- #1
Joshua Benabou
An interesting problem posed to me by a friend:
A small sphere, initially neutral, of radius ##a## emits ##n## charges ##q## of mass ##m## per unit time isotropically from its surface at a radial velocity of constant norm ##v##.
Determine the spatial distribution of charges and currents at time ##t##.
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Qualitative Analysis:
- The charge density and current density will be spherically symmetric.
- The magnetic field produced by a spherically symmetric current density is zero (classic)
- without loss of generality we may assume that ##q>0##. Assuming the mechanism by which the charges are radiated respects the conservation of charge, the radiating sphere will develop an increasing negative charge
- any electric field generated by the charge distribution will be directed radially and will be spherically symmetric.
- At any point in time ##t##, we can draw a ball of some minimal radius ##R(t)>a## enclosing all of the charges. At a distance ##r>R(t)##, the E field will be zero by Gauss's law (since the charge enclosed is zero). For ##a<r<R(t)##, the charge enclosed will necessarily be negative, thus the E field will be directed towards the origin, meaning charges will feel a force pulling them back towards the origin. So we might be end up with some periodic motion...
- Note that if we don't assume that the radiation mechanism conserves charge (e.g the charges are being somehow injected from the exterior into the sphere and then radiated away), we could end up with a potentially simpler problem, because enclosed charge in any Gaussian sphere of radius ##r>a## will always be positive, and thus the electric field will be directed away from origin, tending to accelerate the charges away from the origin.
- the acceleration of the charges in turn affects the charge distribution, so there will be some differential equation to solve
Quantitative Analysis:
Let ##Q(r)## be the charge contained within a sphere centered at the origin of radius ##r## (note that ##Q(r)## is time dependent).
Gauss's law gives: ##E(r)=Q(r)/(4 \pi \epsilon_0r^2)##
Hence the acceleration on a charge ##q## is ##a(r)=qQ(r)/(4 \pi \epsilon_0 mr^2)##.
By conservation of charge we also have that the charge density (which is spherically symmetric) is given by ##j(r)=-\partial Q(r)/\partial t##. We also have that ##j(r)=v(r)\rho(r)## where ##v## is the signed speed of a charge at a distance ##r##.
Finally by defintion ##\rho(r)=\frac{dQ(r)}{dr}\frac{1}{4\pi r^2}##.
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In principle the above equations should be enough to solve for ##Q(r)## and thus ##j(r)##. But I got some complicated partial differential equation involving second derivatives of ##Q(r)## with respect to ##r## and ##t##, which didn't lead me very far. Also I'm not sure whether to assume the radiation mechanism conserves charge or not.
A small sphere, initially neutral, of radius ##a## emits ##n## charges ##q## of mass ##m## per unit time isotropically from its surface at a radial velocity of constant norm ##v##.
Determine the spatial distribution of charges and currents at time ##t##.
-------------------------------------
Qualitative Analysis:
- The charge density and current density will be spherically symmetric.
- The magnetic field produced by a spherically symmetric current density is zero (classic)
- without loss of generality we may assume that ##q>0##. Assuming the mechanism by which the charges are radiated respects the conservation of charge, the radiating sphere will develop an increasing negative charge
- any electric field generated by the charge distribution will be directed radially and will be spherically symmetric.
- At any point in time ##t##, we can draw a ball of some minimal radius ##R(t)>a## enclosing all of the charges. At a distance ##r>R(t)##, the E field will be zero by Gauss's law (since the charge enclosed is zero). For ##a<r<R(t)##, the charge enclosed will necessarily be negative, thus the E field will be directed towards the origin, meaning charges will feel a force pulling them back towards the origin. So we might be end up with some periodic motion...
- Note that if we don't assume that the radiation mechanism conserves charge (e.g the charges are being somehow injected from the exterior into the sphere and then radiated away), we could end up with a potentially simpler problem, because enclosed charge in any Gaussian sphere of radius ##r>a## will always be positive, and thus the electric field will be directed away from origin, tending to accelerate the charges away from the origin.
- the acceleration of the charges in turn affects the charge distribution, so there will be some differential equation to solve
Quantitative Analysis:
Let ##Q(r)## be the charge contained within a sphere centered at the origin of radius ##r## (note that ##Q(r)## is time dependent).
Gauss's law gives: ##E(r)=Q(r)/(4 \pi \epsilon_0r^2)##
Hence the acceleration on a charge ##q## is ##a(r)=qQ(r)/(4 \pi \epsilon_0 mr^2)##.
By conservation of charge we also have that the charge density (which is spherically symmetric) is given by ##j(r)=-\partial Q(r)/\partial t##. We also have that ##j(r)=v(r)\rho(r)## where ##v## is the signed speed of a charge at a distance ##r##.
Finally by defintion ##\rho(r)=\frac{dQ(r)}{dr}\frac{1}{4\pi r^2}##.
-----------------------------
In principle the above equations should be enough to solve for ##Q(r)## and thus ##j(r)##. But I got some complicated partial differential equation involving second derivatives of ##Q(r)## with respect to ##r## and ##t##, which didn't lead me very far. Also I'm not sure whether to assume the radiation mechanism conserves charge or not.
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