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The electric potential at points in an \(x y\) plane is given by \(V=\left(2.0 \mathrm{~V} / \mathrm{m}^{2}\right) x^{2}-\left(3.0 \mathrm{~V} / \mathrm{m}^{2}\right) y^{2} .\) In unit-vector notation, what is the electric field at the point \((3.0 \mathrm{~m}, 2.0 \mathrm{~m})\) ?

Short Answer

Expert verified
\( \vec{E} = (-12.0 \hat{i} + 12.0 \hat{j}) \, \mathrm{V/m} \).

Step by step solution

01

Understanding the Problem

We need to find the electric field vector, denoted as \( \vec{E} \), at the specific point \( (3.0 \; \mathrm{m}, 2.0 \; \mathrm{m}) \) given the electric potential \( V = (2.0 \, \mathrm{V/m^2}) x^2 - (3.0 \, \mathrm{V/m^2}) y^2 \). The electric field can be found from the gradient of the potential, \( \vec{E} = -abla V \).
02

Compute the Partial Derivatives

To find the components of the electric field, compute the negative partial derivatives of the potential \( V \) with respect to \( x \) and \( y \). This gives us \( E_x = -\frac{\partial V}{\partial x} \) and \( E_y = -\frac{\partial V}{\partial y} \).
03

Calculate \( E_x \)

First, find the partial derivative of \( V \) with respect to \( x \): \, \( \frac{\partial V}{\partial x} = 2 \times (2.0) x = 4.0 x \). Evaluate at \( x = 3.0 \; \mathrm{m} \): \, \( \frac{\partial V}{\partial x} = 4.0 \times 3.0 = 12.0 \, \mathrm{V/m} \). Thus, \( E_x = -12.0 \, \mathrm{V/m} \).
04

Calculate \( E_y \)

Next, calculate the partial derivative of \( V \) with respect to \( y \): \, \( \frac{\partial V}{\partial y} = 2 \times (-3.0) y = -6.0 y \). Evaluate at \( y = 2.0 \; \mathrm{m} \): \, \( \frac{\partial V}{\partial y} = -6.0 \times 2.0 = -12.0 \, \mathrm{V/m} \). Thus, \( E_y = 12.0 \, \mathrm{V/m} \).
05

Formulate the Electric Field Vector

Combine \( E_x \) and \( E_y \) to express the electric field in unit-vector notation. Therefore, \( \vec{E} = (-12.0 \hat{i} + 12.0 \hat{j}) \, \mathrm{V/m} \).

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Electric Potential
Electric potential is a measure of the electric potential energy per unit charge at a specific point in space. In simpler words, it's like the height for electric charge - just as height determines potential energy for gravity, electric potential determines potential energy for electric forces.
In the given exercise, the electric potential is given by the equation \( V= (2.0 \, \mathrm{V/m^2}) x^2 - (3.0 \, \mathrm{V/m^2}) y^2 \).
This means that at any point \((x, y)\) on the plane, you can determine the electric potential by plugging in the \(x\) and \(y\) coordinates into the formula. The unit \(\mathrm{V/m^2}\) indicates the variation of potential with respect to distance squared.
The properties of this function show how electric potential varies within space and eventually, how it can influence electric field calculations.
Gradient of Potential
The gradient of a potential is a crucial concept because it helps us understand the direction and magnitude of the electric field derived from the potential.
The gradient of a scalar field, like electric potential \(V\), gives us a vector field, which in this case is the electric field \(\vec{E}\). Mathematically, this is expressed as \(\vec{E} = -abla V\), where \(abla\) (nabla) symbol denotes the gradient operator.
The negative sign indicates that the electric field points in the direction where the potential decreases the fastest. This corresponds to the natural behavior of charges moving from higher to lower potential regions, akin to objects falling downhill toward lower gravitational potential.
Partial Derivatives
Partial derivatives are mathematical tools used when we deal with functions of multiple variables. They let us see how the function changes as one variable changes, while keeping other variables constant.
In the context of this problem, our task is to compute partial derivatives of the potential \(V\) with respect to \(x\) and \(y\). These partial derivatives help find the components of the electric field.
For example:
  • For the x-component, compute \(E_x = -\frac{\partial V}{\partial x}\).
  • For the y-component, compute \(E_y = -\frac{\partial V}{\partial y}\).
By calculating these derivatives at specific points, you get the values of the electric field components at that location, revealing the influence each coordinate has on the electric field.
Unit-Vector Notation
Unit-vector notation is a compact and clear way to express vector quantities, like electric fields, by breaking them into direction components.
In our exercise, the electric field \(\vec{E}\) is expressed as \(\vec{E} = (-12.0 \hat{i} + 12.0 \hat{j}) \, \mathrm{V/m}\). Here:
  • \(\hat{i}\) is the unit vector in the x-direction (horizontal).
  • \(\hat{j}\) is the unit vector in the y-direction (vertical).
The numbers next to these unit vectors describe the magnitude of the electric field along each direction, providing a clear picture of how the field is oriented in space. This notation becomes immensely useful for vector addition and helps in visualizing directionality in multidimensional problems.

