For the fusion reactions powering the Sun to take place, protons (with charge +1.6x10¹⁹C, and mass 3.3x10-²7kg) must come within 2.4x10*¹5m of each other. (At that range the strong nuclear force overcomes their electrical repulsion, and they merge into deuterium. Later, two deuterium fuse into helium, completing the reaction.) a) If two protons have a head on collision at equal speeds, how fast must they be going in order to get close enough to react? b) Use the ideal gas equation for average kinetic energy: Kavg = (3/2)kT to find the temperature at which the average proton would be moving fast enough to undergo fusion. Note that this is Boltzman's constant, k, = 1.38x10²³ J/K, in this formula. (Note that this temperature is actually much hotter than the core of the Sun - in the sun it's not the average H* that need to be moving fast enough to fuse, just the fastest ones.)

Modern Physics
3rd Edition
ISBN:9781111794378
Author:Raymond A. Serway, Clement J. Moses, Curt A. Moyer
Publisher:Raymond A. Serway, Clement J. Moses, Curt A. Moyer
Chapter14: Nuclear Physics Applications
Section: Chapter Questions
Problem 33P
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For the fusion reactions powering the Sun to take place, protons (with charge +1.6x10¹⁹C, and mass
3.3x10-²7kg) must come within 2.4x10*¹5m of each other. (At that range the strong nuclear force
overcomes their electrical repulsion, and they merge into deuterium. Later, two deuterium fuse into
helium, completing the reaction.)
a) If two protons have a head on collision at equal speeds, how fast must they be going in order to
get close enough to react?
b)
Use the ideal gas equation for average kinetic energy: Kavg = (3/2)kT to find the temperature at
which the average proton would be moving fast enough to undergo fusion. Note that this is
Boltzman's constant, k, = 1.38x10²³ J/K, in this formula. (Note that this temperature is actually
much hotter than the core of the Sun - in the sun it's not the average H* that need to be moving
fast enough to fuse, just the fastest ones.)
Transcribed Image Text:For the fusion reactions powering the Sun to take place, protons (with charge +1.6x10¹⁹C, and mass 3.3x10-²7kg) must come within 2.4x10*¹5m of each other. (At that range the strong nuclear force overcomes their electrical repulsion, and they merge into deuterium. Later, two deuterium fuse into helium, completing the reaction.) a) If two protons have a head on collision at equal speeds, how fast must they be going in order to get close enough to react? b) Use the ideal gas equation for average kinetic energy: Kavg = (3/2)kT to find the temperature at which the average proton would be moving fast enough to undergo fusion. Note that this is Boltzman's constant, k, = 1.38x10²³ J/K, in this formula. (Note that this temperature is actually much hotter than the core of the Sun - in the sun it's not the average H* that need to be moving fast enough to fuse, just the fastest ones.)
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Can you please solve this without using calculus? There has to be a way to use the formulas for kinetic energy and potential energy to solve for velocity. 

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