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An important milestone in the evolution of the universe just after the Big Bang is the Planck time t_(p), the value of which depends on three fundamental constants-speed of light in vacuum c, Gravitational constant G and Planck's constant h. Then, t_(p) prop |
Answer» <html><body><p>`Ghc^(5)`<br/>`(C^(5))/(<a href="https://interviewquestions.tuteehub.com/tag/gh-468237" style="font-weight:bold;" target="_blank" title="Click to know more about GH">GH</a>)`<br/>`(Gh)/(c^(5)`<br/>`((Gh)/(c^(5)))^(1//2)`</p>Solution :`[Gh]= [M^(-1)<a href="https://interviewquestions.tuteehub.com/tag/l-535906" style="font-weight:bold;" target="_blank" title="Click to know more about L">L</a>^(3)T^(-2)][ML^(2)T^(-1)]= [M^(<a href="https://interviewquestions.tuteehub.com/tag/0-251616" style="font-weight:bold;" target="_blank" title="Click to know more about 0">0</a>)L^(5)T^(-3)], [c]= [LT^(-1)]` <br/> `:. [(Gh)/(c^(5))]^(1//2)=[ T]` <a href="https://interviewquestions.tuteehub.com/tag/hence-484344" style="font-weight:bold;" target="_blank" title="Click to know more about HENCE">HENCE</a>, `t_(p) prop ((Gh)/(c^(5)))^(1//2) :. [t_(p)]= [T]`</body></html> | |