\( \frac{\nu}{3} \)
The photoelectric effect is governed by Einstein’s photoelectric equation:
\[ eV_0 = h\nu - h\nu_0 \]
where \( e \) is the electron charge, \( V_0 \) is the stopping potential, \( h \) is Planck’s constant, \( \nu \) is the light frequency, and \( \nu_0 \) is the threshold frequency.
Given:
From \( eV_0 = h\nu - h\nu_0 \), for frequency \( \nu \):
\[ eV_0 = h\nu - h\nu_0 \quad ...(1) \]
For frequency \( \frac{\nu}{2} \), we have:
\[ e\frac{V_0}{4} = h\left(\frac{\nu}{2}\right) - h\nu_0 \quad ...(2) \]
Let's solve equations (1) and (2). Multiply equation (2) by 4:
\[ eV_0 = 2h\left(\frac{\nu}{2}\right) - 4h\nu_0 \]
Simplifying gives:
\[ eV_0 = h\nu - 4h\nu_0 \quad ...(3) \]
We equate equations (1) and (3):
\[ h\nu - h\nu_0 = h\nu - 4h\nu_0 \]
Cancel \( h\nu \) and divide by \( h \):
\[ -\nu_0 = -4\nu_0 \]
Thus, solving for \( \nu_0 \) gives:
\[ 3\nu_0 = \nu \]
Therefore,
\[ \nu_0 = \frac{\nu}{3} \]
The threshold frequency \( \nu_0 \) for photoelectric emission is \( \frac{\nu}{3} \).
To find the threshold frequency \( \nu_0 \), we use the photoelectric equation: \( eV_0 = h(\nu - \nu_0) \).
1. For frequency \( \nu \), the stopping potential is \( V_0 \):
\( eV_0 = h(\nu - \nu_0) \).
2. For frequency \( \frac{\nu}{2} \), the stopping potential is \( \frac{V_0}{4} \):
\( e\left(\frac{V_0}{4}\right) = h\left(\frac{\nu}{2} - \nu_0\right) \).
Now, solve these equations simultaneously:
From equation 1:
\( eV_0 = h(\nu - \nu_0) \) ⇒ \( \nu_0 = \nu - \frac{eV_0}{h} \).
From equation 2:
\( e\left(\frac{V_0}{4}\right) = h\left(\frac{\nu}{2} - \nu_0\right) \)
⇒ \( \frac{eV_0}{4h} = \frac{\nu}{2} - \nu_0 \).
Substitute \( \nu_0 = \nu - \frac{eV_0}{h} \) into the second equation:
\( \frac{eV_0}{4h} = \frac{\nu}{2} - \left(\nu - \frac{eV_0}{h}\right) \).
Simplify:
\( \frac{eV_0}{4h} = \frac{\nu}{2} - \nu + \frac{eV_0}{h} \)
⇒ \( \frac{eV_0}{4h} = -\frac{\nu}{2} + \frac{eV_0}{h} \).
Rearrange:
\( \frac{eV_0}{4h} + \frac{\nu}{2} = \frac{eV_0}{h} \).
Calculate:
\( \frac{\nu}{2} = \frac{3eV_0}{4h} \)
Plug this back into \( \nu_0 = \nu - \frac{eV_0}{h} \):
Using \( \frac{\nu}{2} = \frac{3eV_0}{4h} \), so, \( \nu = \frac{3eV_0}{2h} \)
⇒ \( \nu_0 = \frac{3eV_0}{2h} - \frac{eV_0}{h} = \frac{3eV_0}{2h} - \frac{2eV_0}{2h} \)
⇒ \( \nu_0 = \frac{eV_0}{2h} \).
Thus, comparing \( \nu_0 \) in terms of \( \nu = \frac{3eV_0}{2h} \):
⇒ \( \nu_0 = \frac{\nu}{3} \).
The threshold frequency for the photoelectric emission is \( \frac{\nu}{3} \).
A solid cylinder of mass 2 kg and radius 0.2 m is rotating about its own axis without friction with angular velocity 5 rad/s. A particle of mass 1 kg moving with a velocity of 5 m/s strikes the cylinder and sticks to it as shown in figure.
The angular velocity of the system after the particle sticks to it will be: