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Third derivative
Third derivative
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In calculus, a branch of mathematics, the third derivative or third-order derivative is the rate at which the second derivative, or the rate of change of the rate of change, is changing. The third derivative of a function can be denoted by

Other notations for differentiation can be used, but the above are the most common.

Mathematical definitions

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Let . Then and . Therefore, the third derivative of f is, in this case,

or, using Leibniz notation,

Now for a more general definition. Let f be any function of x such that f ′′ is differentiable. Then the third derivative of f is given by

The third derivative is the rate at which the second derivative (f′′(x)) is changing.

Applications in geometry

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In differential geometry, the torsion of a curve — a fundamental property of curves in three dimensions — is computed using third derivatives of coordinate functions (or the position vector) describing the curve.[1]

Applications in physics

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In physics, particularly kinematics, jerk is defined as the third derivative of the position function of an object. It is, essentially, the rate at which acceleration changes. In mathematical terms:

where j(t) is the jerk function with respect to time, and r(t) is the position function of the object with respect to time.

Economic examples

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When campaigning for a second term in office, U.S. President Richard Nixon announced that the rate of increase of inflation was decreasing, which has been noted as "the first time a sitting president used the third derivative to advance his case for reelection."[2] Since inflation is itself a derivative—the rate at which the purchasing power of money decreases—then the rate of increase of inflation is the derivative of inflation, opposite in sign to the second time derivative of the purchasing power of money. Stating that a function is decreasing is equivalent to stating that its derivative is negative, so Nixon's statement is that the second derivative of inflation is negative, and so the third derivative of purchasing power is positive.

Since Nixon's statement allowed for the rate of inflation to increase, his statement did not necessarily indicate immediate price stability but proposed a trend of more stability in the future.

See also

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References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
In , the third derivative of a function f(x)f(x) is defined as the of its f(x)f''(x), denoted as f(x)f'''(x) or d3fdx3\frac{d^3 f}{dx^3}, and it measures the rate of change of the concavity of the function's graph. This higher-order provides insight into how rapidly the —captured by the second derivative—is itself changing at a given point, which can indicate the behavior near inflection points or the sharpness of transitions in the function's shape. Notation for the third derivative follows standard conventions in , such as the prime notation f(x)f'''(x) for successive differentiation or the Leibniz notation d3ydx3\frac{d^3 y}{dx^3} for a function y=f(x)y = f(x). For example, if f(x)=5x33x2+10x5f(x) = 5x^3 - 3x^2 + 10x - 5, the first is f(x)=15x26x+10f'(x) = 15x^2 - 6x + 10, the second is f(x)=30x6f''(x) = 30x - 6, and the third is the constant f(x)=30f'''(x) = 30. In general, for functions of degree nn, the third (and higher) will simplify accordingly, becoming zero if the order exceeds the degree. In physics and , particularly , the third derivative of position with respect to time—known as jerk (symbol jj)—represents the rate of change of and has units of meters per second cubed (m/s³). Jerk is crucial for analyzing motion profiles in systems like vehicles and machinery, where limiting its magnitude (e.g., below 2 m/s³ for passenger comfort in trains) helps minimize discomfort and mechanical stress. Early research by , for instance, identified jerk as a key factor in ride quality during road testing, extending beyond mere control to optimize dynamic responses in . Applications also extend to , such as constraining jerk in the Hubble Space Telescope's mechanisms to protect sensitive instruments.

