Giving Statistical Mechanics The Shakes: Analogies Between Ideal Gases and Granular Systems Justin Mitchell, Aaron Coyner, Matthew Olson, Rebecca Ragar,

Slides:



Advertisements
Similar presentations
Kinetic Theory of Matter
Advertisements

Proto-Planetary Disk and Planetary Formation
Granular Jets Alexander BarnaveliGeorgia If a steel ball is dropped onto a bed of dry sand, a "splash" will be observed that may be followed by the ejection.
Chapter 16 Section 1 Kinetic Theory.
Classical Statistical Mechanics in the Canonical Ensemble.
Internal structure of planets Internal structures of planets (not at scale). The three sub-families on the left are part of the terrestrial family. Giant.
LAMIA RAO XI KINETIC MOLECULAR THEORY. MondayTuesdayWednesdayThursdayFriday Introduction to Kinetic molecular theory by showing examples Explanation of.
Chapter 10 Review. What is the heat in Joules required to melt 25 grams of ice? Useful information: heat of fusion of water = 334 J/g q = m·ΔHf q = (25.
John Drozd Colin Denniston Simulations of Collision Times In Gravity Driven Granular Flow bottom sieve particles at bottom go to top reflecting left and.
In your NOTEBOOK: Write down the question and answer.
2008 Physics 2111 Fundamentals of Physics Chapter 9 1 Fundamentals of Physics Chapter 9a Systems of Particles 1.A Special Point 2.The Center of Mass 3.Newton’s.
Measurement of the Charge of a Particle in a Dusty Plasma Jerome Fung, Swarthmore College July 30, 2004.
More Forces Lecturer: Professor Stephen T. Thornton
Kinetic Theory and the States of Matter. Kinetic Theory All matter (solids, liquids, and gases) are made up of particles. The kinetic theory states that.
Kinetic Theory.
The Brazil Nut Effect Modelling granular convection with bouncing balls By Richie Stauffer.
Granular Systems in Microgravity Michael L. Wilson The University of Tulsa Supported by Research Corporation.
Granular Materials R. Behringer Duke University Durham, NC, USA.
Section 5: The Ideal Gas Law The atmospheres of planets (and the Sun too) can be modelled as an Ideal Gas – i.e. consisting of point-like particles (atoms.
Topic 17: States of Matter Table of Contents Topic 17 Topic 17 Click box to view movie clip.
Goal: To understand how stars form. Objectives: 1)To learn about the properties for the initial gas cloud for 1 star. 2)To understand the collapse and.
Impact Data Analysis and Sensor Modification for Pressure Data of Granular Gases in Reduced Gravity Aaron Coyner, Justin Mitchell, and Matthew Olson University.
Temperature Oscillations in a Compartmetalized Bidisperse Granular Gas C. K. Chan 陳志強 Institute of Physics, Academia Sinica, Dept of Physics,National Central.
1 Granular Fluidization in Reduced Gravity University of Tulsa Supported by Research Corp. Justin Mitchell, Aaron Coyner, Rebecca Ragar, Matt Olson, Ian.
The study of fission dynamics in fusion-fission reactions within a stochastic approach Theoretical model for description of fission process Results of.
Physical Science Objective 5.03
Knight: Chapter 15 Fluids & Elasticity ( Fluids & Pressure)
Gas class #1 OBJECTIVE: understanding the nature of gases, the KMT, the 4 variables to measure gases, and the first demo diagram for gases.
Std 4 - Questions Grade: «grade» Subject: Standard 4 - practice q's Date: «date»
The Nature of Gases Kinetic Theory and a Model for Gases.
1. 1.The Parts of the Solar System 2 We live on the planet Earth Vocabulary Planet A large, solid object that travels around a star 3.
Physical Properties of Matter
Properties of Gases Kinetic Molecular Theory. Kinetic-Molecular Theory  Based on idea that particles of matter are always in motion.  Provides reasoning.
16.1 Notes Kinetic Theory. KINETIC THEORY Kinetic Theory- An explanation of how particles in matter behave. The 3 Assumptions of Kinetic Theory: 1. All.
States of Matter Chapter 13. Chapter 13- The States of Matter  Gases- indefinite volume and shape, low density.  Liquids- definite volume, indefinite.
Chapter 15FLUIDS 15.1 Fluid and the World Around Us 1.A fluid is a substance that cannot support a shearing stress. 2.Both gases and liquids are fluids.
Lab Demos with Particles Observations Smell jars Icebergs A Drop of Color Ice to Steam KINETIC Molecular Theory.
Unit 5 Section 2 Notes Matter and Energy Kinetic Theory of Matter:  Useful for seeing differences in the 3 common states of matter on earth: solid,
Chiral phase transition and chemical freeze out Chiral phase transition and chemical freeze out.
Granular matter 김종현.
Geotechnical Engineering
Metals I: Free Electron Model
THERMAL ENERGY AND HEAT SPH4C April THERMAL ENERGY James Prescott Joule ( ) spent much of his honeymoon studying waterfalls. He noticed.
Unit 7-Behavior of Gas Molecules Kinetic Molecular Theory Collision Theory of Gas Molecules.
Vocabulary Click Below to start with a video – when the window opens be sure to click download.
Liquids 10.2 Liquids Fun Fact - Least common type of matter! Definite volume; no definite shape How do you think the particles behave? Fluid – substance.
Gr.A.I.N.S. II Presentation Scrapbook Proposal ID University of Tulsa.
Chapter 16 Kinetic Theory of Gases. Ideal gas model 2 1. Large number of molecules moving in random directions with random speeds. 2. The average separation.
The Particle Model. Models in Science Have you ever put together a model car or airplane? If so, in what ways are the model and the real object the.
Solar System Formation Solar System Comprised of a star and the planets that orbit the star Binary – Two stars at center of system –Eclipsing is when.
Fluid Mechanics Liquids and gases have the ability to flow
Phase Transitions of Complex Networks and related Xiaosong Chen Institute of Theoretical Physics Chinese Academy of Sciences CPOD-2011, Wuhan.
“One does not meet oneself until one catches the reflection from an eye other than human.” - Loren Eiseley -
John Drozd Colin Denniston Simulations of Collision Times and Stress In Gravity Driven Granular Flow bottom sieve particles at bottom go to top reflecting.
Managing A Computer Simulation of Gravity-Driven Granular Flow The University of Western Ontario Department of Applied Mathematics John Drozd and Dr. Colin.
Slow Relaxations in Complex Fluids: Origin and Nature of Dynamical Heterogeneities B. Chakraborty, Brandeis University, DMR Materials as diverse.
Kinetic Molecular Theory Chemistry. Kinetic Molecular Theory The theory that the behavior of substances can be explained by the motion of the molecules.
Essential Questions How does the Kinetic molecular theory explain the behavior of gases? How does the kinetic molecular theory explain the phase changes.
Chapter 10. States of Matter 10.1 Kinetic Molecular Theory and Gases.
Computer Simulation of Gravity-Driven Granular Flow University of Western Ontario Department of Applied Mathematics John Drozd and Dr. Colin Denniston.
CHAPTER 16 SOLIDS, LIQUIDS, and GASES. video SECTION 1 KINETIC THEORY KINETIC THEORY (Particle Theory) of MATTER: KINETIC THEORY (Particle Theory) of.
Kinetic theory model This model demos how the pressure and volume of a gas are directly linked to the velocity and therefore temperature of a gas. They.
UNDERSTANDING KMT USING GAS PROPERTIES AND STATES OF MATTER Learning Goals: Students will be able to describe matter in terms of particle motion. The description.
Bell Ringer 09/05/2012 Look at the display in front of the room… Describe, in complete sentences, what you see in each box.
States of Matter Learning Goal: I can explain the relationship between kinetic energy and states of matter.
The solar system Topic # 2 Term # 2 The Local System.
John Drozd Colin Denniston
State of Matter Volume Shape Structure/Energy
FLUID MECHANICS - Review
Physics Physics is the branch of science that encompasses the natural world, including the earth and all of the physical systems within, as well as the.
Presentation transcript:

Giving Statistical Mechanics The Shakes: Analogies Between Ideal Gases and Granular Systems Justin Mitchell, Aaron Coyner, Matthew Olson, Rebecca Ragar, Jeffery Wagner, Adrienne McVey, Justin Eskridge, Erin Lewallen, Ian Zedalis, Shawn Jackson, Michael Wilson* The University of Tulsa *Currently at National Research Council

Granular Systems? We know systems of or 2 particles. This neglects dunes, avalanches and other systems. Granular systems involve dust, sand, powder, and grains. We investigate statistics of driven systems.

Inelastic Collapse Each inelastic collision will remove energy. Many collisions will cause system to collapse. Energy in and out will define our granular phase.

Project Description Goals Look for definitive inelastic collapse of a 3-d granular system in zero gravity. Determine parameters necessary for a granular gas, the precursor to collapse. * É. Falcon et al., Phys. Rev. Lett (1999). Methods Preliminary testing on NASA KC-135A low gravity aircraft Future flight on Space Shuttle Testing on sounding rocket *

Why Investigate Granular Gases? Large granular systems, such as planets, are not well understood. Asteroids, planetary rings, etc. are not fully explained by gravity because sizes are too small for gravity to act alone. Inelastic collapse models provide plausible method for formation of these smaller objects. Small scale granular gas studies allow for lab testing of the models on reasonable time scales.

Experimental Description Box set: 8 sapphire walled cubes, 1 in 3 each. Box set mechanically shaken sinusoidally along body diagonal. Each cube has one free wall attached to a piezoelectric sensor. Video cameras view 3 orthogonal box set faces.

Box Set as Flown on KC- 135A

System Acceleration Shaking direction is perpendicular to mean effective gravity. In “microgravity” the residual acceleration is ~0.03 g earth. Residual acceleration is usually pointed up. shaking g earth Residual acceleration

Granular Phases Solid Grains pack in one corner Fluid Grains slosh around box walls Gas ~uniform distribution of kinetic grains g residual

Phase Diagram o  =A  2 /g residual   is the ratio of wall acceleration to g residual   diverges as g residual goes to zero. o Wall acceleration, density and g residual define the phase.

Recent Work Second KC-135 flight Free floating experiment. No system accelerations until bumped. Lower shaking accelerations. Further testing before shuttle flight.

Clustering Into Lattice Lattice Random

Conclusion Clusters are stable and keep a lattice. Clusters only exist in slow shaking (~4Hz). Gases form for all shaking parameters. Only solid for non-shaking system. Partial proof of concept. Experiment is ready for a shuttle flight.