Question #50819

A)A sphere of radius R carries a charge of volume charge density p = cr, where c is a constant and r denotes the distance from the centre of the sphere. Calculate the total charge enclosed by the sphere and the electric field at points lying inside and outside the sphere. B) A dielectric object is placed in an electric field. The object becomes polarised and a large number of atomic /molecular dipoles in the object align in the direction of the applied electric field. Derive an expression for the electric field produced by this polarised dielectric at a point outside the dielectric object. C)Determine the magnitude of the pointing vector and the energy per unit time delivered to a wire of length L and cross-section A when electric current I flows in it.
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Expert's answer

2015-02-20T08:19:07-0500

Answer on Question #50819-Physics-Electromagnetism

A) A sphere of radius R carries a charge of volume charge density p=crp = cr , where c is a constant and r denotes the distance from the center of the sphere. Calculate the total charge enclosed by the sphere and the electric field at points lying inside and outside the sphere.

B) A dielectric object is placed in an electric field. The object becomes polarized and a large number of atomic /molecular dipoles in the object align in the direction of the applied electric field. Derive an expression for the electric field produced by this polarized dielectric at a point outside the dielectric object.

C) Determine the magnitude of the pointing vector and the energy per unit time delivered to a wire of length L and cross-section A when electric current I flows in it.

Solution

A) The total charge enclosed by the sphere is


Q=02πdφ0πsinθdθ0R(cr)r2dr=2π2cR44=πcR4.Q = \int_ {0} ^ {2 \pi} d \varphi \int_ {0} ^ {\pi} \sin \theta d \theta \int_ {0} ^ {R} (c r) r ^ {2} d r = 2 \pi \cdot 2 \cdot \frac {c R ^ {4}}{4} = \pi c R ^ {4}.


The electric field outside a charged, spherical, conducting shell is the same as that generated when all the charge is concentrated at the center of the shell. Thus, the electric field at the distance rr outside the sphere is


E=14πε0Qr2=c4ε0R4r2.E = \frac {1}{4 \pi \varepsilon_ {0}} \frac {Q}{r ^ {2}} = \frac {c}{4 \varepsilon_ {0}} \frac {R ^ {4}}{r ^ {2}}.


Applying Gauss's law at distances r<Rr < R we get


4πr2E=1ε002πdφ0πsinθdθ0R(cr)r2dr=1ε0πcr4.4 \pi r ^ {2} E = \frac {1}{\varepsilon_ {0}} \int_ {0} ^ {2 \pi} d \varphi \int_ {0} ^ {\pi} \sin \theta d \theta \int_ {0} ^ {R} (c r) r ^ {2} d r = \frac {1}{\varepsilon_ {0}} \pi c r ^ {4}.


The electric field at the distance rr inside the sphere is


E=c4ε0r2.E = \frac {c}{4 \varepsilon_ {0}} r ^ {2}.


B) In the presence of an electric field, a dielectric becomes polarized and acquires a dipole moment PP , per unit volume. The aim is to calculate field at point rr [denoted by Q(r)Q(r') in Fig. outside the dielectric. Let the volume of the dielectric is divided into small elementary volumes and



consider one such volume element dV\mathrm{dV} of the dielectric. The potential due to dielectric body occupying volume dV\mathrm{dV} as observed outside dV\mathrm{dV} for single dipole potential can be expressed as,


ϕ(r)=14πε0VP(r).(rr)(rr)2dV\phi \left(r ^ {\prime}\right) = \frac {1}{4 \pi \varepsilon_ {0}} \int_ {V} \frac {P (r) . (r - r ^ {\prime})}{\left| (r - r ^ {\prime}) \right| ^ {2}} d Vϕ(r)=14πε0VP(r).(rr)(rr)dV(rr)2\phi \left(r ^ {\prime}\right) = \frac {1}{4 \pi \varepsilon_ {0}} \int_ {V} \frac {P (r) . \frac {(r - r ^ {\prime})}{\left| (r - r ^ {\prime}) \right|} d V}{\left| (r - r ^ {\prime}) \right| ^ {2}}ϕ(r)=14πε0VP(r).(rr)0(rr)2dV\phi \left(r ^ {\prime}\right) = \frac {1}{4 \pi \varepsilon_ {0}} \int_ {V} \frac {P (r) . (r - r ^ {\prime}) ^ {0}}{\left| (r - r ^ {\prime}) \right| ^ {2}} d V


where (rr)0(\mathbf{r} - \mathbf{r}^{\prime})0 represents unit vector directed from Q towards dV. It is obviously equal to