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Most popular questions from this chapter

A solid copper sphere whose radius is \(1.0 \mathrm{~cm}\) has a very thin surface coating of nickel. Some of the nickel atoms are radioactive, each atom emitting an electron as it decays. Half of these electrons enter the copper sphere, each depositing \(100 \mathrm{keV}\) of energy there. The other half of the electrons escape, each carrying away a charge \(-e\). The nickel coating has an activity of \(3.70 \times 10^{8}\) radioactive decays per second. The sphere is hung from a long, nonconducting string and isolated from its surroundings. (a) How long will it take for the potential of the sphere to increase by \(1000 \mathrm{~V} ?\) (b) How long will it take for the temperature of the sphere to increase by \(5.0 \mathrm{~K}\) due to the energy deposited by the electrons? The heat capacity of the sphere is \(14 . \mathrm{J} / \mathrm{K}\)

Two metal spheres, each of radius \(3.0 \mathrm{~cm}\), have a center-to-center separation of \(2.0 \mathrm{~m} .\) Sphere 1 has charge \(+1.0 \times\) \(10^{-8} \mathrm{C}\); sphere 2 has charge \(-3.0 \times 10^{-8} \mathrm{C}\). Assume that the separation is large enough for us to say that the charge on each sphere is uniformly distributed (the spheres do not affect each other). With \(V=0\) at infinity, calculate (a) the potential at the point halfway between the centers and the potential on the surface of (b) sphere 1 and \((\mathrm{c})\) sphere \(2 .\)

A solid conducting sphere of radius \(3.0 \mathrm{~cm}\) has a charge of \(30 \mathrm{nC}\) distributed uniformly over its surface. Let \(A\) be a point \(1.0 \mathrm{~cm}\) from the center of the sphere, \(S\) be a point on the surface of the sphere, and \(B\) be a point \(5.0 \mathrm{~cm}\) from the center of the sphere. What are the electric potential differences (a) \(V_{S}-V_{B}\) and (b) \(V_{A}-V_{B} ?\)

A particle of positive charge \(Q\) is fixed at point \(P .\) A second particle of mass \(m\) and negative charge \(-q\) moves at constant speed in a circle of radius \(r_{1}\), centered at \(P .\) Derive an expression for the work \(W\) that must be done by an external agent on the second particle to increase the radius of the circle of motion to \(r_{2}\).

A thick spherical shell of charge \(Q\) and uniform volume charge density \(\rho\) is bounded by radii \(r_{1}\) and \(r_{2}>r_{1} .\) With \(V=0\) at infinity, find the electric potential \(V\) as a function of distance \(r\) from the center of the distribution, considering regions (a) \(r>r_{2}\), (b) \(r_{2}>r>r_{1}\), and (c) \(r

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