Velocity distribution of ideal gas molecules

Size: px
Start display at page:

Download "Velocity distribution of ideal gas molecules"

Transcription

1 August 25, 2006

2 Contents Review of thermal movement of ideal gas molecules.

3 Contents Review of thermal movement of ideal gas molecules. Distribution of the velocity of a molecule in ideal gas.

4 Contents Review of thermal movement of ideal gas molecules. Distribution of the velocity of a molecule in ideal gas. Boltzmann distribution.

5 Time slots starts from week 3 (28AUG-1SEP).

6 Time slots starts from week 3 (28AUG-1SEP). A class tutorial every week, on Friday 9 am - 10 am.

7 Time slots starts from week 3 (28AUG-1SEP). A class tutorial every week, on Friday 9 am - 10 am. A small group tutorial every even week (4,6,8,10), on Mon ( pm) or on Wed ( pm). The small group tutorial classroom is S

8 Time slots starts from week 3 (28AUG-1SEP). A class tutorial every week, on Friday 9 am - 10 am. A small group tutorial every even week (4,6,8,10), on Mon ( pm) or on Wed ( pm). The small group tutorial classroom is S Group A(30%): week 4, 8,12, Mon; group B(70%): week 6,10, 12, Wed.

9 Review: random walk leads to Gaussian distribution

10 Temperature is a measure of the molecule movements Ideal gas law: PV = Nk B T. Pressure is determined by gas molecule move: PV = m < v 2 x > N = m<v 2 >N 3. We thus have: The average kinetic energy ε k = 1 2 m < v 2 > of a molecule in an ideal gas is 3 2 k BT. Each degree of freedom contribute 1 2 k BT.

11 Speed of gas molecules on earth surface at room temperature At the earth surface, P = 10 5 Pa, the mole density is c = 1 24 M = 1 mol 24 L (1mol = ; 1L = 10 3 m 3 ). Let N = 1mol, please compute Nk B T, PV, and Nk BT PV. Show that the ideal gas is a reasonable approximation to the gas on earth. Gas on earth mostly consists nitrogen. One nitrogen molecule has a mass m kg. At room temperature T = 300K, please compute that its kinetic energy ε k, and show that the average of the magnitude of its speed < v 2 > 500 m s.

12 Why gas molecules does not fall onto the ground in earth? The change in the potential: U(z) = mgz, assuming it is a nitrogen molecule. So Z max ε k mg. Please compute Z max. Please show that in a room, the gravitation does not affect the gas molecule distribution. At what mass the gravitation can affect the distribution of the molecules in a room on earth? At what mass the gravity can trap a molecule within 1micron = 10 6 m?

13 Interaction strength between molecules General rule of estimating the interaction strength: fd k B T, where f is the force, and d is the characteristic interaction distance. So f k BT d pn for d nm. Many proteins can bind to and unbind from DNA. The binding and unbinding equilibrium is driven by electrostatic interactions and thermal fluctuation. In usual physiological salt condition ( 150 mm NaCl), the interaction distance is 1.7nm. If the binding and unbinding are both frequent, please show that the interaction strength must be around several Pico Newtons.

14 Wild guess of the velocity distribution of the gas molecules Range of velocity: < v x <. Symmetry in direction: ρ(v x ) = ρ( v x ), so < v x >= 0. Since 1 2 m < v 2 x >= 1 2 k BT, the higher the T, the bigger the variance σ 2 v x =< v 2 x >. Orientational symmetry: ρ(v x ) = ρ(v y ) = ρ(v z ). At small T, ρ(v x ) quickly goes to zero for v x > 0. What function is a good candidate?

15 Random walk in the velocity space We know a random walk in coordinate space leads to a Gaussian distribution. Gas molecules are changing their their accelerations randomly. This can be thought as a random walk in the velocity space. Not strictly, we can guess the velocity distribution is a Gaussian. We already knew < v 2 x >= k BT m,and < v x >= 0. Please show that: ρ(v x ) = m mv 2 2πk B T e x 2k B T.

