How to Take Derivatives

Understand the definition of the derivative., Understand the derivative notation., Substitute (x+Δx){\displaystyle (x+\Delta x)} into the function., Substitute the function into the limit., Use the power rule when f(x){\displaystyle f(x)} is a...

15 Steps 10 min read Advanced

Step-by-Step Guide

  1. Step 1: Understand the definition of the derivative.

    While this will almost never be used to actually take derivatives, an understanding of this concept is vital nonetheless.

    Recall that the linear function is of the form y=mx+b.{\displaystyle y=mx+b.} To find the slope m{\displaystyle m} of this function, two points on the line are taken, and their coordinates are plugged into the relation m=y2−y1x2−x1.{\displaystyle m={\frac {y_{2}-y_{1}}{x_{2}-x_{1}}}.} Of course, this can only be used with linear graphs.

    For nonlinear functions, the line will be curved, so taking the difference of two points can only give the average rate of change between them.

    The line that intersects these two points is called the secant line, with a slope m=f(x+Δx)−f(x)Δx,{\displaystyle m={\frac {f(x+\Delta x)-f(x)}{\Delta x}},} where Δx=x2−x1{\displaystyle \Delta x=x_{2}-x_{1}} is the change in x,{\displaystyle x,} and we have replaced y{\displaystyle y} with f(x).{\displaystyle f(x).} This is the same equation as the one before.

    The concept of the derivatives comes in when we take the limit Δx→0.{\displaystyle \Delta x\to
    0.} When this happens, the distance between the two points shrinks, and the secant line better approximates the rate of change of the function.

    When we do send the limit to 0, we end up with the instantaneous rate of change and obtain the slope of the tangent line to the curve (see animation above).

    Then, we end up with the definition of the derivative, where the prime symbol denotes the derivative of the function f.{\displaystyle f.} f′(x)=limΔx→0f(x+Δx)−f(x)Δx{\displaystyle f^{\prime }(x)=\lim _{\Delta x\to 0}{\frac {f(x+\Delta x)-f(x)}{\Delta x}}} Finding the derivative from this definition stems from expanding the numerator, canceling, and then evaluating the limit, since immediately evaluating the limit will give a 0 in the denominator.
  2. Step 2: Understand the derivative notation.

    There are two common notations for the derivative, though there are others.

    Lagrange's Notation.

    In the previous step, we used this notation to denote the derivative of a function f(x){\displaystyle f(x)} by adding a prime symbol. f′(x){\displaystyle f^{\prime }(x)} This notation is pronounced "f{\displaystyle f} prime of x.{\displaystyle x.}" To form higher order derivatives, simply add another prime symbol.

    When derivatives of fourth or higher order are taken, the notation becomes f(4)(x),{\displaystyle f^{(4)}(x),} where this represents the fourth derivative.

    Leibniz's Notation.

    This is the other commonly used notation, and we will use it in the rest of the article. dfdx{\displaystyle {\frac {{\mathrm {d} }f}{{\mathrm {d} }x}}} (For shorter expressions, the function can be placed in the numerator.) This notation literally means "the derivative of f{\displaystyle f} with respect to x.{\displaystyle x.}" It may be helpful to think of it as ΔyΔx{\displaystyle {\frac {\Delta y}{\Delta x}}} for values of x{\displaystyle x} and y{\displaystyle y} that are infinitesimally different from each other.

