrahedron), the six edges connect all four vertices directly, leaving no room for face or space diagonals on the boundary or interior. This property makes simplices fundamental building blocks in simplicial complexes, where higher-dimensional structures are assembled without introducing diagonals at the vertex level. In terms of combinatorial geometry, the number of diagonals in an n-simplex is zero. Seminal works on enumeration confirm this for simplices due to their maximal .

In Hypercubes

In an n-dimensional , also known as an n-cube, the vertices can be represented as all points with coordinates in {0,1}^n, forming a where edges connect vertices differing in exactly one coordinate. Diagonals are the line segments joining non-adjacent vertices, i.e., those differing in k coordinates where 2 ≤ k ≤ n; these are classified by the value of k, known as the type or of the diagonal. The total number of diagonals in an n-cube is given by \binom{2^n}{2} - n \cdot 2^{n-1} = 2^{n-1}(2^n - n - 1), where \binom{2^n}{2} counts all possible line segments between the 2^n vertices, and n \cdot 2^{n-1} subtracts the edges. For example, in the 3-cube (), there are 16 diagonals: 12 of type k=2 (face diagonals) and 4 of type k=3 (space diagonals). In the 4-cube (), the total rises to 88 diagonals: 48 of type k=2, 32 of type k=3, and 8 of type k=4. The number of diagonals of type k (differing in exactly k coordinates, or Hamming distance k) is \binom{n}{k} 2^{n-1}. This follows from selecting the k differing coordinates in \binom{n}{k} ways and, for each of the 2^n choices of starting vertex, flipping those k coordinates to reach the endpoint, then dividing by 2 for undirected segments. For k=2, these are the shortest diagonals, lying in the 2-dimensional square faces; there are \binom{n}{2} 2^{n-1} such diagonals. For k=n, the space diagonals connect opposite vertices and number 2^{n-1}, as each of the 2^n vertices pairs uniquely with its antipodal vertex. In n-cube with side 1, the of is \sqrt{}, since the arises from unit displacements along orthogonal axes. The longest diagonals (=n), spanning the full extent, thus have \sqrt{n}. These properties extend the notions from lower dimensions, where face diagonals (=2, \sqrt{2}) and diagonals appear in cubes, but in higher dimensions, types (2 < < n) emerge, enriching the .

Geometric Applications

Length and Distance Formulas

In a with l and width w, the diagonals are equal in length and can be found using the applied to one of the right triangles formed by the diagonal. The formula is d = \sqrt{l^2 + w^2}. This holds because the diagonal forms the of a with legs l and w. For , a special case of the where l = w = s, the diagonal length simplifies to d = s\sqrt{2}. This result follows directly from substituting equal sides into the rectangle formula, yielding the irrational factor \sqrt{2} that relates the diagonal to the side length. In a regular n-gon inscribed in a circle of radius R (the circumradius), the length of any diagonal connecting two non-adjacent vertices separated by k steps (where $2 \leq k \leq \lfloor n/2 \rfloor) is given by the chord length formula d_k = 2R \sin\left( \frac{k\pi}{n} \right). Here, k = 1 corresponds to the side length, while larger k values give diagonals of increasing length up to the diameter for k = \lfloor n/2 \rfloor. The circumradius R itself can be expressed in terms of the side length a as R = \frac{a}{2 \sin(\pi/n)}, allowing substitution for computation from side length alone. This trigonometric approach arises from the central angle $2\pi k / n subtended by the arc between the vertices. Face diagonals in polyhedra are simply the diagonals of the polygonal faces. For example, in a (rectangular prism) with dimensions l, w, and h, the face diagonals on the l \times w faces have length \sqrt{l^2 + w^2}, and similarly for the other pairs of faces. Space diagonals in polyhedra connect non-adjacent vertices through the interior. In a , all four space diagonals are equal and given by d = \sqrt{l^2 + w^2 + h^2}, derived by applying the first to a face diagonal and then to the resulting in three dimensions with the third edge as the other leg. For more general polyhedra, such as regular ones, space diagonal lengths require coordinate geometry or methods, often involving the distances between vertices in space. These formulas extend the metric, where the length of a diagonal between two points (x_1, y_1) and (x_2, y_2) in the plane is \sqrt{(x_2 - x_1)^2 + (y_2 - y_1)^2}, generalizing to three dimensions as \sqrt{(x_2 - x_1)^2 + (y_2 - y_1)^2 + (z_2 - z_1)^2} for space diagonals. In geometric applications, such distances quantify separations in lattices or grids, where diagonals represent shortest paths avoiding edges.

Theorems Involving Diagonals

Several fundamental theorems in plane relate to the properties and relationships of diagonals in quadrilaterals and polygons. One of the most prominent is , which applies to . For a cyclic quadrilateral ABCD with sides a = BC, b = CD, c = DA, d = AB, and diagonals p = AC, q = BD, the theorem states that the product of the diagonals equals the sum of the products of the opposite sides: p \cdot q = ac + bd. This relation, originally described by the Greek astronomer in the 2nd century AD, provides a way to compute diagonal lengths or verify cyclicity. In , the diagonals exhibit a characteristic bisecting property. The diagonals of a parallelogram bisect each other, meaning they intersect at their midpoints. Conversely, if the diagonals of a bisect each other, then the is a parallelogram. This bidirectional is central to classifying parallelograms and can be proved using vector or congruent triangles formed by the intersection point. For kites, a specific type of with two pairs of adjacent equal sides, the diagonals are , and one diagonal bisects the other. Specifically, the of diagonal bisects both the other diagonal and the two equal angles adjacent to it. The holds: if one diagonal of a is the bisector of the other, the quadrilateral is a . This property arises from the and can be demonstrated via the in the resulting right triangles. Varignon's theorem connects diagonals to a derived . Connecting the midpoints of the sides of any forms a (the Varignon parallelogram), whose perimeter equals the sum of the lengths of the original 's diagonals. Additionally, the area of this Varignon is half the area of the original . These relations highlight how diagonals influence the geometry of constructions. When diagonals are perpendicular, regardless of the quadrilateral type, the area simplifies significantly. For any with diagonals of lengths d_1 and d_2, the area is \frac{1}{2} d_1 d_2. This , applicable to kites, rhombi, and orthodiagonal quadrilaterals, follows from dividing the into four right triangles and summing their areas. In regular polygons, diagonals satisfy symmetry-based theorems, such as the equality of diagonals spanning the same number of sides. For example, in a regular pentagon, all diagonals are equal in length, forming a , and their intersections divide each diagonal in the \phi = \frac{1 + \sqrt{5}}{2}. This ratio emerges from solving quadratic equations derived from the pentagon's isosceles triangles. Such properties extend to higher regular polygons, where diagonal lengths can be expressed using like \cos\left(\frac{2\pi k}{n}\right) for the k-th diagonal in an n-gon.

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