Mathematical Foundations

Definition and Computation

In single-variable calculus, the third derivative of a function f(x)f(x) is defined as the derivative of its second derivative, denoted f(x)f'''(x) or d3fdx3\frac{d^3 f}{dx^3}, which quantifies the rate of change of the concavity of the function as determined by the second derivative f(x)f''(x). To compute the third derivative analytically, differentiation is applied successively starting from the original function. First, obtain the first f(x)f'(x) using standard rules such as the power rule or ; then differentiate f(x)f'(x) to yield the second f(x)f''(x); finally, differentiate f(x)f''(x) to arrive at f(x)f'''(x). For instance, consider the cubic f(x)=x3f(x) = x^3: the first is f(x)=3x2f'(x) = 3x^2, the second is f(x)=6xf''(x) = 6x, and the third is f(x)=6f'''(x) = 6. This process assumes f(x)f(x) is sufficiently differentiable, and for polynomials of degree nn, the (n+1)(n+1)-th and higher are zero. In multivariable calculus, the third derivative extends to partial derivatives, including pure partials like 3fx3\frac{\partial^3 f}{\partial x^3} (differentiating three times with respect to xx) and mixed partials such as 3fxyz\frac{\partial^3 f}{\partial x \partial y \partial z} for a function f(x,y,z)f(x, y, z). These are computed by applying the partial differentiation operator sequentially to the lower-order partials, following the same rules as single-variable cases but holding other variables constant. Clairaut's theorem, extended to higher orders, states that if the relevant partial derivatives are continuous in a neighborhood of the point, then mixed partials of the same total order are equal regardless of differentiation sequence—for example, 3fxyz=3fzxy\frac{\partial^3 f}{\partial x \partial y \partial z} = \frac{\partial^3 f}{\partial z \partial x \partial y}. When analytical computation is infeasible, numerical approximations of the third can be obtained using methods, which rely on function evaluations at discrete points. A common forward for the third at xx with step size h>0h > 0 is given by f(x)f(x+3h)3f(x+2h)+3f(x+h)f(x)h3,f'''(x) \approx \frac{f(x + 3h) - 3f(x + 2h) + 3f(x + h) - f(x)}{h^3}, with a of order O(h)O(h). This derives from the third-order Taylor expansion and is exact for cubic polynomials.

Notation and Symbols

The third derivative of a function f(x)f(x) is commonly denoted using several established notations in mathematics. In Leibniz notation, introduced in the late 17th century, it is expressed as d3ydx3\frac{d^3 y}{dx^3} for a function y=f(x)y = f(x), emphasizing the infinitesimal changes through repeated differentiation. This form highlights the variable of differentiation in the denominator, making it particularly useful for partial derivatives or when specifying the independent variable. In contrast, Lagrange notation, developed in the 18th century, uses primes to indicate successive derivatives, writing the third derivative as f(x)f'''(x). This compact functional notation, inspired by earlier ideas from Newton, is prevalent in pure mathematics for its simplicity in expressing higher-order derivatives without explicit variables. Newton's notation, originally fluxional and adapted for time derivatives, employs dots over the variable to denote differentiation with respect to time tt. For position x(t)x(t), the first () is x˙\dot{x}, the second () is x¨\ddot{x}, and the third (jerk) is x...\dddot{x}. This overdot convention extends naturally to higher orders but is primarily used in physics and contexts involving temporal rates of change. The historical evolution of these notations traces back to the independent development of calculus by Isaac Newton and Gottfried Wilhelm Leibniz in the 1670s. Leibniz first proposed his fractional form, including dxdx and dydy, in a 1675 manuscript, formalizing it in publications from 1684 onward to represent differentials and their ratios. By the late 18th century, Joseph-Louis Lagrange refined the notation in his 1797 treatise Théorie des fonctions analytiques, introducing the prime symbol f(x)f'(x) as a shorthand for the derivative, which was later extended to multiple primes for higher orders; this shift aimed to treat derivatives as operations on functions rather than ratios of infinitesimals. Newton's dot notation, detailed in his Principia Mathematica (1687) and later works, evolved from fluxions and gained traction in applied sciences for its alignment with physical motions. In physics, particularly kinematics, the third time derivative of position—known as jerk—is often denoted by x...\dddot{x} or the symbol jj, with units of m/s³. This extends Newton's dot notation and is used to describe changes in acceleration, such as in vehicle dynamics or roller coaster design. In vector calculus, 3f\nabla^3 f is not standard notation for the third derivative but may refer to a higher-order operator, such as components of the third partial derivatives tensor, depending on context; it is distinct from scalar third derivatives like f(x)f'''(x). Conventions for higher-order derivatives build on these notations, with the fourth derivative (snap or jounce) marked by quadruple dots x....\ddddot{x} in Newtonian form or f(4)(x)f^{(4)}(x) in Lagrange notation, distinguishing it from the third. The following table compares notations for the first three derivatives of y=f(x)y = f(x) or position x(t)x(t):
OrderDescriptionLeibniz NotationLagrange NotationNewton Notation (time tt)
1First derivativedydx\frac{dy}{dx} or dxdt\frac{dx}{dt}f(x)f'(x)x˙\dot{x}
2Second derivatived2ydx2\frac{d^2 y}{dx^2} or d2xdt2\frac{d^2 x}{dt^2}f(x)f''(x)x¨\ddot{x}
3Third derivatived3ydx3\frac{d^3 y}{dx^3} or d3xdt3\frac{d^3 x}{dt^3}f(x)f'''(x)x...\dddot{x}