(xx)i+(yy)j+(zz)k(xx)2+(yy)2+(zz)2\frac {\left(x ^ {\prime} - x\right) i + \left(y ^ {\prime} - y\right) j + \left(z ^ {\prime} - z\right) k}{\sqrt {\left| \left(x ^ {\prime} - x\right) ^ {2} + \left(y ^ {\prime} - y\right) ^ {2} + \left(z ^ {\prime} - z\right) ^ {2} \right|}}


where x,y,zx', y', z' are the Cartesian coordinates of point rr' and (x,y,z)(x, y, z) those at rr . Further,


(rr)0=[ix(rr)+jx(rr)+kx(rr)]\left(r - r ^ {\prime}\right) ^ {0} = - \left[ i \frac {\partial}{\partial x} \left(r - r ^ {\prime}\right) + j \frac {\partial}{\partial x} \left(r - r ^ {\prime}\right) + k \frac {\partial}{\partial x} \left(r - r ^ {\prime}\right) \right]P(r)=iPx(x.y.z)+jPy(x.y.z)+kPz(x.y.z)P (r) = i P _ {x} (x. y. z) + j P _ {y} (x. y. z) + k P _ {z} (x. y. z)


substituting these values in equation, we get


ϕ(r)=14πε0{VPx(rr)2x(rr)dV+VPy(rr)2y(rr)dV+VPz(rr)2z(rr)dV}=ϕ1+ϕ2+ϕ3\begin{array}{l} \phi \left(r ^ {\prime}\right) = \frac {1}{4 \pi \varepsilon_ {0}} \left\{\int_ {V} \frac {P _ {x}}{\left(r - r ^ {\prime}\right) ^ {2}} \frac {\partial}{\partial x} \left(r - r ^ {\prime}\right) d V + \int_ {V} \frac {P _ {y}}{\left(r - r ^ {\prime}\right) ^ {2}} \frac {\partial}{\partial y} \left(r - r ^ {\prime}\right) d V + \int_ {V} \frac {P _ {z}}{\left(r - r ^ {\prime}\right) ^ {2}} \frac {\partial}{\partial z} \left(r - r ^ {\prime}\right) d V \right\} \\ = \phi_ {1} + \phi_ {2} + \phi_ {3} \\ \end{array}


Now we shall consider the integrals separately. It is obvious that


1(rr)2(rr)x=x1(rr)2- \frac {1}{\left| (r - r ^ {\prime}) \right| ^ {2}} \frac {\partial (r - r ^ {\prime})}{\partial x} = \frac {\partial}{\partial x} \frac {1}{\left| (r - r ^ {\prime}) \right| ^ {2}}dV=dxdydzd V = d x d y d z


Therefore


ϕ1=14πε0Pxx1(rr)2dxdydz\phi_ {1} = \frac {1}{4 \pi \varepsilon_ {0}} \iiint P _ {x} \frac {\partial}{\partial x} \frac {1}{\left| (r - r ^ {\prime}) \right| ^ {2}} d x d y d z


After integration we get


ϕ(r)=14πεsP.n(rr)dA14πεr(divP)dV(rr)\phi (r ^ {\prime}) = \frac {1}{4 \pi \varepsilon_ {\circ}} \int_ {s} \frac {\mathbf {P} . n}{| (r - r ^ {\prime}) |} d A - \frac {1}{4 \pi \varepsilon_ {\circ}} \int_ {r} \frac {(- d i v P) d V}{| (r - r ^ {\prime}) |}


Equation obviously shows that the potential at point rr' due to dielectric body is the same as if it were replaced by a system of bound charges in empty space. A part of these bound charges appears on the dielectric surfaces as a surface density δP\delta P' given by


σP=P.n\sigma_ {\mathrm {P}} ^ {\prime} = \mathrm {P . n}


while the remaining bound charge appears throughout the volume VV as a volume density rprp' given as