    When using this notation for higher derivatives, you must write d2fdx2,{\displaystyle {\frac {{\mathrm {d} }^{2}f}{{\mathrm {d} }x^{2}}},} where this represents the second derivative. (Note that there "should" be parentheses in the denominator, but no one ever writes them, since everyone understands what we mean without them anyway.) , For this example, we will define f(x)=2x2+6x.{\displaystyle f(x)=2x^{2}+6x.} f(x+Δx)=2(x+Δx)2+6(x+Δx)=2(x2+2xΔx+(Δx)2)+6x+6Δx=2x2+4xΔx+2(Δx)2+6x+6Δx.{\displaystyle {\begin{aligned}f(x+\Delta x)&=2(x+\Delta x)^{2}+6(x+\Delta x)\\&=2(x^{2}+2x\Delta x+(\Delta x)^{2})+6x+6\Delta x\\&=2x^{2}+4x\Delta x+2(\Delta x)^{2}+6x+6\Delta x.\end{aligned}}} , Then evaluate the limit. ddxf(x)=limΔx→0(2x2+4xΔx+2(Δx)2+6x+6Δx)−(2x2+6x)Δx=limΔx→04xΔx+2(Δx)2+6ΔxΔx=limΔx→0Δx(4x+2Δx+6)Δx=limΔx→04x+2Δx+6=4x+6.{\displaystyle {\begin{aligned}{\frac {\mathrm {d} }{{\mathrm {d} }x}}f(x)&=\lim _{\Delta x\to 0}{\frac {(2x^{2}+4x\Delta x+2(\Delta x)^{2}+6x+6\Delta x)-(2x^{2}+6x)}{\Delta x}}\\&=\lim _{\Delta x\to 0}{\frac {4x\Delta x+2(\Delta x)^{2}+6\Delta x}{\Delta x}}\\&=\lim _{\Delta x\to 0}{\frac {\Delta x(4x+2\Delta x+6)}{\Delta x}}\\&=\lim _{\Delta x\to 0}4x+2\Delta x+6\\&=4x+6.\end{aligned}}} This is a lot of work for such a simple function.

    We will see that there are plenty of derivative rules to skirt past this type of evaluation.

    You can find the slope anywhere on the function f(x)=2x2+6x.{\displaystyle f(x)=2x^{2}+6x.} Simply plug in any x value into the derivative df(x)dx=4x+6.{\displaystyle {\frac {{\mathrm {d} }f(x)}{{\mathrm {d} }x}}=4x+6.} , The formula is ddx(xn)=nxn−1.{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}(x^{n})=nx^{n-1}.} Although the intuitive method seems to only apply to natural number exponents, it can be generalized to all real numbers; that is, n∈R.{\displaystyle n\in {\mathbb {R} }.} , f(x)=2x2+6x.{\displaystyle f(x)=2x^{2}+6x.} Remember that x=x1.{\displaystyle x=x^{1}.} f(x)=2x2+6xddxf(x)=(2)2x2−1+(1)6x1−1=4x+6.{\displaystyle {\begin{aligned}f(x)&=2x^{2}+6x\\{\frac {\mathrm {d} }{{\mathrm {d} }x}}f(x)&=(2)2x^{2-1}+(1)6x^{1-1}\\&=4x+6.\end{aligned}}} We have used the property that the derivative of a sum is the sum of the derivatives (technically, the reason why we can do this is because the derivative is a linear operator).

    Obviously, the power rule makes finding derivatives of polynomials much easier.

    Before going on, it is important to note that the derivative of a constant is 0, because the derivative measures the rate of change, and no such change exists with a constant. , Taking a higher order derivative of a function just means you take the derivative of the derivative (for order of 2).

    For example, if it asks you to take the third derivative, just differentiate the function three times.

    For polynomial functions of degree n,{\displaystyle n,} the n+1{\displaystyle n+1} order derivative will be
    0. , ddxf(x)=4x+6d2dx2f(x)=4d3dx3f(x)=0{\displaystyle {\begin{aligned}{\frac {\mathrm {d} }{{\mathrm {d} }x}}f(x)&=4x+6\\{\frac {{\mathrm {d} }^{2}}{{\mathrm {d} }x^{2}}}f(x)&=4\\{\frac {{\mathrm {d} }^{3}}{{\mathrm {d} }x^{3}}}f(x)&=0\end{aligned}}} In most applications of derivatives, especially in physics and engineering, you will at most differentiate twice, or perhaps three times. , In general, the derivative of a product does not equal the product of the derivatives.

    Rather, each function "gets its turn" to differentiate. ddx(fg)=dfdxg+fdgdx{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}(fg)={\frac {{\mathrm {d} }f}{{\mathrm {d} }x}}g+f{\frac {{\mathrm {d} }g}{{\mathrm {d} }x}}} , As with products in general, the derivative of a quotient does not equal the quotient of the derivatives. ddx(fg)=gdfdx−fdgdxg2{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\left({\frac {f}{g}}\right)={\frac {g{\frac {{\mathrm {d} }f}{{\mathrm {d} }x}}-f{\frac {{\mathrm {d} }g}{{\mathrm {d} }x}}}{g^{2}}}} A useful mnemonic for the numerator of the derivative is "Down-dee-up, up-dee-down," since the minus sign means the order matters.