16 More on ρ(v x )

17 Maxwell distribution of the velocity of individual molecules We have learnt that: ρ(v x ) = m mv 2 2πk B T e x 2k B T. But molecules are moving in 3-d. Reasonable guess: moving in each direction is independent. So ρ( v) = ρ(v x, v y, v z ) = ρ(v x ) ρ(v y ) ρ(v z ). Please show ρ( v) = ( v 2 = vx 2 + vy 2 + vz 2. Find < v >, u = < v 2 >. m 2πk B T )3/2 e mv 2 2k B T, where

18 More on ρ( v)

19 Maxwell distribution of the scalar velocity of individual molecules What is the distribution of the magnitude of the velocity ρ(u), where u = v? 2 2k B T. m It can be shown that ρ(u) = 4π( 2πk B T )3/2 u 2 e mu Prove ρ(u) is normalized. Show that the most probable u max = (Hint: d du ρ(u) = 0). 2k B T m

20 More on ρ(u)

21 Maxwell distribution of the velocity-n molecule We have N molecules in the tank. The velocity distribution of each molecule follows ρ( v i ) = ( mv i 2 m 2πk B T )3/2 2k e B T. The movement of the molecules are independent, so the joint prob of the system is ρ( v 1, v 2,, v N ) = ρ( v 1 )ρ( v 2 ) ρ( v N ) = ( m(v 1 2 m +v v2 N ) 2πk B T )3N/2 2k e B T. The above distribution only applies to ideal gas (no interactions among the gas molecules).

Velocity distribution of ideal gas molecules

Velocity distribution of ideal gas molecules September 5, 2006 Contents Review of the distribution of the velocity of a molecule in ideal gas. Contents Review of the distribution of the velocity of a molecule in ideal gas. Boltzmann distribution

More information

PHYSICS - CLUTCH CH 19: KINETIC THEORY OF IDEAL GASSES.

PHYSICS - CLUTCH CH 19: KINETIC THEORY OF IDEAL GASSES. !! www.clutchprep.com CONCEPT: ATOMIC VIEW OF AN IDEAL GAS Remember! A gas is a type of fluid whose volume can change to fill a container - What makes a gas ideal? An IDEAL GAS is a gas whose particles

More information

Handout 11: Ideal gas, internal energy, work and heat. Ideal gas law

Handout 11: Ideal gas, internal energy, work and heat. Ideal gas law Handout : Ideal gas, internal energy, work and heat Ideal gas law For a gas at pressure p, volume V and absolute temperature T, ideal gas law states that pv = nrt, where n is the number of moles and R

More information

CHAPTER 21 THE KINETIC THEORY OF GASES-PART? Wen-Bin Jian ( 簡紋濱 ) Department of Electrophysics National Chiao Tung University

CHAPTER 21 THE KINETIC THEORY OF GASES-PART? Wen-Bin Jian ( 簡紋濱 ) Department of Electrophysics National Chiao Tung University CHAPTER 1 THE KINETIC THEORY OF GASES-PART? Wen-Bin Jian ( 簡紋濱 ) Department of Electrophysics National Chiao Tung University 1. Molecular Model of an Ideal Gas. Molar Specific Heat of an Ideal Gas. Adiabatic

More information

Handout 11: Ideal gas, internal energy, work and heat. Ideal gas law

Handout 11: Ideal gas, internal energy, work and heat. Ideal gas law Handout : Ideal gas, internal energy, work and heat Ideal gas law For a gas at pressure p, volume V and absolute temperature T, ideal gas law states that pv = nrt, where n is the number of moles and R

More information

ε tran ε tran = nrt = 2 3 N ε tran = 2 3 nn A ε tran nn A nr ε tran = 2 N A i.e. T = R ε tran = 2

ε tran ε tran = nrt = 2 3 N ε tran = 2 3 nn A ε tran nn A nr ε tran = 2 N A i.e. T = R ε tran = 2 F1 (a) Since the ideal gas equation of state is PV = nrt, we can equate the right-hand sides of both these equations (i.e. with PV = 2 3 N ε tran )and write: nrt = 2 3 N ε tran = 2 3 nn A ε tran i.e. T

More information

Kinetic Theory of Gases

Kinetic Theory of Gases Kinetic Theory of Gases Chapter 3 P. J. Grandinetti Chem. 4300 Aug. 28, 2017 P. J. Grandinetti (Chem. 4300) Kinetic Theory of Gases Aug. 28, 2017 1 / 45 History of ideal gas law 1662: Robert Boyle discovered

