Presentation is loading. Please wait.

Presentation is loading. Please wait.

Ch 2 - Kinetic Theory reinisch_85.511.

Published byΚαίσαρ Αλεξιάδης Modified over 5 years ago

Similar presentations

Presentation on theme: "Ch 2 - Kinetic Theory reinisch_85.511."— Presentation transcript:

1 Ch 2 - Kinetic Theory reinisch_85.511

2 Particle Distribution Function
reinisch_85.511

3 Density Function ns reinisch_85.511

4 2.1.2 The Boltzmann Equation
reinisch_85.511

5 Total Derivative in Phase Space
reinisch_85.511

6 Examples of Distribution Functions
reinisch_85.511

7 2.2.2 Maxwellian Distribution Functions
reinisch_85.511

8 One-dimensional Maxwellian, cont’d
reinisch_85.511

9 Thermal speed reinisch_85.511

10 Equilibrium Distribution
charge x voltage = energy reinisch_85.511

11 2.3 Velocity Moments reinisch_85.511

12 Bulk flow velocity reinisch_85.511

13 Pressure tensor reinisch_85.511

14 Scalar pressure reinisch_85.511

15 Heat Flux reinisch_85.511

16 2.4.1 Continuity equation reinisch_85.511

17 reinisch_85.511

18 reinisch_85.511

Download ppt "Ch 2 - Kinetic Theory reinisch_85.511."

Similar presentations

Ideal gas Assumptions 1.Particles that form the gas have no volume and consist of single atoms. 2.Intermolecular interactions are vanishingly small.

Ideal gas Assumptions 1.Particles that form the gas have no volume and consist of single atoms. 2.Intermolecular interactions are vanishingly small.
Effects of Bulk Viscosity on p T -Spectra and Elliptic Flow Parameter Akihiko Monnai Department of Physics, The University of Tokyo, Japan Collaborator:

Effects of Bulk Viscosity on p T -Spectra and Elliptic Flow Parameter Akihiko Monnai Department of Physics, The University of Tokyo, Japan Collaborator:
Meanwhile, somewhere in California. Solar plasma Convection is complicated Temperature is very high Completely or partially ionized gas -> Charges (protons.

Meanwhile, somewhere in California. Solar plasma Convection is complicated Temperature is very high Completely or partially ionized gas -> Charges (protons.
Plasma Astrophysics Chapter 3: Kinetic Theory Yosuke Mizuno Institute of Astronomy National Tsing-Hua University.

Plasma Astrophysics Chapter 3: Kinetic Theory Yosuke Mizuno Institute of Astronomy National Tsing-Hua University.
We consider a dilute gas of N atoms in a box in the classical limit Kinetic theory de Broglie de Broglie wave length with density classical limit high.

We consider a dilute gas of N atoms in a box in the classical limit Kinetic theory de Broglie de Broglie wave length with density classical limit high.
Fluid equations, magnetohydrodynamics Multi-fluid theory Equation of state Single-fluid theory Generalised Ohm‘s law Magnetic tension and plasma beta Stationarity.

Fluid equations, magnetohydrodynamics Multi-fluid theory Equation of state Single-fluid theory Generalised Ohm‘s law Magnetic tension and plasma beta Stationarity.
Thermo & Stat Mech - Spring 2006 Class 14 1 Thermodynamics and Statistical Mechanics Kinetic Theory of Gases.

Thermo & Stat Mech - Spring 2006 Class 14 1 Thermodynamics and Statistical Mechanics Kinetic Theory of Gases.
Kinetic Theory of Gasses Physics 102 Professor Lee Carkner Lecture 4.

Kinetic Theory of Gasses Physics 102 Professor Lee Carkner Lecture 4.
Chapter 3. Transport Equations The plasma flows in planetary ionospheres can be in equilibrium (d/dt = 0), like the midlatitude terrestrial ionosphere,

Chapter 3. Transport Equations The plasma flows in planetary ionospheres can be in equilibrium (d/dt = 0), like the midlatitude terrestrial ionosphere,
Kinetic Theory of Gases Physics 102 Professor Lee Carkner Lecture 3 (Session: 104884) Would anyone in Monday 2:30 lab or Tuesday 12:30 lab like to switch.

Kinetic Theory of Gases Physics 102 Professor Lee Carkner Lecture 3 (Session: ) Would anyone in Monday 2:30 lab or Tuesday 12:30 lab like to switch.
2/24/02Prof. Reinisch 85.483/5111 4.3 Collision Cross Section (1) We are now extending from binary collisions (2 particles) to a flux of particles scattered.

2/24/02Prof. Reinisch / Collision Cross Section (1) We are now extending from binary collisions (2 particles) to a flux of particles scattered.
A k-  model for turbulently thermal convection in solar like and RGB stars Li Yan Yunnan Astronomical Observatory, CAS.

A k-  model for turbulently thermal convection in solar like and RGB stars Li Yan Yunnan Astronomical Observatory, CAS.
Main Points All matter is made up of invisible particles Particles have spaces between them Particles are moving all the time Particles move faster when.

Main Points All matter is made up of invisible particles Particles have spaces between them Particles are moving all the time Particles move faster when.
Viscosity. Average Speed The Maxwell-Boltzmann distribution is a function of the particle speed. The average speed follows from integration.  Spherical.

Viscosity. Average Speed The Maxwell-Boltzmann distribution is a function of the particle speed. The average speed follows from integration.  Spherical.
Elements of kinetic theory Introduction Phase space density Equations of motion Average distribution function Boltzmann-Vlasov equation Velocity distribution.

Elements of kinetic theory Introduction Phase space density Equations of motion Average distribution function Boltzmann-Vlasov equation Velocity distribution.
Deriving the Kinetic Theory Equation Thermal Physics Lesson 6.

Deriving the Kinetic Theory Equation Thermal Physics Lesson 6.
Thermal Energy.

Thermal Energy.
Aerodynamics Linear Motion (Moving Air ).

Aerodynamics Linear Motion (Moving Air ).
Kinetic energy Derivation of kinetic energy. Kinetic Energy 2 starting equations F = m x a (Newton’s 2 nd law) W = Force x distance.

Kinetic energy Derivation of kinetic energy. Kinetic Energy 2 starting equations F = m x a (Newton’s 2 nd law) W = Force x distance.
CH. 2. Base unit = coulomb also the base unit for current and voltage Symbol = Q Abbreviation = C.

CH. 2. Base unit = coulomb also the base unit for current and voltage Symbol = Q Abbreviation = C.

Similar presentations

Ads by Google