
Concept explainers
(a)
Interpretation:
A
When the real gas molecules occupy a relatively small volume and have large intermolecular attractions, the pressure of the two gases has to be compared.
Concept Introduction:
The ideal gas equation is:
Where,
P is the pressure
V is the volume
T is the temperature
R is molar gas constant
n is the mole
(b)
Interpretation:
A
When the real gas molecules occupy a relatively large volume and have negligible intermolecular attractions, the pressure of the two gases has to be compared.
Concept Introduction:
Ideal
The ideal gas equation is:
Where,
P is the pressure
V is the volume
T is the temperature
R is molar gas constant
n is the mole
(c)
Interpretation:
A
When the real gas molecules occupy a relatively large volume and have large intermolecular attractions, the pressure of the two gases has to be compared.
Concept Introduction:
Ideal Gas Law:
The ideal gas equation is:
Where,
P is the pressure
V is the volume
T is the temperature
R is molar gas constant
n is the mole

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Chapter 5 Solutions
Student Solutions Manual for Ebbing/Gammon's General Chemistry
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- The quantum yield of the photochemical decay of HI is 2. Calculate the number of Einsteins absorbed per mole knowing that the energy absorbed per mole of photons is 490 kJ.arrow_forwardThe quantum yield of the photochemical decay of HI is 2. How many moles of HI per kJ of radiant energy can be decayed knowing that the energy absorbed per mole of photons is 490 kJ.arrow_forwardIf the energy absorbed per mole of photons is 450 kJ, the number of Einsteins absorbed per 1 mole.arrow_forward
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