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Vector Differentiation (Definition)

Vector Differentiation in Physics: Vector-Valued Functions, Moving Bases, and Kinematics

Vector differentiation is the study of how a vector changes with respect to a scalar parameter such as time, arc length, or an angle. It is one of the basic mathematical operations of mechanics because position, velocity, acceleration, momentum, angular momentum, force, and many other physical quantities are vectors whose magnitudes and directions may both change. A mathematically careful treatment also explains why differentiating vectors in polar, cylindrical, spherical, or rotating coordinates requires more than differentiating their scalar components [1, 2, 3].

This article focuses on derivatives of vector-valued functionshttps://physicslibrary.org/encyclopedia/Bijective.html and on their use in mechanics. Gradient, divergence, curl, and related differential operators acting on scalar and vector fields belong more naturally to vector calculus, although the final sections show how the two subjects connect.

1 A vector-valued function

Let a vector depend on a scalar parameter t:

A =  A(t).
(1)

For motion in three-dimensional Euclidean space one may write

A (t) = A  (t)e + A  (t)e +  A (t)e ,
         x    x    y    y    z    z
(2)

where ex,ey,ez are fixed Cartesian basis vectors.

The derivative is defined by the same limit used for scalar functions, except that the difference quotient is now a vector:

dA         A (t + Δt) − A (t)
----=  lim  ------------------,
 dt   Δt→0         Δt
(3)

provided this vector limit exists.

Equivalently, A is differentiable at t if there exists a vector B such that

A (t + Δt) = A (t) + BΔt  + R (Δt),
(4)

with

lim  |R-(Δt-)|=  0.
Δt→0   |Δt |
(5)

Then

     dA--
B  =  dt .
(6)

This form makes the local-linear meaning of the derivative explicit: over a sufficiently short interval, the change in the vector is the derivative multiplied by the parameter increment, plus a remainder that becomes negligible faster than Δt.

2 Componentwise differentiation in a fixed basis

If the basis vectors are constant in time,

de     de    de
--x-=  --y-= ---z = 0.
 dt    dt     dt
(7)

Therefore

dA--= dAx- e +  dAy-e +  dAz-e .
dt     dt   x    dt  y    dt  z
(8)

Thus a vector-valued function in a fixed Cartesian basis is differentiable exactly when its component functions are differentiable, and its derivative is obtained component by component.

This simple rule is often the first rule learned for vector differentiation. It is correct only because the Cartesian basis is fixed. Later we will see that a moving basis contributes its own derivatives.

3 Geometric meaning: the derivative is tangent to a curve

A vector-valued function

r = r(t)
(9)

may represent a curve in physical space. For two nearby parameter values, the difference

Δr =  r(t + Δt ) − r(t)
(10)

is a chord joining two nearby points of the curve. The difference quotient

Δr-
Δt
(11)

points along that chord. As Δt → 0, the chord direction approaches the tangent direction to the curve.

PIC

Figure 1. The derivative of a vector-valued position function is the limit of secant vectors and is tangent to the trajectory. In mechanics this derivative is velocity.

For a particle position r(t),

       dr
v(t) = ---
       dt
(12)

is therefore tangent to the path. The acceleration is the derivative of the velocity,

              2
a(t) = dv- = d-r-.
       dt    dt2
(13)

Acceleration need not point along the path because it measures the change of the entire velocity vector, including both its magnitude and its direction.

4 Differentiation with respect to another parameter

A curve can be parameterized by a quantity other than time. Suppose

r = r(s)
(14)

and s = s(t). The chain rule gives

dr-   drds-
dt =  dsdt .
(15)

If s is arc length, then

|   |
|dr |
||---|| = 1,
 ds
(16)

so the vector

     dr
et = ---
     ds
(17)

is the unit tangent to the path. Since

ds-=  v,
dt
(18)

where v = |v| is speed,

v = ve .
      t
(19)

This decomposition will be useful when differentiating the velocity.