    For example, consider the function f(x)=x2+2x−21x−3.{\displaystyle f(x)={\frac {x^{2}+2x-21}{x-3}}.} Let g(x)=x2+2x−21{\displaystyle g(x)=x^{2}+2x-21} and h(x)=x−3.{\displaystyle h(x)=x-3.} Then use the quotient rule. ddx(gh)=(x−3)(2x+2)−(x2+2x−21)(1)(x−3)2=x2−6x+15(x−3)2{\displaystyle {\begin{aligned}{\frac {\mathrm {d} }{{\mathrm {d} }x}}\left({\frac {g}{h}}\right)&={\frac {(x-3)(2x+2)-(x^{2}+2x-21)(1)}{(x-3)^{2}}}\\&={\frac {x^{2}-6x+15}{(x-3)^{2}}}\end{aligned}}} Make sure your algebra is up to par.

    Derivatives involving quotients like these can quickly become cumbersome in terms of the algebra involved.

    This means you should be comfortable with factoring out constants and keeping track of negative signs. , For example, consider the scenario where z(y){\displaystyle z(y)} is a differentiable function of y{\displaystyle y} and y(x){\displaystyle y(x)} is a differentiable function of x.{\displaystyle x.} Then there is a composite function z(y(x)),{\displaystyle z(y(x)),} or z{\displaystyle z} as a function of x,{\displaystyle x,} that we can take the derivative of. ddxz(y(x))=dzdydydx{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}z(y(x))={\frac {{\mathrm {d} }z}{{\mathrm {d} }y}}{\frac {{\mathrm {d} }y}{{\mathrm {d} }x}}} As with the product rule, this works with any number of functions; hence the "chain" rule.

    Here, an easy way to see how this works is if one imagines a dydy{\displaystyle {\frac {{\mathrm {d} }y}{{\mathrm {d} }y}}} inserted between dzdx.{\displaystyle {\frac {{\mathrm {d} }z}{{\mathrm {d} }x}}.} , Notice that this function can be decomposed into two elementary functions, g(x)=2x4−x{\displaystyle g(x)=2x^{4}-x} and h(g)=g3.{\displaystyle h(g)=g^{3}.} Then, we want to find the derivative of the composition f(x)=h(g(x)).{\displaystyle f(x)=h(g(x)).} Use the chain rule ddxh(g(x))=dhdgdgdx.{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}h(g(x))={\frac {{\mathrm {d} }h}{{\mathrm {d} }g}}{\frac {{\mathrm {d} }g}{{\mathrm {d} }x}}.} We have now written the derivative in terms of derivatives that are easier to take.

    Then, ddxh(g(x))=3(2x4−x)2(8x3−1).{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}h(g(x))=3(2x^{4}-x)^{2}(8x^{3}-1).} With practice, you will see that applying the chain rule is easiest if you "peel away the onion." The first layer is everything inside the parentheses, cubed.

    The second layer is the function inside the parentheses.

    When dealing with more complex functions, this way of thinking helps to keep yourself on track and not get lost in what functions are taken with respect to what variables, etc. , Understanding the chain rule is a must in order to implicitly differentiate. , ddxex=ex{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}e^{x}=e^{x}} ddxax=axln⁡a{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}a^{x}=a^{x}\ln a} ddxln⁡x=1x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\ln x={\frac {1}{x}}} ddxloga⁡x=1xln⁡a{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\log _{a}x={\frac {1}{x\ln a}}} , ddxsin⁡x=cos⁡x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\sin x=\cos x} ddxcos⁡x=−sin⁡x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\cos x=-\sin x} ddxtan⁡x=sec2⁡x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\tan x=\sec ^{2}x} ddxcot⁡x=−csc2⁡x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\cot x=-\csc ^{2}x} ddxsec⁡x=sec⁡xtan⁡x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\sec x=\sec x\tan x} ddxcsc⁡x=−csc⁡xcot⁡x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\csc x=-\csc x\cot x}
  3. Step 3: Substitute (x+Δx){\displaystyle (x+\Delta x)} into the function.

  4. Step 4: Substitute the function into the limit.

  5. Step 5: Use the power rule when f(x){\displaystyle f(x)} is a polynomial function of degree n. Multiply the exponent with the coefficient and bring down the power by one.

