The principle of conservation of momentum and conservation of energy is applied to solve the problem.
The total initial momentum is equal to the total final momentum, and the total initial energy is equal to the total final energy.
Let the kinetic energy of \( {}^{17}_{8}O \) be \( K_{{}^{17}_{8}O} \). From conservation of momentum, the momentum of the particles is related to their kinetic energy \( K \) as:
\[ p = \sqrt{2mK} \]
where \( m \) is the mass of the particle.
For \( {}^{17}_{8}O \) and \( {}^{1}_{1}H \), the relationship between their momenta can be written as:
\[ p_{{}^{17}_{8}O} = - p_{{}^{1}_{1}H} \]
The total kinetic energy is given as:
\[ K_{\text{total}} = K_{{}^{4}_{2}He} + K_{{}^{14}_{7}N} = K_{{}^{17}_{8}O} + K_{{}^{1}_{1}H} \]
Substituting the given values:
\[ 5.314 + 0 = K_{{}^{17}_{8}O} + 4.012 \]
Solving for \( K_{{}^{17}_{8}O} \):
\[ K_{{}^{17}_{8}O} = 5.314 - 4.012 = 1.302 \text{ MeV} \]
The masses of the particles influence the kinetic energy distribution. Using the mass ratio correction:
\[ K_{{}^{17}_{8}O} = \frac{m_{{}^{1}_{1}H}}{m_{{}^{17}_{8}O}} K_{{}^{1}_{1}H} \]
Substituting \( m_{{}^{1}_{1}H} = 1.008u \) and \( m_{{}^{17}_{8}O} = 16.999u \):
\[ K_{{}^{17}_{8}O} = \frac{1.008}{16.999} \times 4.012 \]
\[ K_{{}^{17}_{8}O} \approx 0.400 \text{ MeV} \]
The corrected kinetic energy of \( {}^{17}_{8}O \) is approximately 0.400 MeV.
The motion of a particle in the XY plane is given by \( x(t) = 25 + 6t^2 \, \text{m} \); \( y(t) = -50 - 20t + 8t^2 \, \text{m} \). The magnitude of the initial velocity of the particle, \( v_0 \), is given by:
At a particular temperature T, Planck's energy density of black body radiation in terms of frequency is \(\rho_T(\nu) = 8 \times 10^{-18} \text{ J/m}^3 \text{ Hz}^{-1}\) at \(\nu = 3 \times 10^{14}\) Hz. Then Planck's energy density \(\rho_T(\lambda)\) at the corresponding wavelength (\(\lambda\)) has the value \rule{1cm}{0.15mm} \(\times 10^2 \text{ J/m}^4\). (in integer)
[Speed of light \(c = 3 \times 10^8\) m/s]
(Note: The unit for \(\rho_T(\nu)\) in the original problem was given as J/mΒ³, which is dimensionally incorrect for a spectral density. The correct unit J/(mΒ³Β·Hz) or JΒ·s/mΒ³ is used here for the solution.)