ρP=(Pxx+Pyy+Pzz)\rho_ {P} ^ {\prime} = - \left(\frac {\partial P _ {x}}{\partial x} + \frac {\partial P _ {y}}{\partial y} + \frac {\partial P _ {z}}{\partial z}\right)


The intensity of electric field due to the polarized volume may be expressed as


E(r)=14πε[sσP(rr)rr3dA+rρP(rr)rr3dV]E \left(r ^ {\prime}\right) = \frac {1}{4 \pi \varepsilon_ {\circ}} \left[ \int_ {s} \frac {\sigma_ {P} ^ {\prime} \left(r - r ^ {\prime}\right)}{\left| r - r ^ {\prime} \right| ^ {3}} d A + \int_ {r} \frac {\rho_ {P} ^ {\prime} \left(r - r ^ {\prime}\right)}{\left| r - r ^ {\prime} \right| ^ {3}} d V \right]


C) We choose unit vectors as shown in the figure below



There is an electric potential difference across the resistor that is equal to ΔV=IR\Delta V = IR. The electric field is uniform in the resistor so ΔV=Eds=EL=IR|\Delta V| = \left|\int \vec{E} d\vec{s}\right| = EL = IR. Therefore the direction and magnitude of the electric field is given by


E=IRLk^.\vec {E} = \frac {I R}{L} \hat {k}.


We can use Ampere's Law to find the magnetic field surface of the resistor. Choose a circular loop as shown in the figure of radius =a= a.



Ampere's law is


circleBds=μ0diskJnda.\oint_ {c i r c l e} \vec {B} d \vec {s} = \mu_ {0} \iint_ {d i s k} \vec {J} \vec {n} d a.


By symmetry,


circleBds=B2πa.\oint_{circle} \vec{B} \, d\vec{s} = B2\pi a.


The current through the disk is


diskfnda=I.\iint_{disk} \vec{f} \, \vec{n} \, da = I.


So Ampere's Law becomes


B2πa=μ0I.B2\pi a = \mu_0 I.


With our choice of unit vectors, the direction and magnitude of the magnetic field on the surface of the resistor is


B=μ0I2πaθ^.\vec{B} = \frac{\mu_0 I}{2\pi a} \hat{\theta}.


The Poynting vector is given by


S=E×Bμ0=(IRLk^)×(μ0I2πaθ^)μ0=IRLI2πa(r^)\vec{S} = \frac{\vec{E} \times \vec{B}}{\mu_0} = \frac{\left(\frac{IR}{L} \hat{k}\right) \times \left(\frac{\mu_0 I}{2\pi a} \hat{\theta}\right)}{\mu_0} = \frac{IR}{L} \frac{I}{2\pi a} (-\hat{r})


In order to calculate the power flow into the resistor we need to calculate the closed surface flux of the Poynting vector over the surface of the resistor.



Because the Poynting vector points radially inward we only calculate the flux over the cylindrical body of the resistor. Hence we set r=ar = a for Poynting vector and then integrate it over the outside cylindrical area of the resistor. For a closed surface we choose n^out=r^\hat{n}_{out} = \hat{r} and so Sr^=S\vec{S} \hat{r} = -|\vec{S}|.


Power=Sn^outda=cylinderSr^da=cylinderSda=S(r=a)A.Power = \oint \vec{S} \, \hat{n}_{out} \, da = \iint_{cylinder} \vec{S} \hat{r} \, da = - \iint_{cylinder} |\vec{S}| \, da = - |\vec{S}(r = a)| \, A.


The surface area in question is =2πaL= 2\pi aL. Thus using our result for the magnitude of the Poynting vector we have that the power flow through the surface is


Power=(IRLI2πa)2πaL=I2R.Power = - \left(\frac{IR}{L} \frac{I}{2\pi a}\right) 2\pi aL = -I^2 R.


The negative sign indicates that power is flowing into the resistor. We know that the rate that work is done by the electric field in the wire is I2RI^2 R so our answer makes because energy per sec flows in and is equal to the rate that work is done on the charges in the wire. This energy is dissipated in the form of random thermal motion due to collisions in the wire and eventually is transmitted to the motion of the air molecules surrounding the wire.

The energy per unit time delivered to a wire is


P=I2R.P = I ^ {2} R.


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