Interpretations in Calculus

Role in Taylor Series Expansion

In the Taylor series expansion of a function f(x)f(x) around a point aa, the third derivative plays a crucial role in providing a cubic approximation to the function's local behavior. states that if ff is three times differentiable in an interval containing aa and xx, then f(x)=f(a)+f(a)(xa)+f(a)2!(xa)2+f(c)3!(xa)3f(x) = f(a) + f'(a)(x - a) + \frac{f''(a)}{2!}(x - a)^2 + \frac{f'''(c)}{3!}(x - a)^3 for some cc between aa and xx, where the third-order term f(c)3!(xa)3\frac{f'''(c)}{3!}(x - a)^3 captures the leading nonlinear deviation beyond quadratic behavior, enabling more precise s for functions with or rapid changes near aa. To quantify the accuracy of truncating the expansion after the quadratic term, the Lagrange form of the remainder after the second derivative (or equivalently, the error bound using the third derivative for the next term) is given by R2(x)=f(ξ)3!(xa)3R_2(x) = \frac{f'''(\xi)}{3!}(x - a)^3 for some ξ\xi between aa and xx, but for approximations up to the third order, the remainder becomes R3(x)=f(4)(ξ)4!(xa)4R_3(x) = \frac{f^{(4)}(\xi)}{4!}(x - a)^4 for some ξ\xi between aa and xx, assuming ff is four times differentiable. This remainder term highlights how the third derivative indirectly bounds the error in lower-order approximations by influencing the cubic contribution, which is essential for estimating convergence in numerical methods or series summations. A concrete example is the Maclaurin series expansion of sin(x)\sin(x) around a=0a = 0, where f(x)=sin(x)f(x) = \sin(x), f(x)=cos(x)f'(x) = \cos(x), f(x)=sin(x)f''(x) = -\sin(x), and f(x)=cos(x)f'''(x) = -\cos(x), yielding the third-order term x36-\frac{x^3}{6} since f(0)=1f'''(0) = -1. This cubic term approximates the oscillatory nature of sin(x)\sin(x) near the origin, improving accuracy for small xx compared to linear or quadratic approximations. The Maclaurin series, as the special case of at a=0a = 0, relies on the third to reveal cubic or higher-order asymmetries in function behavior close to the origin, particularly for oscillatory functions like trigonometric ones or those with points.