5 Product rules for vectors

The familiar scalar product rule extends naturally to vector products. Let f(t) be a scalar and let A(t) and B(t) be differentiable vectors.

For scalar multiplication,

-d(f A ) = df-A +  fdA--.
dt         dt       dt
(20)

For the dot product,

d-          dA--          dB-
dt(A ⋅ B ) = dt ⋅ B + A ⋅ dt .
(21)

For the cross product,

d-(A  × B ) = dA--× B +  A ×  dB-.
dt            dt              dt
(22)

The order in the cross-product rule matters because

A  × B  = − B × A.
(23)

These identities can be proved directly from the limit definition using bilinearity of the dot and cross products.

6 Derivative of a vector magnitude

Let

A = |A |
(24)

with A≠0. Since

A2 = A  ⋅ A,
(25)

differentiation gives

2A dA-=  2A ⋅ dA-.
   dt         dt
(26)

Therefore

dA-   -A--  dA--
dt  = |A | ⋅ dt .
(27)

If

e  = -A--,
 A   |A |
(28)

then

dA-       dA--
dt =  eA ⋅ dt .
(29)

Only the part of dA∕dt parallel to A changes the magnitude. A perpendicular derivative changes the direction without changing the magnitude to first order.

A useful mechanics example is

dv-=  v-⋅ a-,
dt      v
(30)

provided v≠0.

7 Derivative of a unit vector

Let

e =  A-
     A
(31)

be a unit vector. Differentiating

e ⋅ e = 1
(32)

gives

    de
2e ⋅---=  0.
    dt
(33)

Hence

   de
e ⋅--- = 0.
    dt
(34)

The derivative of a unit vector is therefore perpendicular to the unit vector itself.

A more explicit formula follows from e = A∕A:

        [        (       ) ]
de-=  1-  dA--− e  e ⋅ dA-   .
dt    A   dt           dt
(35)

The bracket removes the component of dA∕dt parallel to A. What remains is the perpendicular part responsible for turning the vector.

This result is fundamental in orbital mechanics, rigid-body kinematics, moving coordinate systems, and Differential Geometry.

8 Velocity and acceleration along a curved path

Write the velocity as

v = vet,
(36)

where et is the unit tangent. Differentiation gives

     dv      det
a =  --et + v---.
     dt       dt
(37)

The derivative of et must be perpendicular to et. For a smooth plane curve, define the radius of curvature ρ and principal normal en by

det-=  1en.
 ds    ρ
(38)

Using ds∕dt = v,

det-=  ve .
 dt    ρ n
(39)

Therefore

     dv     v2
a =  --et + --en.
     dt     ρ
(40)

PIC

Figure 2. Acceleration separates into a tangential part that changes speed and a normal part that changes the direction of the velocity. The normal acceleration points toward the local center of curvature.

Thus

a =  dv-e
 t   dt  t
(41)

changes the speed, while

     v2
an = -ρ en
(42)

changes the direction of motion. Uniform circular motion has dv∕dt = 0 but still has nonzero acceleration because et continuously changes direction.

9 A physics example: differentiating angular momentum

For a particle with position r and momentum p,

L  = r × p.
(43)

Using the cross-product differentiation rule,

dL    dr            dp
--- = ---×  p + r × ---.
 dt   dt            dt
(44)

For constant mass,

p =  mv,
(45)

so

v × p =  mv  × v = 0.
(46)

Newton’s second law gives

dp-=  F.
dt
(47)

Therefore

dL
---=  r × F.
dt
(48)

Since torque is defined by

⃗τ =  r × F,
(49)

we obtain

dL-=  ⃗τ.
dt
(50)

This derivation shows how a basic vector product rule becomes one of the central dynamical relations of mechanics.

10 The crucial complication: a moving basis

Suppose a vector is written in a basis whose directions themselves depend on time:

A  = A  e + A  e  + A e  .
       1 1    2 2     3 3
(51)

Now the product rule gives

dA-=  dA1-e1 + dA2-e2 + dA3-e3 + A1 de1-+ A2 de2-+ A3 de3.
dt     dt       dt       dt         dt       dt       dt
(52)

The last three terms vanish only when the basis vectors are fixed.

This is the source of many additional terms in polar, cylindrical, spherical, and rotating-coordinate equations of motion. They are not artificial corrections; they arise because the coordinate directions themselves change.

11 Polar-coordinate basis derivatives

In the plane, define

e =  cos𝜃 e +  sin 𝜃e
 r         x        y
(53)

and

e 𝜃 = − sin 𝜃ex + cos 𝜃ey.
(54)

Differentiating with respect to 𝜃 gives

der
----=  e𝜃,
 d𝜃
(55)

de-𝜃=  − e .
 d𝜃       r
(56)

The chain rule then gives

der-   ˙
 dt =  𝜃e 𝜃,
(57)

de𝜃-= − ˙𝜃e .
dt        r
(58)

PIC

Figure 3. The polar basis moves with the particle’s angular coordinate. Even when the scalar components of a vector are constant, the vector can change because er and e𝜃 rotate.

The position vector is

r = re .
      r
(59)

Differentiating,

v = ˙r er + r𝜃˙e𝜃.
(60)

Differentiating again,

a =  (¨r − r𝜃˙2)er + (r¨𝜃 + 2˙r𝜃˙)e𝜃.
(61)

The term

− r˙𝜃2er
(62)

is the inward centripetal contribution, while

   ˙
2˙r𝜃e𝜃
(63)

is produced by simultaneous radial motion and rotation of the basis.

These terms follow entirely from differentiating the basis vectors correctly.

12 Rotating frames and the transport theorem

The polar-coordinate result is a special case of a more general rule. Let a rotating basis e′1,e′2,e′3 have angular velocity ω relative to an inertial frame. Each basis vector satisfies

( de′)
  --i   =  ⃗ω × e′i.
  dt   I
(64)

For

A  = A1e ′1 + A2e ′2 + A3e ′3,
(65)

differentiation gives

(     )    (    )
  dA--   =   dA--   + ⃗ω × A.
   dt  I      dt  R
(66)

This is the vector transport theorem.

PIC

Figure 4. A vector expressed in a rotating basis changes in an inertial frame for two reasons: its components can change relative to the rotating frame, and the basis itself rotates with angular velocity ω.

Applying the transport theorem to a particle position relative to a moving origin gives the inertial velocity

vI =  VO +  vR + ⃗ω × r.
(67)

Differentiating once more gives the inertial acceleration

                           ˙
aI = aO  + aR + 2⃗ω ×  vR + ⃗ω × r + ⃗ω × (⃗ω × r).
(68)

The additional terms are, respectively, the Coriolis, Euler, and centrifugal contributions. Their origin is vector differentiation in a rotating basis.

13 Vector fields and the derivative following a particle

The previous sections considered a vector that depends directly on one scalar parameter. Physics also uses vector fields such as velocity, electric field, or magnetic field:

A =  A(r,t).
(69)

A particle following a trajectory r(t) samples different points of the field. The ordinary chain rule applied componentwise gives

dAi-= ∂Ai- + ∂Ai-dx- + ∂Ai-dy-+  ∂Ai-dz.
dt     ∂t     ∂x  dt    ∂y dt    ∂z  dt
(70)

In vector notation this is

dA--  ∂A--
dt  =  ∂t +  (v ⋅ ∇ )A.
(71)

In continuum mechanics and fluid mechanics this is called the material or substantial derivative. The first term measures explicit change of the field at a fixed point, while the second measures change caused by motion through a spatially nonuniform field.

This formula is also a useful bridge to vector calculus. The derivative of a vector-valued trajectory and the spatial differentiation of a vector field are related but distinct ideas.

