Vector Fundamentals and Operations Notes

Vector fundamentals

  • In physics, a vector is an object that has both direction and magnitude, often shown as arrows. An arrow represents a vector pointing from the origin, with length equal to its magnitude and direction given by the angle from the x-axis. This is related to polar coordinates, where you might describe a vector by its radial distance $r$ and angle $\theta$, but we will describe vectors primarily by components.
  • A 2D vector is written as v=(v<em>x,v</em>y)\mathbf{v}=(v<em>x,\,v</em>y) where v<em>xv<em>x is the x-component and v</em>yv</em>y is the y-component. The arrow over a letter (e.g., v\vec{v} or v\mathbf{v}) denotes that the quantity is a vector, not a simple coordinate pair.
  • Examples of vectors in components:
    • If the vector is v=(3,2)\mathbf{v}=(3,\,2) then you go 3 units in +x and 2 units in +y from the origin.
    • If the vector is u=(1,4)\mathbf{u}=(1,4), drawn from the origin, it goes 1 in x and 4 in y.
  • The magnitude (length) of a vector is the length of its arrow, and the direction is the orientation of the arrow (the angle from the x-axis).
  • Distinctions in physics:
    • Vectors vs scalars: vectors have both magnitude and direction; scalars have magnitude only.
    • Examples: velocity, displacement, and acceleration are vectors; time, mass, and temperature are scalars.
  • Velocity is a vector; time is a scalar. Displacement is a vector describing change in position; distance is the magnitude of displacement (a scalar).
  • Velocity and acceleration definitions in vector form:
    • Velocity can be written as the change in displacement over time: v=ΔrΔt\mathbf{v}=\frac{\Delta \mathbf{r}}{\Delta t} or, in continuous form, v=drdt\mathbf{v}=\frac{d\mathbf{r}}{dt}.
    • Acceleration is the change in velocity over time: a=ΔvΔt=dvdt\mathbf{a}=\frac{\Delta \mathbf{v}}{\Delta t}=\frac{d\mathbf{v}}{dt}.
  • Displacement is the difference between final and initial positions: Δr=r<em>fr</em>i.\Delta \mathbf{r}=\mathbf{r}<em>f-\mathbf{r}</em>i\,. Distance is the magnitude of that displacement: distance=Δr\text{distance}=|\Delta \mathbf{r}|.
  • Time is a scalar: it does not have a direction. Expressions with time use scalar arithmetic.
  • Mass and temperature are scalars (e.g., 90 kg, 50 °C) and do not carry directional information.
  • When thinking about whether something is a vector, ask: does it have a direction? If yes, it’s a vector; if not, it’s a scalar.
  • In this course, the primary focus is on velocity, displacement, and acceleration as vectors, and on using scalars like time, mass, and temperature separately.
  • Conceptual takeaway: any math in physics is done with vectors and component-wise operations (i.e., break into x and y components and perform arithmetic on components).

Basic vector operations

  • Scalar multiplication
    • If you multiply a vector by a scalar cc, the result is the vector scaled along its direction: cv=(cv<em>x,cv</em>y)c\,\mathbf{v}=(c\,v<em>x,\,c\,v</em>y).
    • Examples:
    • If a=(1,4)\mathbf{a}=(1,4), then 3a=(3,12)3\mathbf{a}=(3,12).
    • If you multiply by a negative scalar, the vector flips direction: 1a=(v<em>x,v</em>y)-1\cdot\mathbf{a}=(-v<em>x,-v</em>y).
    • Multiples of a vector all lie on the same line through the origin.
  • Vector addition
    • For vectors u=(u<em>x,u</em>y)\mathbf{u}=(u<em>x, u</em>y) and v=(v<em>x,v</em>y)\mathbf{v}=(v<em>x, v</em>y), their sum is u+v=(u<em>x+v</em>x,u<em>y+v</em>y)\mathbf{u}+\mathbf{v}=(u<em>x+v</em>x,\,u<em>y+v</em>y).
    • Example: (1,4)+(3,2)=(4,6)(1,4)+(3,2)=(4,6).
    • Geometrically, you can add vectors using the tip-to-tail method or the parallelogram rule: placing the tail of one vector at the tip of the other yields the resultant vector as the diagonal of the parallelogram.
  • Subtraction
    • Subtraction is vector addition with a negative: uv=u+(v)\mathbf{u}-\mathbf{v}=\mathbf{u}+(-\mathbf{v}).
    • Example: (1,4)(3,2)=(2,2)(1,4) - (3,2) = (-2,2).
    • The opposite vector (negative) points in the exact opposite direction; subtracting changes signs of the components.
  • Important caveat about multiplication
    • There is no general product of two vectors that yields a vector in the same simple sense. The transcript emphasizes that you should not expect to multiply two vectors in the same way you multiply scalars; there are specific products (like dot or cross products) but not a universal vector multiplication rule.
  • Practical note for physics problem-solving
    • Always work with vector components (x and y) and perform component-wise arithmetic.
    • When summing or subtracting, track both components; the resultant vector is formed by adding/subtracting corresponding components.

Geometric interpretation and visualization

  • Tip-to-tail visualization (parallelogram rule) helps you see how addition works graphically.
  • Subtraction corresponds to adding the opposite vector, which flips direction.
  • Graphical intuition is useful for understanding direction and how the resultant vector behaves in planes like the x-y plane.
  • In physics problems, the pictures are often approximations; the algebra on components is what gives you precise results.