  6. Step 6: Use the previous example.

  7. Step 7: Differentiate again.

  8. Step 8: Take the third derivative of the previous example f(x)=2x2+6x{\displaystyle f(x)=2x^{2}+6x}.

  9. Step 9: See this article for a full treatment on the product rule.

  10. Step 10: Use the quotient rule to take derivatives of rational functions.

  11. Step 11: Use the chain rule for nested functions.

  12. Step 12: Consider the function f(x)=(2x4−x)3{\displaystyle f(x)=(2x^{4}-x)^{3}}.

  13. Step 13: See this article for a full treatment on implicit differentiation.

  14. Step 14: See this article for a full treatment on differentiating exponential functions.

  15. Step 15: Memorize basic trigonometric derivatives and how to derive them.

Detailed Guide

While this will almost never be used to actually take derivatives, an understanding of this concept is vital nonetheless.

Recall that the linear function is of the form y=mx+b.{\displaystyle y=mx+b.} To find the slope m{\displaystyle m} of this function, two points on the line are taken, and their coordinates are plugged into the relation m=y2−y1x2−x1.{\displaystyle m={\frac {y_{2}-y_{1}}{x_{2}-x_{1}}}.} Of course, this can only be used with linear graphs.

For nonlinear functions, the line will be curved, so taking the difference of two points can only give the average rate of change between them.

The line that intersects these two points is called the secant line, with a slope m=f(x+Δx)−f(x)Δx,{\displaystyle m={\frac {f(x+\Delta x)-f(x)}{\Delta x}},} where Δx=x2−x1{\displaystyle \Delta x=x_{2}-x_{1}} is the change in x,{\displaystyle x,} and we have replaced y{\displaystyle y} with f(x).{\displaystyle f(x).} This is the same equation as the one before.

The concept of the derivatives comes in when we take the limit Δx→0.{\displaystyle \Delta x\to
0.} When this happens, the distance between the two points shrinks, and the secant line better approximates the rate of change of the function.

When we do send the limit to 0, we end up with the instantaneous rate of change and obtain the slope of the tangent line to the curve (see animation above).

Then, we end up with the definition of the derivative, where the prime symbol denotes the derivative of the function f.{\displaystyle f.} f′(x)=limΔx→0f(x+Δx)−f(x)Δx{\displaystyle f^{\prime }(x)=\lim _{\Delta x\to 0}{\frac {f(x+\Delta x)-f(x)}{\Delta x}}} Finding the derivative from this definition stems from expanding the numerator, canceling, and then evaluating the limit, since immediately evaluating the limit will give a 0 in the denominator.

There are two common notations for the derivative, though there are others.

Lagrange's Notation.

In the previous step, we used this notation to denote the derivative of a function f(x){\displaystyle f(x)} by adding a prime symbol. f′(x){\displaystyle f^{\prime }(x)} This notation is pronounced "f{\displaystyle f} prime of x.{\displaystyle x.}" To form higher order derivatives, simply add another prime symbol.

When derivatives of fourth or higher order are taken, the notation becomes f(4)(x),{\displaystyle f^{(4)}(x),} where this represents the fourth derivative.

Leibniz's Notation.

This is the other commonly used notation, and we will use it in the rest of the article. dfdx{\displaystyle {\frac {{\mathrm {d} }f}{{\mathrm {d} }x}}} (For shorter expressions, the function can be placed in the numerator.) This notation literally means "the derivative of f{\displaystyle f} with respect to x.{\displaystyle x.}" It may be helpful to think of it as ΔyΔx{\displaystyle {\frac {\Delta y}{\Delta x}}} for values of x{\displaystyle x} and y{\displaystyle y} that are infinitesimally different from each other.

