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Question: Find the typical de Broglie wavelength associated with a He atom in helium gas at room temperature \...

Find the typical de Broglie wavelength associated with a He atom in helium gas at room temperature (27C)\left( {27^\circ C} \right)and 1atm pressure, and compare it with the mean separation between two atoms under these conditions.

  1. ro=6.4×109m{r_o} = 6.4 \times {10^{ - 9}}m
  2. ro=3.4×109m{r_o} = 3.4 \times {10^{ - 9}}m
  3. ro=4.4×109m{r_o} = 4.4 \times {10^{ - 9}}m
  4. ro=5.4×109m{r_o} = 5.4 \times {10^{ - 9}}m
Explanation

Solution

In the question we have asked to compare the De-Broglie wavelength which is associated with the He atom with the mean separation between two atoms. De – Broglie wavelength is the starting of quantum mechanics. It determines the probability density of finding the object at a given time in a specified space.

Step by step solution:
Step 1: Calculate the De-Broglie wavelength
Find out the mass of the helium atom:
m=Atomic mass of HeAvogadro’s Numberm = \dfrac{{{\text{Atomic mass of He}}}}{{{\text{Avogadro's Number}}}} ;
Put in the given value in the above equation:
m=46×1023gms\Rightarrow m = \dfrac{4}{{6 \times {{10}^{23}}}}gms;
m=6.67×1027kg\Rightarrow m = 6.67 \times {10^{ - 27}}kg;
De-Broglie wavelength is given as:
λ=hp\lambda = \dfrac{h}{p} ;
Where:
λ\lambda = Wavelength;
hh= Planck’s Constant;
pp= momentum;
λ=h3mkT\Rightarrow \lambda = \dfrac{h}{{\sqrt {3mkT} }};
Here:
p=3mkTp = \sqrt {3mkT} ;
m = Mass;
k = Constant;
T= Absolute Temperature;

Put in the given value in the above equation:
λ=6.63×10343×6.67×1027×1.38×1023×300\Rightarrow \lambda = \dfrac{{6.63 \times {{10}^{ - 34}}}}{{\sqrt {3 \times 6.67 \times {{10}^{ - 27}} \times 1.38 \times {{10}^{ - 23}} \times 300} }};
λ=7×1011m\Rightarrow \lambda = 7 \times {10^{ - 11}}m;

Step 2: Calculate the mean separation
The kinetic gas equation for 1mole of gas is given as:
PV=RT=kNTPV = RT = kNT;
Where:
P = Pressure;
V = Volume;
T = Absolute Temperature;
R = Ideal gas constant;
N = Number of atoms and molecules;
k = Constant;

VN=kTP \Rightarrow \dfrac{V}{N} = \dfrac{{kT}}{P};
The mean separation is given by:
ro=(Molar VolumeAvogadro’s Number)13{r_o} = {\left( {\dfrac{{{\text{Molar Volume}}}}{{{\text{Avogadro's Number}}}}} \right)^{\dfrac{1}{3}}} ;
ro=(VN)13{r_o} = {\left( {\dfrac{{\text{V}}}{N}} \right)^{\dfrac{1}{3}}};
Now put VN=kTP\dfrac{V}{N} = \dfrac{{kT}}{P}in the above equation and solve:
ro=(KTP)13\Rightarrow {r_o} = {\left( {\dfrac{{{\text{KT}}}}{P}} \right)^{\dfrac{1}{3}}};
Put in the given values in the above equation:
ro=(1.38×1023×3001.01×105)13\Rightarrow {r_o} = {\left( {\dfrac{{{\text{1}}{\text{.38}} \times {\text{1}}{{\text{0}}^{ - 23}} \times 300}}{{1.01 \times {{10}^5}}}} \right)^{\dfrac{1}{3}}};
The mean separation is:
ro=3.4×109m\Rightarrow {r_o} = 3.4 \times {10^{ - 9}}m;

Option “2” is correct. The mean separation is ro=3.4×109m{r_o} = 3.4 \times {10^{ - 9}}m. Here the mean separation is very large as compared to the de Broglie wavelength.

Note: Here, we have to first find out the De-Broglie wavelength by first finding out the mass of the helium atom and then put the mass in the famous equation of the De-Broglie wavelength. Then apply the formula for mean separation and make a relation with the formula for gas constant PV = RT = kNT.