Higher-Order Derivative Tests

In , higher-order derivative tests extend the first and tests to classify critical points and points when lower-order derivatives are inconclusive, particularly relying on the when the second derivative vanishes. These tests leverage the expansion around a point cc where f(c)=0f'(c) = 0, approximating the function's behavior locally as f(x)f(c)+f(c)2!(xc)2+f(c)3!(xc)3+f(x) \approx f(c) + \frac{f''(c)}{2!}(x-c)^2 + \frac{f'''(c)}{3!}(x-c)^3 + \cdots. If the second derivative f(c)=0f''(c) = 0, the third derivative f(c)f'''(c) determines the nature of the point by examining the sign and order of the leading non-zero term. The third derivative test for inflection points applies when f(c)=0f''(c) = 0. If f(c)0f'''(c) \neq 0, then cc is an , as the concavity of ff changes at cc. This follows from the Taylor expansion, where the cubic term f(c)6(xc)3\frac{f'''(c)}{6}(x-c)^3 dominates near cc, causing the second derivative to change sign: for f(c)>0f'''(c) > 0, the function transitions from concave down to concave up, and vice versa if f(c)<0f'''(c) < 0. For example, consider f(x)=x3f(x) = x^3: here, f(x)=6xf''(x) = 6x, so f(0)=0f''(0) = 0, and f(x)=6>0f'''(x) = 6 > 0 at x=0x=0, confirming an where concavity changes from down (for x<0x < 0) to up (for x>0x > 0). For refining the classification of extrema at critical points where f(c)=0f''(c) = 0, the higher-order derivative test examines successive derivatives until finding the first non-zero one beyond the first. Suppose the lowest order k2k \geq 2 with f(k)(c)0f^{(k)}(c) \neq 0; a brief proof sketch uses , showing that near cc, f(x)f(c)f(x) - f(c) has the sign of f(k)(c)k!(xc)k\frac{f^{(k)}(c)}{k!}(x-c)^k. If kk is even and f(k)(c)>0f^{(k)}(c) > 0, then cc is a local minimum; if f(k)(c)<0f^{(k)}(c) < 0, a local maximum. If kk is odd (such as k=3k=3), cc is neither a local extremum nor an inflection point in the extremum sense but indicates a horizontal inflection, as the function changes monotonicity without extremal behavior. Thus, when f(c)=0f''(c) = 0 and f(c)0f'''(c) \neq 0, the odd order implies no local extremum. An illustrative example is f(x)=x4f(x) = x^4: f(x)=4x3f'(x) = 4x^3, so f(0)=0f'(0) = 0; f(x)=12x2f''(x) = 12x^2, so f(0)=0f''(0) = 0; f(x)=24xf'''(x) = 24x, so f(0)=0f'''(0) = 0. The third derivative vanishes, requiring the fourth: f(4)(x)=24>0f^{(4)}(x) = 24 > 0, an even order, confirming a local minimum at x=0x=0. This distinguishes cases where even lower orders suffice from those needing higher scrutiny, unlike odd-order scenarios that preclude extrema. These tests have limitations: if f(c)=0f'''(c) = 0, the analysis is inconclusive, necessitating higher derivatives or alternative methods like the . For instance, functions like f(x)=x5f(x) = x^5 at x=0x=0 have f(0)=0f'''(0) = 0 and an odd fifth-order term, yielding neither extremum nor in the concavity sense, highlighting the need for complete Taylor assessment.

Applications in Physics

Jerk in Kinematics

In kinematics, jerk is defined as the third time derivative of an object's position or the first time derivative of its acceleration, quantifying the rate at which acceleration changes. Mathematically, for one-dimensional motion, it is expressed as j(t)=d3x(t)dt3=da(t)dtj(t) = \frac{d^3 x(t)}{dt^3} = \frac{da(t)}{dt}, where x(t)x(t) is position and a(t)a(t) is acceleration. This derivative builds sequentially on lower-order kinematic quantities: position x(t)x(t) yields v(t)=dx(t)dtv(t) = \frac{dx(t)}{dt}, which in turn yields a(t)=d2x(t)dt2a(t) = \frac{d^2 x(t)}{dt^2}, and finally jerk j(t)=d3x(t)dt3j(t) = \frac{d^3 x(t)}{dt^3}. In three-dimensional space, jerk is a vector j(t)=d3r(t)dt3\vec{j}(t) = \frac{d^3 \vec{r}(t)}{dt^3}
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