When using this notation for higher derivatives, you must write d2fdx2,{\displaystyle {\frac {{\mathrm {d} }^{2}f}{{\mathrm {d} }x^{2}}},} where this represents the second derivative. (Note that there "should" be parentheses in the denominator, but no one ever writes them, since everyone understands what we mean without them anyway.) , For this example, we will define f(x)=2x2+6x.{\displaystyle f(x)=2x^{2}+6x.} f(x+Δx)=2(x+Δx)2+6(x+Δx)=2(x2+2xΔx+(Δx)2)+6x+6Δx=2x2+4xΔx+2(Δx)2+6x+6Δx.{\displaystyle {\begin{aligned}f(x+\Delta x)&=2(x+\Delta x)^{2}+6(x+\Delta x)\\&=2(x^{2}+2x\Delta x+(\Delta x)^{2})+6x+6\Delta x\\&=2x^{2}+4x\Delta x+2(\Delta x)^{2}+6x+6\Delta x.\end{aligned}}} , Then evaluate the limit. ddxf(x)=limΔx→0(2x2+4xΔx+2(Δx)2+6x+6Δx)−(2x2+6x)Δx=limΔx→04xΔx+2(Δx)2+6ΔxΔx=limΔx→0Δx(4x+2Δx+6)Δx=limΔx→04x+2Δx+6=4x+6.{\displaystyle {\begin{aligned}{\frac {\mathrm {d} }{{\mathrm {d} }x}}f(x)&=\lim _{\Delta x\to 0}{\frac {(2x^{2}+4x\Delta x+2(\Delta x)^{2}+6x+6\Delta x)-(2x^{2}+6x)}{\Delta x}}\\&=\lim _{\Delta x\to 0}{\frac {4x\Delta x+2(\Delta x)^{2}+6\Delta x}{\Delta x}}\\&=\lim _{\Delta x\to 0}{\frac {\Delta x(4x+2\Delta x+6)}{\Delta x}}\\&=\lim _{\Delta x\to 0}4x+2\Delta x+6\\&=4x+6.\end{aligned}}} This is a lot of work for such a simple function.

We will see that there are plenty of derivative rules to skirt past this type of evaluation.

You can find the slope anywhere on the function f(x)=2x2+6x.{\displaystyle f(x)=2x^{2}+6x.} Simply plug in any x value into the derivative df(x)dx=4x+6.{\displaystyle {\frac {{\mathrm {d} }f(x)}{{\mathrm {d} }x}}=4x+6.} , The formula is ddx(xn)=nxn−1.{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}(x^{n})=nx^{n-1}.} Although the intuitive method seems to only apply to natural number exponents, it can be generalized to all real numbers; that is, n∈R.{\displaystyle n\in {\mathbb {R} }.} , f(x)=2x2+6x.{\displaystyle f(x)=2x^{2}+6x.} Remember that x=x1.{\displaystyle x=x^{1}.} f(x)=2x2+6xddxf(x)=(2)2x2−1+(1)6x1−1=4x+6.{\displaystyle {\begin{aligned}f(x)&=2x^{2}+6x\\{\frac {\mathrm {d} }{{\mathrm {d} }x}}f(x)&=(2)2x^{2-1}+(1)6x^{1-1}\\&=4x+6.\end{aligned}}} We have used the property that the derivative of a sum is the sum of the derivatives (technically, the reason why we can do this is because the derivative is a linear operator).

Obviously, the power rule makes finding derivatives of polynomials much easier.

Before going on, it is important to note that the derivative of a constant is 0, because the derivative measures the rate of change, and no such change exists with a constant. , Taking a higher order derivative of a function just means you take the derivative of the derivative (for order of 2).

For example, if it asks you to take the third derivative, just differentiate the function three times.

For polynomial functions of degree n,{\displaystyle n,} the n+1{\displaystyle n+1} order derivative will be
0. , ddxf(x)=4x+6d2dx2f(x)=4d3dx3f(x)=0{\displaystyle {\begin{aligned}{\frac {\mathrm {d} }{{\mathrm {d} }x}}f(x)&=4x+6\\{\frac {{\mathrm {d} }^{2}}{{\mathrm {d} }x^{2}}}f(x)&=4\\{\frac {{\mathrm {d} }^{3}}{{\mathrm {d} }x^{3}}}f(x)&=0\end{aligned}}} In most applications of derivatives, especially in physics and engineering, you will at most differentiate twice, or perhaps three times. , In general, the derivative of a product does not equal the product of the derivatives.

Rather, each function "gets its turn" to differentiate. ddx(fg)=dfdxg+fdgdx{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}(fg)={\frac {{\mathrm {d} }f}{{\mathrm {d} }x}}g+f{\frac {{\mathrm {d} }g}{{\mathrm {d} }x}}} , As with products in general, the derivative of a quotient does not equal the quotient of the derivatives. ddx(fg)=gdfdx−fdgdxg2{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\left({\frac {f}{g}}\right)={\frac {g{\frac {{\mathrm {d} }f}{{\mathrm {d} }x}}-f{\frac {{\mathrm {d} }g}{{\mathrm {d} }x}}}{g^{2}}}} A useful mnemonic for the numerator of the derivative is "Down-dee-up, up-dee-down," since the minus sign means the order matters.

