The torque on a magnetic dipole is $\tau=mB\sin\theta$. Hence $m=\tau/(B\sin\theta)=4.5\times10^{-2}/[0.25\sin30^\circ]=0.36\,\text{J T}^{-1}$.
$0.36\,\text{J T}^{-1}$.
Potential energy of a magnetic dipole in a field is $U=-\mathbf{m}\cdot\mathbf{B}=-mB\cos\theta$. For stable equilibrium, $\theta=0^\circ$, so $U=-mB=-(0.32)(0.15)=-4.8\times10^{-2}\,\text{J}$. For unstable equilibrium, $\theta=180^\circ$, so $U=+mB=+4.8\times10^{-2}\,\text{J}$.
(a) Stable equilibrium occurs when $\mathbf{m}$ is parallel to $\mathbf{B}$; $U=-4.8\times10^{-2}\,\text{J}$. (b) Unstable equilibrium occurs when $\mathbf{m}$ is antiparallel to $\mathbf{B}$; $U=+4.8\times10^{-2}\,\text{J}$.
A current-carrying solenoid produces a magnetic field similar to that of a bar magnet: one end behaves as a north pole and the other as a south pole, with field lines forming closed loops. The magnetic moment is $m=NIA=800(3.0)(2.5\times10^{-4})=0.60\,\text{A m}^2$.
The solenoid behaves like a bar magnet with north and south poles at its ends; its magnetic moment is $0.60\,\text{A m}^2$.
Potential energy is $U=-mB\cos\theta$. Initially, $\theta=0^\circ$, so $U_i=-mB=-(1.5)(0.22)=-0.33\,\text{J}$. For normal alignment, $\theta=90^\circ$, $U=0$, so work required is $0-(-0.33)=0.33\,\text{J}$. For opposite alignment, $\theta=180^\circ$, $U=+0.33\,\text{J}$, so work required is $0.33-(-0.33)=0.66\,\text{J}$. Torque magnitude is $mB\sin\theta$; it is $0.33\,\text{N m}$ at $90^\circ$ and zero at $180^\circ$.
(a) Work required is $0.33\,\text{J}$ for normal alignment and $0.66\,\text{J}$ for opposite alignment. (b) Torque is $0.33\,\text{N m}$ in case (i) and zero in case (ii).
Magnetic moment is $m=NIA=2000(4.0)(1.6\times10^{-4})=1.28\,\text{A m}^2$. A magnetic dipole in a uniform magnetic field experiences no net force. The torque is $\tau=mB\sin\theta=1.28(7.5\times10^{-2})\sin30^\circ=4.8\times10^{-2}\,\text{N m}$.
(a) $1.28\,\text{A m}^2$. (b) Net force is zero; torque is $4.8\times10^{-2}\,\text{N m}$.
For a short magnet, axial field is $B_a=(\mu_0/4\pi)(2m/r^3)$ and equatorial field has magnitude $B_e=(\mu_0/4\pi)(m/r^3)$, directed opposite to $\mathbf{m}$. With $m=0.48\,\text{J T}^{-1}$ and $r=0.10\,\text{m}$, $B_a=10^{-7}(0.96)/(10^{-3})=9.6\times10^{-5}\,\text{T}$ and $B_e=10^{-7}(0.48)/(10^{-3})=4.8\times10^{-5}\,\text{T}$.
(a) $9.6\times10^{-5}\,\text{T}$ along the magnetic moment on the axis. (b) $4.8\times10^{-5}\,\text{T}$ opposite to the magnetic moment on the equatorial line.