Ch 12 - Kinetic Theory11th Physics
Historical Atomic Hypothesis
Which ancient Indian school of thought first detailed the atomic picture of matter, and what was the specific Sanskrit word used for the smallest indivisible particle?
Which ancient Indian school of thought first detailed the atomic picture of matter, and what was the specific Sanskrit word used for the smallest indivisible particle?
Historical Context
- Vaiseshika School: Founded by Kanada in the 6th century B.C., this school detailed the atomic picture of matter long before modern science.
- Paramanu: The Sanskrit word for the smallest, indivisible ultimate particle of matter.
Note: In ancient Greece, Democritus also proposed the 'atom' (meaning indivisible) in the 4th century B.C., while John Dalton is credited with the modern scientific atomic theory.
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Brownian Motion
What is Brownian Motion, and how does it serve as direct empirical evidence for the Kinetic Theory of Gases?
What is Brownian Motion, and how does it serve as direct empirical evidence for the Kinetic Theory of Gases?
Definition
Brownian Motion is the continuous, random, zig-zag macroscopic movement of microscopic particles (like pollen grains) suspended in a fluid (liquid or gas).
Evidence for Kinetic Theory
- It physically proves that the molecules of the fluid are in constant, chaotic, thermal motion.
- The random macroscopic movement of the suspended particles is caused by the unequal, unbalanced microscopic collisions from the invisible fluid molecules striking them from all sides.
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Perfect Gas Equation (Boltzmann Form)
Perfect Gas Equation (Boltzmann Form)
State the Perfect (Ideal) Gas Equation in terms of the total number of molecules () and the Boltzmann constant ().
Derivation
From , substitute . Thus, . Since , we get .
Variables & Units:
- P = Pressure (Pa)
- V = Volume (m³)
- N = Total number of gas molecules
- k_B = Boltzmann constant ( J/K)
- T = Absolute temperature (K)
Conditions/Notes:
- The Boltzmann constant relates macroscopic thermodynamic temperature to microscopic energy.
- This can also be written in terms of number density () as .
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Also in this chapter
30 more cards to study in Prism
- 4Interatomic Distances in States of Matter
- 5Estimating Molecular Radius
- 6Avogadro's Hypothesis
- 7Kinetic Theory Formula for Gas Pressure
- 8Real Gases vs. Ideal Gas Behaviour
- 9Kinetic Interpretation of Temperature
- 10Root Mean Square (RMS) Speed
- 11Postulates of Kinetic Theory
- 12Specific Heat: Monatomic Gas
- 13Specific Heat: Rigid Diatomic Gas
- 14Internal Energy: Ideal vs. Real Gases
- 15Specific Heat: Non-Rigid Diatomic Gas
- 16Specific Heat: Polyatomic Gases
- 17Specific Heat Capacity of Solids
- 18Absence of Hydrogen & Helium in Atmosphere
- 19Specific Heat Capacity of Water
- 20Maxwell-Boltzmann Speed Distribution
- 21Mean Free Path Formula
- 22Collision Frequency / Relaxation Time
- 23Hierarchy of Molecular Speeds
- 24Evaporative Cooling via Kinetic Theory
- 25Most Probable Speed ($v_p$) & Average Speed ($\bar{v}$)
- 26Degrees of Freedom ($f$)
- 27Dalton's Law of Partial Pressures (Kinetic Origin)
- 28Law of Equipartition of Energy
- 29Graham's Law of Diffusion
- 30Law of Atmospheres (Barometric Formula)
- 31Pressure and Total Translational Kinetic Energy
- 32Mean Free Path ($l$)
- 33Maxwell-Boltzmann Speed Distribution Function
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