Velocity, displacement, and acceleration: physics context

  • Vector vs scalar in a physics equation:
    • Velocity, displacement, and acceleration are vectors (have arrows over them).
    • Time is a scalar (no arrow).
    • Mass and temperature are scalars.
  • Core relationships:
    • Velocity is the rate of change of displacement: v=drdt\mathbf{v}=\frac{d\mathbf{r}}{dt} and, for discrete changes, v=ΔrΔt\mathbf{v}=\frac{\Delta \mathbf{r}}{\Delta t}.
    • Acceleration is the rate of change of velocity: a=dvdt\mathbf{a}=\frac{d\mathbf{v}}{dt} and, for discrete changes, a=ΔvΔt\mathbf{a}=\frac{\Delta \mathbf{v}}{\Delta t}.
  • Signs and directions matter: components can be positive or negative, indicating direction along each axis.
  • Common scalar examples (for contrast): time tt, mass mm, temperature (e.g., 50 °C) are scalars; they do not specify a direction.
  • When analyzing equations, identify which quantities are vectors and perform operations component-wise.

Example problem: acceleration from velocity data

  • Given a velocity final v<em>f=(1,5)\mathbf{v}<em>f=(1,5), a velocity initial v</em>i=(2,6)\mathbf{v}</em>i=(2,6), and a time interval t=67t=67, find the acceleration a\mathbf{a}.
  • Start from the velocity-time relation: v<em>f=v</em>i+at\mathbf{v}<em>f = \mathbf{v}</em>i + \mathbf{a} t.
  • Solve for the acceleration: subtract the initial velocity and divide by time:
    • a=v<em>fv</em>it=(1,5)(2,6)67=(167,167).\mathbf{a} = \frac{\mathbf{v}<em>f - \mathbf{v}</em>i}{t} = \frac{(1,5)-(2,6)}{67} = \left(-\frac{1}{67},\,-\frac{1}{67}\right).
  • Magnitude of acceleration:
    • a=(167)2+(167)2=(1672)+(1672)=2672=2670.0211.|\mathbf{a}| = \sqrt{\left(-\frac{1}{67}\right)^2 + \left(-\frac{1}{67}\right)^2} = \sqrt{\left(\frac{1}{67^2}\right) + \left(\frac{1}{67^2}\right)} = \sqrt{\frac{2}{67^2}} = \frac{\sqrt{2}}{67} \approx 0.0211.
  • Direction of acceleration:
    • Since both components are negative and equal, the vector lies along the line $y=x$ in the third quadrant. The angle from the +x axis is
    • θ=π+π4=5π4\theta = \pi + \frac{\pi}{4} = \frac{5\pi}{4} (or equivalently, $-135^{\circ}$).
  • Note on the transcript’s numeric value: the speaker stated the magnitude as approximately $1.113\times 10^{-4}$, which is inconsistent with the computed magnitude above. The correct magnitude is about a0.0211.|\mathbf{a}| \approx 0.0211. The exact symbolic form is a=267.|\mathbf{a}| = \dfrac{\sqrt{2}}{67}.
  • Summary: the acceleration vector is a=(167,167)\mathbf{a}=\left(-\frac{1}{67},\,-\frac{1}{67}\right) with magnitude a=2670.0211|\mathbf{a}|=\dfrac{\sqrt{2}}{67} \approx 0.0211 and direction in the third quadrant (angle 5π4\frac{5\pi}{4} from +x or -135°).
  • The absolute length notation for magnitude is often shown with double vertical lines around a number or vector; symbolically, the magnitude is a scalar value (the length of the arrow).
  • Final practical point: break vectors into components and use component-wise arithmetic to solve problems; this helps you determine both magnitude and direction of the resultant vector.

Quick recap: key distinctions and rules

  • Vector vs scalar:
    • Vectors have magnitude and direction; scalars have magnitude only.
    • Examples: vector\text{vector}: v,r,a\mathbf{v}, \mathbf{r}, \mathbf{a}; scalar\text{scalar}: t,m,Tt, m, T.
  • Operations on vectors:
    • Scalar multiplication: cv=(cv<em>x,cv</em>y)c\,\mathbf{v}=(c\,v<em>x, c\,v</em>y).
    • Vector addition: u+v=(u<em>x+v</em>x,u<em>y+v</em>y)\mathbf{u}+\mathbf{v}=(u<em>x+v</em>x, u<em>y+v</em>y).
    • Subtraction: uv=u+(v)=(u<em>xv</em>x,u<em>yv</em>y)\mathbf{u}-\mathbf{v}=\mathbf{u}+(-\mathbf{v}) = (u<em>x-v</em>x, u<em>y-v</em>y).
    • No general vector multiplication (there are specific products like dot and cross products, but no universal vector multiplication rule).
  • Practical habit: always use components for algebra in physics problems; this keeps direction and magnitude clear and helps with subsequent steps like rotations or decompositions.
  • In physics problems, be mindful of units (e.g., meters per second for velocity, meters per second squared for acceleration); magnitudes often come with units, and mixing units can lead to mistakes.
  • Course logistics mentioned in the transcript (not concepts): daily notes, link to a PDF with course notes, and posting homework problems from the textbook on the course homepage under Resources.