More information

Physics 231 Topic 12: Temperature, Thermal Expansion, and Ideal Gases Alex Brown Nov

Physics 231 Topic 12: Temperature, Thermal Expansion, and Ideal Gases Alex Brown Nov Physics 231 Topic 12: Temperature, Thermal Expansion, and Ideal Gases Alex Brown Nov 18-23 2015 MSU Physics 231 Fall 2015 1 homework 3 rd midterm final Thursday 8-10 pm makeup Friday final 9-11 am MSU

More information

Kinetic theory of the ideal gas

Kinetic theory of the ideal gas Appendix H Kinetic theory of the ideal gas This Appendix contains sketchy notes, summarizing the main results of elementary kinetic theory. The students who are not familiar with these topics should refer

More information

1 Particles in a room

1 Particles in a room Massachusetts Institute of Technology MITES 208 Physics III Lecture 07: Statistical Physics of the Ideal Gas In these notes we derive the partition function for a gas of non-interacting particles in a

More information

Lecture 18 Molecular Motion and Kinetic Energy

Lecture 18 Molecular Motion and Kinetic Energy Physical Principles in Biology Biology 3550 Fall 2017 Lecture 18 Molecular Motion and Kinetic Energy Monday, 2 October c David P. Goldenberg University of Utah goldenberg@biology.utah.edu Fick s First

More information

Homework: 13, 14, 18, 20, 24 (p )

Homework: 13, 14, 18, 20, 24 (p ) Homework: 13, 14, 18, 0, 4 (p. 531-53) 13. A sample of an ideal gas is taken through the cyclic process abca shown in the figure below; at point a, T=00 K. (a) How many moles of gas are in the sample?

More information

(a) (i) One of the assumptions of the kinetic theory of gases is that molecules make elastic collisions. State what is meant by an elastic collision.

(a) (i) One of the assumptions of the kinetic theory of gases is that molecules make elastic collisions. State what is meant by an elastic collision. 1 (a) (i) One of the assumptions of the kinetic theory of gases is that molecules make elastic collisions. State what is meant by an elastic collision. State two more assumptions that are made in the kinetic

More information

PHY101: Major Concepts in Physics I. Photo: J. M. Schwarz

PHY101: Major Concepts in Physics I. Photo: J. M. Schwarz PHY101: Major Concepts in Physics I Photo: J. M. Schwarz Announcements We will be talking about the laws of thermodynamics today, which will help get you ready for next week s lab on the Stirling engine.

More information

Kinetic Theory 1 / Probabilities

Kinetic Theory 1 / Probabilities Kinetic Theory 1 / Probabilities 1. Motivations: statistical mechanics and fluctuations 2. Probabilities 3. Central limit theorem 1 Reading check Main concept introduced in first half of this chapter A)Temperature

More information

If the position of a molecule is measured after increments of 10, 100, 1000 steps, what will the distribution of measured steps look like?

If the position of a molecule is measured after increments of 10, 100, 1000 steps, what will the distribution of measured steps look like? If the position of a molecule is measured after increments of 10, 100, 1000 steps, what will the distribution of measured steps look like? (1) No longer Gaussian (2) Identical Gaussians (3) Gaussians with

More information

Chapter 15 Thermal Properties of Matter

Chapter 15 Thermal Properties of Matter Chapter 15 Thermal Properties of Matter To understand the mole and Avogadro's number. To understand equations of state. To study the kinetic theory of ideal gas. To understand heat capacity. To learn and

More information

- Apply closed system energy balances, observe sign convention for work and heat transfer.

- Apply closed system energy balances, observe sign convention for work and heat transfer. CHAPTER : ENERGY AND THE FIRST LAW OF THERMODYNAMICS Objectives: - In this chapter we discuss energy and develop equations for applying the principle of conservation of energy. Learning Outcomes: - Demonstrate

More information

Chapter 18 Thermal Properties of Matter

Chapter 18 Thermal Properties of Matter Chapter 18 Thermal Properties of Matter In this section we define the thermodynamic state variables and their relationship to each other, called the equation of state. The system of interest (most of the

More information

Chapter 10: Thermal Physics

Chapter 10: Thermal Physics Chapter 10: hermal Physics hermal physics is the study of emperature, Heat, and how these affect matter. hermal equilibrium eists when two objects in thermal contact with each other cease to echange energy.

