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Find the charged enclosed by a sphere of charge density ρ and radius a.
To find the charge enclosed by a sphere of charge density ρ and radius a, you can use the formula for the charge, which is given by:[ Q = rho cdot V ]where ( V ) is the volume of the sphere. The volume ( V ) of a sphere is calculated using the formula:[ V = frac{4}{3} pi r^3 ]Substituting the radiusRead more
To find the charge enclosed by a sphere of charge density ρ and radius a, you can use the formula for the charge, which is given by:
[ Q = rho cdot V ]
where ( V ) is the volume of the sphere. The volume ( V ) of a sphere is calculated using the formula:
[ V = frac{4}{3} pi r^3 ]
Substituting the radius ( a ) into the volume formula gives:
[ V = frac{4}{3} pi a^3 ]
Therefore, the total charge ( Q ) enclosed within the sphere is:
[ Q = rho cdot frac{4}{3} pi a^3 ]
So, the charge enclosed by the sphere is:
[ Q = frac{4}{3} pi rho a^3 ]
See lessThe volume integral is three dimensional. State True/False
True.
True.
See lessThe triple integral is used to compute volume. State True/False
True.
True.
See lessIf D = 2xy i + 3yz j + 4xz k, how much flux passes through x = 3 plane for which -1<y<2 and 0<z<4?
To find the flux ( Phi ) of the vector field ( D = 2xy hat{i} + 3yz hat{j} + 4xz hat{k} ) through the plane ( x = 3 ), we can use the formula for flux:[Phi = iint_S mathbf{D} cdot mathbf{n} , dS]where ( mathbf{n} ) is the outward normal vector to the surface ( S ), and ( dS ) is the differential areRead more
To find the flux ( Phi ) of the vector field ( D = 2xy hat{i} + 3yz hat{j} + 4xz hat{k} ) through the plane ( x = 3 ), we can use the formula for flux:
[
Phi = iint_S mathbf{D} cdot mathbf{n} , dS
]
where ( mathbf{n} ) is the outward normal vector to the surface ( S ), and ( dS ) is the differential area element.
1. Identify the normal vector: For the plane ( x = 3 ), the outward normal vector is ( mathbf{n} = hat{i} ).
2. Evaluate the vector field on the plane: Since we are considering the plane where ( x = 3 ), we substitute ( x = 3 ) into the vector field ( D ):
[
D = 2(3)y hat{i} + 3yz hat{j} + 4(3)z hat{k} = 6y hat{i} + 3yz hat{j} + 12z hat{k}
]
3. Take the dot product with the normal vector:
[
mathbf{D} cdot mathbf{n} = (6y hat
See lessFind the value of divergence theorem for the field D = 2xy i + x2 j for the rectangular parallelepiped given by x = 0 and 1, y = 0 and 2, z = 0 and 3.
To apply the Divergence Theorem, we first need to compute the divergence of the vector field ( mathbf{D} = 2xy mathbf{i} + x^2 mathbf{j} ).The divergence of a vector field ( mathbf{D} = P mathbf{i} + Q mathbf{j} + R mathbf{k} ) is given by:[nabla cdot mathbf{D} = frac{partial P}{partial x} + frac{paRead more
To apply the Divergence Theorem, we first need to compute the divergence of the vector field ( mathbf{D} = 2xy mathbf{i} + x^2 mathbf{j} ).
The divergence of a vector field ( mathbf{D} = P mathbf{i} + Q mathbf{j} + R mathbf{k} ) is given by:
[
nabla cdot mathbf{D} = frac{partial P}{partial x} + frac{partial Q}{partial y} + frac{partial R}{partial z}
]
For our vector field ( mathbf{D} ):
– ( P = 2xy )
– ( Q = x^2 )
– ( R = 0 )
Now we compute the partial derivatives:
1. ( frac{partial P}{partial x} = frac{partial (2xy)}{partial x} = 2y )
2. ( frac{partial Q}{partial y} = frac{partial (x^2)}{partial y} = 0 )
3. ( frac{partial R}{partial z} = frac{partial (0)}{partial z} = 0 )
Thus, the divergence is:
[
nabla cdot mathbf{D} = 2y + 0 + 0 = 2y
See lessFind the value of divergence theorem for A = xy2 i + y3 j + y2z k for a cuboid given by 0<x<1, 0<y<1 and 0<z<1.
