Cuspidal Cubic
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mathematics Mathematics is an area of knowledge that includes the topics of numbers, formulas and related structures, shapes and the spaces in which they are contained, and quantities and their changes. These topics are represented in modern mathematics ...
, a cuspidal cubic or semicubical parabola is an algebraic plane curve that has an implicit equation of the form : y^2 - a^2 x^3 = 0 (with ) in some
Cartesian coordinate system A Cartesian coordinate system (, ) in a plane is a coordinate system that specifies each point uniquely by a pair of numerical coordinates, which are the signed distances to the point from two fixed perpendicular oriented lines, measured in t ...
. Solving for leads to the ''explicit form'' : y = \pm a x^, which imply that every real point satisfies . The exponent explains the term ''semicubical parabola''. (A parabola can be described by the equation .) Solving the implicit equation for yields a second ''explicit form'' :x = \left(\frac\right)^. The
parametric equation In mathematics, a parametric equation defines a group of quantities as functions of one or more independent variables called parameters. Parametric equations are commonly used to express the coordinates of the points that make up a geometric obj ...
: \quad x = t^2, \quad y = a t^3 can also be deduced from the implicit equation by putting t = \frac. . The semicubical parabolas have a cuspidal singularity; hence the name of ''cuspidal cubic''. The arc length of the curve was calculated by the English mathematician William Neile and published in 1657 (see section History).


Properties of semicubical parabolas


Similarity

Any semicubical parabola (t^2,at^3) is similar to the ''semicubical unit parabola'' ''Proof:'' The similarity (x,y) \rightarrow (a^2x,a^2y) (uniform scaling) maps the semicubical parabola (t^2,at^3) onto the curve ((at)^2,(at)^3) = (u^2,u^3) with


Singularity

The parametric representation (t^2,at^3) is '' regular except'' at point At point (0,0) the curve has a '' singularity'' (cusp). The ''proof'' follows from the tangent vector Only for t=0 this vector has zero length.


Tangents

Differentiating the ''semicubical unit parabola'' y = \pm x^ one gets at point (x_0,y_0) of the ''upper'' branch the equation of the tangent: : y = \frac\left(3x-x_0\right) . This tangent intersects the ''lower'' branch at exactly one further point with coordinates : \left(\frac, -\frac\right) . (Proving this statement one should use the fact, that the tangent meets the curve at (x_0,y_0) twice.)


Arclength

Determining the arclength of a curve (x(t),y(t)) one has to solve the integral \int \sqrt \;dt . For the semicubical parabola (t^2,at^3), \; 0\le t\le b , one gets : \int^b_0\sqrt \;dt = \int^b_0 t\sqrt\; dt = \cdots = \left frac \left(4 + 9a^2t^2\right)^\frac\rightb_0\; . (The integral can be solved by the
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''Example:'' For (semicubical unit parabola) and which means the length of the arc between the origin and point (4,8), one gets the arc length 9.073.


Evolute of the unit parabola

The evolute of the ''parabola'' (t^2,t) is a semicubical parabola shifted by 1/2 along the ''x''-axis: \left(\frac+t^2,\fract^3\right).


Polar coordinates

In order to get the representation of the semicubical parabola (t^2,at^3) in polar coordinates, one determines the intersection point of the line y=mx with the curve. For m\ne 0 there is one point different from the origin: \left(\frac, \frac\right). This point has distance \frac\sqrt from the origin. With m=\tan \varphi and \sec^2 \varphi = 1 + \tan^2\varphi ( see List of identities) one gets August Pein: ''Die semicubische oder Neil'sche Parabel, ihre Sekanten und Tangenten '',p. 10 : r=\left(\frac\right)^2 \sec \varphi \; ,\quad -\frac < \varphi < \frac .


Relation between a semicubical parabola and a cubic function

Mapping the semicubical parabola (t^2,t^3) by the
projective map In projective geometry, a homography is an isomorphism of projective spaces, induced by an isomorphism of the vector spaces from which the projective spaces derive. It is a bijection that maps lines to lines, and thus a collineation. In general, ...
(x,y) \rightarrow \left(\frac, \frac\right) (involutoric perspectivity with axis y=1 and center yields \left(\frac, \frac\right), hence the ''cubic function'' y=x^3. The cusp (origin) of the semicubical parabola is exchanged with the point at infinity of the y-axis. This property can be derived, too, if one represents the semicubical parabola by '' homogeneous coordinates'': In equation (A) the replacement x=\tfrac, \; y=\tfrac (the line at infinity has equation and the multiplication by x_3^3 is performed. One gets the equation of the curve *in ''homogeneous coordinates'': x_3 x_2^2 - x_1^3 = 0 . Choosing line x_=0 as line at infinity and introducing x=\tfrac, \; y=\tfrac yields the (affine) curve y=x^3.


Isochrone curve

An additional defining property of the semicubical parabola is that it is an isochrone curve, meaning that a particle following its path while being pulled down by gravity travels equal vertical intervals in equal time periods. In this way it is related to the tautochrone curve, for which particles at different starting points always take equal time to reach the bottom, and the brachistochrone curve, the curve that minimizes the time it takes for a falling particle to travel from its start to its end.


History

The semicubical parabola was discovered in 1657 by William Neile who computed its arc length. Although the lengths of some other non-algebraic curves including the logarithmic spiral and cycloid had already been computed (that is, those curves had been ''rectified''), the semicubical parabola was the first algebraic curve (excluding the
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and circle) to be rectified.


References

*August Pein: ''Die semicubische oder Neil'sche Parabel, ihre Sekanten und Tangenten '', 1875
Dissertation Clifford A. Pickover: ''The Length of Neile's Semicubical Parabola''


External links

* {{DEFAULTSORT:Semicubical Parabola Plane curves