Question 515 Marks
In 1959 Lyttleton and Bondi suggested that the expansion of the Universe could be explained if matter carried a net charge. Suppose that the Universe is made up of hydrogen atoms with a number density N, which is maintained a constant. Let the charge on the proton be: $e_p = -(1 + y)e$ where e is the electronic charge.
Find the critical value of y such that expansion may start.
Find the critical value of y such that expansion may start.
Answer
View full question & answer→Let the Universe have a radius R. Assume that the hydrogen atoms are uniformly distributed. The Expansion starts if the Coulumb repulsion on a hydrogen atom, at R, is larger than the gravitational attraction.
The hydrogen atom contains one proton and one electron, charge on each hydrogen atom.
$e_H = e_P + e = -(1 + y)e + e = -ye = |ye|$
Let E be elecrtric field intensity at distance R, on the surface of the sphere, the according to Gauss' theorem,
$\oint\overrightarrow{\text{E}}.\text{d}\overrightarrow{\text{S}}=\frac{\text{q}_\text{enclosed}}{\in_0}$
$\Rightarrow\ \text{E}(4\pi\text{R}^2)=\frac{4}{3}\frac{\pi\text{R}^3\text{N}|\text{ye}|}{\in_0}$
$\Rightarrow\ \text{E}=\frac{1}{3}\frac{\text{N}|\text{ye}|\text{R}}{\in_0}\ .....(\text{i})$
Let us suppose the mass of each nydrogen atom $= m_p =$ Mass of a proton and $G_R =$ gravitational rield at distance R on the sphere.
Then $-4\pi\text{R}^2\text{G}_\text{R}=4\pi\text{Gm}_\text{p}\Big(\frac{4}{3}\pi\text{R}^3\Big)\text{N}$
$\Rightarrow\ \text{G}_\text{R}=\frac{-4}{3}\pi\text{Gm}_\text{p}\text{NR}\ .....(\text{ii})$
$\therefore$ Gravitational force on this atom is
$\text{F}_\text{G}=\text{m}_\text{p}\times\text{G}_\text{p}=\frac{-4\pi}{3}\text{Gm}_\text{p}^2\text{NR}\ .....(\text{iii})$
Coulomb force on hydrogen atom at R is
$\text{F}_\text{C}=(\text{ye})\text{E}=\frac{1}{3}\frac{\text{Ny}^2\text{e}^2\text{R}}{\in_0}\ \ [\text{from Eq. (i)}]$
Now, to start expansion $F_C > F_G$ and aritical value of y to start expansion wolud be when,
$F_C = F_G$
$\Rightarrow\ \frac{1}{3}\frac{\text{Ny}^2\text{e}^2\text{R}}{\in_0}=\frac{4\pi}{3}\text{Gm}_\text{p}^2\text{NR}$
$\Rightarrow\ \text{y}^2=(4\pi\in_0)\text{G}\Big(\frac{\text{m}_\text{p}}{\text{e}}\Big)^2$
$=\frac{1}{9\times10^9}\times(6.67\times10^{-11})$
$=\frac{1}{9\times10^9}\times(6.67\times10^{-11})\Big(\frac{(1.66\times10^{-27})^2}{(1.6\times10^{-19})^2}\Big)$
$\Rightarrow\ \text{y}=\sqrt{79.8\times10^{-38}}=8.9\times10^{-19}\simeq10^{-18}$
Hence $10^{-18}$ is the required critical value of y corresponding to which expansion of universe would start.
The hydrogen atom contains one proton and one electron, charge on each hydrogen atom.
$e_H = e_P + e = -(1 + y)e + e = -ye = |ye|$
Let E be elecrtric field intensity at distance R, on the surface of the sphere, the according to Gauss' theorem,
$\oint\overrightarrow{\text{E}}.\text{d}\overrightarrow{\text{S}}=\frac{\text{q}_\text{enclosed}}{\in_0}$
$\Rightarrow\ \text{E}(4\pi\text{R}^2)=\frac{4}{3}\frac{\pi\text{R}^3\text{N}|\text{ye}|}{\in_0}$
$\Rightarrow\ \text{E}=\frac{1}{3}\frac{\text{N}|\text{ye}|\text{R}}{\in_0}\ .....(\text{i})$
Let us suppose the mass of each nydrogen atom $= m_p =$ Mass of a proton and $G_R =$ gravitational rield at distance R on the sphere.
Then $-4\pi\text{R}^2\text{G}_\text{R}=4\pi\text{Gm}_\text{p}\Big(\frac{4}{3}\pi\text{R}^3\Big)\text{N}$
$\Rightarrow\ \text{G}_\text{R}=\frac{-4}{3}\pi\text{Gm}_\text{p}\text{NR}\ .....(\text{ii})$
$\therefore$ Gravitational force on this atom is
$\text{F}_\text{G}=\text{m}_\text{p}\times\text{G}_\text{p}=\frac{-4\pi}{3}\text{Gm}_\text{p}^2\text{NR}\ .....(\text{iii})$
Coulomb force on hydrogen atom at R is
$\text{F}_\text{C}=(\text{ye})\text{E}=\frac{1}{3}\frac{\text{Ny}^2\text{e}^2\text{R}}{\in_0}\ \ [\text{from Eq. (i)}]$
Now, to start expansion $F_C > F_G$ and aritical value of y to start expansion wolud be when,
$F_C = F_G$
$\Rightarrow\ \frac{1}{3}\frac{\text{Ny}^2\text{e}^2\text{R}}{\in_0}=\frac{4\pi}{3}\text{Gm}_\text{p}^2\text{NR}$
$\Rightarrow\ \text{y}^2=(4\pi\in_0)\text{G}\Big(\frac{\text{m}_\text{p}}{\text{e}}\Big)^2$
$=\frac{1}{9\times10^9}\times(6.67\times10^{-11})$
$=\frac{1}{9\times10^9}\times(6.67\times10^{-11})\Big(\frac{(1.66\times10^{-27})^2}{(1.6\times10^{-19})^2}\Big)$
$\Rightarrow\ \text{y}=\sqrt{79.8\times10^{-38}}=8.9\times10^{-19}\simeq10^{-18}$
Hence $10^{-18}$ is the required critical value of y corresponding to which expansion of universe would start.