To apply the divergence theorem, we first need to compute the divergence of the vector field ( mathbf{A} = xy^2 mathbf{i} + y^3 mathbf{j} + y^2z mathbf{k} ).The divergence ( nabla cdot mathbf{A} ) is given by:[nabla cdot mathbf{A} = frac{partial (xy^2)}{partial x} + frac{partial (y^3)}{partial y} +Read more
To apply the divergence theorem, we first need to compute the divergence of the vector field ( mathbf{A} = xy^2 mathbf{i} + y^3 mathbf{j} + y^2z mathbf{k} ).
The divergence ( nabla cdot mathbf{A} ) is given by:
[
nabla cdot mathbf{A} = frac{partial (xy^2)}{partial x} + frac{partial (y^3)}{partial y} + frac{partial (y^2z)}{partial z}
]
Calculating each term individually:
1. ( frac{partial (xy^2)}{partial x} = y^2 )
2. ( frac{partial (y^3)}{partial y} = 3y^2 )
3. ( frac{partial (y^2z)}{partial z} = y^2 )
Adding these together, we get:
[
nabla cdot mathbf{A} = y^2 + 3y^2 + y^2 = 5y^2
]
Next, to apply the divergence theorem, we need to integrate the divergence over the volume of the cuboid defined by ( 0 < x < 1 ), ( 0 < y < 1 ), and ( 0 < z < 1 ):
See lessCompute divergence theorem for D= 5r2 /4 i in spherical coordinates between r=1 and r=2.
To compute the divergence theorem for the vector field ( mathbf{D} = frac{5r^2}{4} mathbf{i} ) in spherical coordinates between ( r = 1 ) and ( r = 2 ), we follow these steps: 1. Convert the Vector Field to Spherical Coordinates:In spherical coordinates, the relationship to Cartesian coordinates isRead more
To compute the divergence theorem for the vector field ( mathbf{D} = frac{5r^2}{4} mathbf{i} ) in spherical coordinates between ( r = 1 ) and ( r = 2 ), we follow these steps:
1. Convert the Vector Field to Spherical Coordinates:
In spherical coordinates, the relationship to Cartesian coordinates is given by:
– ( x = r sin theta cos phi )
– ( y = r sin theta sin phi )
– ( z = r cos theta )
The vector ( mathbf{i} ) represents the unit vector in the x-direction, so we express ( mathbf{D} ) as:
[
mathbf{D} = frac{5r^2}{4} mathbf{i} = frac{5r^2}{4} ( sin theta cos phi , sin theta sin phi , cos theta )
]
2. Compute the Divergence:
The divergence in spherical coordinates for a vector field ( mathbf{D} = (D_r, D_theta, D_phi) ) is given by:
[
nabla cdot mathbf{D} = frac{1}{r^2} frac{partial}{partial
See lessThe decimal code of Interpret as Command (IAC) character is _______
255
255
See lessCompute the Gauss law for D= 10ρ3 /4 i, in cylindrical coordinates with ρ= 4m, z=0 and z=5.
To compute Gauss's Law using the displacement field D, we first write down Gauss’s Law for electric displacement fields:[Phi_D = oint_S mathbf{D} cdot dmathbf{A} = Q_{free}]Where Q_free is the free charge enclosed by the surface S. Here, the displacement field is given as:[mathbf{D} = frac{10rho^3}{Read more
To compute Gauss’s Law using the displacement field D, we first write down Gauss’s Law for electric displacement fields:
[
Phi_D = oint_S mathbf{D} cdot dmathbf{A} = Q_{free}
]
Where Q_free is the free charge enclosed by the surface S. Here, the displacement field is given as:
[
mathbf{D} = frac{10rho^3}{4} mathbf{i}
]
In cylindrical coordinates, D can be expressed as a function of ρ, and given constants indicate that D has only an i component (along the x-axis).
Given:
– ρ = 4 m
– z = 0 (which we could consider as the bottom face of a cylindrical volume)
– z = 5 (top face of the volume)
1. Calculate D at ρ = 4 m:
[
mathbf{D} = frac{10(4)^3}{4} mathbf{i} = frac{10 times 64}{4} mathbf{i} = 160 mathbf{i}
]
2. Define the Gaussian surface: A cylinder with radius 4 m and height 5 m.
3. Calculate the area vector: The enclosed area of the Gaussian surface includes the curved surface and two flat circular areas.
– Curved surface area
See lessCoulomb’s law can be derived from Gauss law. State True/ False
True
True
See less