For example, consider the function f(x)=x2+2x−21x−3.{\displaystyle f(x)={\frac {x^{2}+2x-21}{x-3}}.} Let g(x)=x2+2x−21{\displaystyle g(x)=x^{2}+2x-21} and h(x)=x−3.{\displaystyle h(x)=x-3.} Then use the quotient rule. ddx(gh)=(x−3)(2x+2)−(x2+2x−21)(1)(x−3)2=x2−6x+15(x−3)2{\displaystyle {\begin{aligned}{\frac {\mathrm {d} }{{\mathrm {d} }x}}\left({\frac {g}{h}}\right)&={\frac {(x-3)(2x+2)-(x^{2}+2x-21)(1)}{(x-3)^{2}}}\\&={\frac {x^{2}-6x+15}{(x-3)^{2}}}\end{aligned}}} Make sure your algebra is up to par.

Derivatives involving quotients like these can quickly become cumbersome in terms of the algebra involved.

This means you should be comfortable with factoring out constants and keeping track of negative signs. , For example, consider the scenario where z(y){\displaystyle z(y)} is a differentiable function of y{\displaystyle y} and y(x){\displaystyle y(x)} is a differentiable function of x.{\displaystyle x.} Then there is a composite function z(y(x)),{\displaystyle z(y(x)),} or z{\displaystyle z} as a function of x,{\displaystyle x,} that we can take the derivative of. ddxz(y(x))=dzdydydx{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}z(y(x))={\frac {{\mathrm {d} }z}{{\mathrm {d} }y}}{\frac {{\mathrm {d} }y}{{\mathrm {d} }x}}} As with the product rule, this works with any number of functions; hence the "chain" rule.

Here, an easy way to see how this works is if one imagines a dydy{\displaystyle {\frac {{\mathrm {d} }y}{{\mathrm {d} }y}}} inserted between dzdx.{\displaystyle {\frac {{\mathrm {d} }z}{{\mathrm {d} }x}}.} , Notice that this function can be decomposed into two elementary functions, g(x)=2x4−x{\displaystyle g(x)=2x^{4}-x} and h(g)=g3.{\displaystyle h(g)=g^{3}.} Then, we want to find the derivative of the composition f(x)=h(g(x)).{\displaystyle f(x)=h(g(x)).} Use the chain rule ddxh(g(x))=dhdgdgdx.{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}h(g(x))={\frac {{\mathrm {d} }h}{{\mathrm {d} }g}}{\frac {{\mathrm {d} }g}{{\mathrm {d} }x}}.} We have now written the derivative in terms of derivatives that are easier to take.

Then, ddxh(g(x))=3(2x4−x)2(8x3−1).{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}h(g(x))=3(2x^{4}-x)^{2}(8x^{3}-1).} With practice, you will see that applying the chain rule is easiest if you "peel away the onion." The first layer is everything inside the parentheses, cubed.

The second layer is the function inside the parentheses.

When dealing with more complex functions, this way of thinking helps to keep yourself on track and not get lost in what functions are taken with respect to what variables, etc. , Understanding the chain rule is a must in order to implicitly differentiate. , ddxex=ex{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}e^{x}=e^{x}} ddxax=axln⁡a{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}a^{x}=a^{x}\ln a} ddxln⁡x=1x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\ln x={\frac {1}{x}}} ddxloga⁡x=1xln⁡a{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\log _{a}x={\frac {1}{x\ln a}}} , ddxsin⁡x=cos⁡x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\sin x=\cos x} ddxcos⁡x=−sin⁡x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\cos x=-\sin x} ddxtan⁡x=sec2⁡x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\tan x=\sec ^{2}x} ddxcot⁡x=−csc2⁡x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\cot x=-\csc ^{2}x} ddxsec⁡x=sec⁡xtan⁡x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\sec x=\sec x\tan x} ddxcsc⁡x=−csc⁡xcot⁡x{\displaystyle {\frac {\mathrm {d} }{{\mathrm {d} }x}}\csc x=-\csc x\cot x}

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