14 Differentials and infinitesimal changes

If A(t) is differentiable, its differential is

       dA--
dA  =  dt dt.
(72)

This equation is best interpreted as the linear part of the change in A associated with a small change dt. More precisely,

       dA
ΔA   = ----Δt + R (Δt ),
        dt
(73)

where

|R-(Δt)|
  |Δt|   →  0.
(74)

This interpretation prevents a common confusion: dA is not an arbitrary tiny vector inserted by notation; it is the linear map generated by the derivative acting on the small scalar increment dt.

15 Common errors

Several mistakes recur in mechanics problems involving vector differentiation.

  • Differentiating only components in a moving basis. In polar, spherical, or rotating coordinates the basis vectors also have derivatives.
  • Assuming zero speed derivative means zero acceleration. Constant speed does not imply constant velocity. Uniform circular motion is the standard counterexample.
  • Treating the derivative of a unit vector as parallel to the vector. Since the magnitude is fixed, the derivative of a unit vector is perpendicular to it.
  • Reversing factors in a differentiated cross product. The correct order is preserved:
    d
--(A ×  B) = A˙ × B +  A × B˙.
dt
    (75)

  • Confusing vector differentiation with vector differential operators. dA∕dt differentiates a vector-valued function with respect to a scalar. Quantities such as ∇⋅ A and ∇× A describe spatial derivatives of a vector field.

16 Worked example: a planar spiral

Consider

r(t) = r0 + ut,
(76)

𝜃(t) = Ωt,
(77)

where u and Ω are constants. Then

˙r = u,
(78)

¨r = 0,
(79)

𝜃˙=  Ω,
(80)

¨𝜃 = 0.
(81)

The polar-coordinate velocity is

v = uer + (r0 + ut)Ωe 𝜃.
(82)

The acceleration is

                2
a =  − (r0 + ut)Ω er + 2u Ωe𝜃.
(83)

Even though both scalar rates u and Ω are constant, the acceleration is not zero because the polar basis rotates and because the tangential speed rΩ changes as the radius changes.

This is a compact demonstration of why vector differentiation is more than differentiating scalar coefficients.

17 Relation to classical mechanics

Vector differentiation underlies many of the standard equations of classical mechanics:

    dr-
v =  dt,
(84)

    dv-
a = dt ,
(85)

     dp
F  = ---,
      dt
(86)

    dL
⃗τ = ---.
    dt
(87)

It also supplies the kinematic machinery behind curvilinear coordinates, orbital frames, rotating rigid bodies, Coriolis effects, and non-inertial reference frames. For this reason physics texts often introduce vector differentiation early in mechanics, before moving on to full equations of motion [1, 2].

Summary

The derivative of a vector-valued function is defined by the vector limit

dA--=  lim  A-(t +-Δt)-−-A-(t).
 dt   Δt→0         Δt
(88)

In a fixed Cartesian basis it is obtained by differentiating components. In a moving basis, the basis vectors must also be differentiated. Product rules apply to scalar multiplication, dot products, and cross products. The derivative of a unit vector is perpendicular to that unit vector, which leads naturally to tangential-normal acceleration and to the extra terms appearing in polar and rotating coordinates.

The central lesson for mechanics is simple:

A vector can change because its components change, because its direction changes, or because the basis used to describe it changes.

A correct derivative must account for all three possibilities.

References

References

[1]   J. R. Taylor, Classical Mechanics, University Science Books, 2005.

[2]   J. B. Marion and S. T. Thornton, Classical Dynamics of Particles and Systems, 5th ed., Brooks/Cole, 2004.

[3]   H. Goldstein, C. Poole, and J. Safko, Classical Mechanics, 3rd ed., Addison-Wesley, 2002.

[4]   G. B. Arfken, H. J. Weber, and F. E. Harris, Mathematical Methods for Physicists, 7th ed., Academic Press, 2013.

[5]   M. L. Boas, Mathematical Methods in the Physical Sciences, 3rd ed., Wiley, 2006.


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 02. (Mathematical methods in physics)
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