More information

Chemistry 451. Prerequisites: CHEM 013, MATH 141, PHYS 202 or PHYS 212. Prof. Mueller/Sykes Chemistry 451 Spring 2004 Lecture 1-1

Chemistry 451. Prerequisites: CHEM 013, MATH 141, PHYS 202 or PHYS 212. Prof. Mueller/Sykes Chemistry 451 Spring 2004 Lecture 1-1 Chemistry 451 CHEM 451 PHYSICAL CHEMISTRY ( 3 credits) Introduction to chemical principles, including properties of matter and fundamentals of chemical thermodynamics. Prerequisites: CHEM 013, MATH 141,

More information

Rate of Heating and Cooling

Rate of Heating and Cooling Rate of Heating and Cooling 35 T [ o C] Example: Heating and cooling of Water E 30 Cooling S 25 Heating exponential decay 20 0 100 200 300 400 t [sec] Newton s Law of Cooling T S > T E : System S cools

More information

Ideal Gas Behavior. NC State University

Ideal Gas Behavior. NC State University Chemistry 331 Lecture 6 Ideal Gas Behavior NC State University Macroscopic variables P, T Pressure is a force per unit area (P= F/A) The force arises from the change in momentum as particles hit an object

More information

KINETIC THEORY OF GASES

KINETIC THEORY OF GASES KINETIC THEORY OF GASES VERY SHORT ANSWER TYPE QUESTIONS ( MARK). Write two condition when real gases obey the ideal gas equation ( nrt). n number of mole.. If the number of molecule in a container is

More information

MP :40-2:40 3:00-4:00 PM

MP :40-2:40 3:00-4:00 PM PHY294H l Professor: Joey Huston l email:huston@msu.edu l office: BPS3230 l Homework will be with Mastering Physics (and an average of 1 handwritten problem per week) Added problem 28.68 for 3 rd MP assignment

More information

Preliminary Examination - Day 2 Friday, August 12, 2016

Preliminary Examination - Day 2 Friday, August 12, 2016 UNL - Department of Physics and Astronomy Preliminary Examination - Day Friday, August 1, 016 This test covers the topics of Thermodynamics and Statistical Mechanics (Topic 1) and Mechanics (Topic ). Each

More information

Organization of NAMD Tutorial Files

Organization of NAMD Tutorial Files Organization of NAMD Tutorial Files .1.1. RMSD for individual residues Objective: Find the average RMSD over time of each residue in the protein using VMD. Display the protein with the residues colored

More information

Newton s Laws of Motion and Gravity ASTR 2110 Sarazin. Space Shuttle

Newton s Laws of Motion and Gravity ASTR 2110 Sarazin. Space Shuttle Newton s Laws of Motion and Gravity ASTR 2110 Sarazin Space Shuttle Discussion Session This Week Friday, September 8, 3-4 pm Shorter Discussion Session (end 3:40), followed by: Intro to Astronomy Department

More information

Physics 125, Spring 2006 Monday, May 15, 8:00-10:30am, Old Chem 116. R01 Mon. 12:50 R02 Wed. 12:50 R03 Mon. 3:50. Final Exam

Physics 125, Spring 2006 Monday, May 15, 8:00-10:30am, Old Chem 116. R01 Mon. 12:50 R02 Wed. 12:50 R03 Mon. 3:50. Final Exam Monday, May 15, 8:00-10:30am, Old Chem 116 Name: Recitation section (circle one) R01 Mon. 12:50 R02 Wed. 12:50 R03 Mon. 3:50 Closed book. No notes allowed. Any calculators are permitted. There are no trick

More information

Chapter 13: Temperature, Kinetic Theory and Gas Laws

Chapter 13: Temperature, Kinetic Theory and Gas Laws Chapter 1: Temperature, Kinetic Theory and Gas Laws Zeroth Law of Thermodynamics (law of equilibrium): If objects A and B are separately in thermal equilibrium with a third object C, then A and B are in

More information

PHY214 Thermal & Kinetic Physics Duration: 2 hours 30 minutes

PHY214 Thermal & Kinetic Physics Duration: 2 hours 30 minutes BSc Examination by course unit. Friday 5th May 01 10:00 1:30 PHY14 Thermal & Kinetic Physics Duration: hours 30 minutes YOU ARE NOT PERMITTED TO READ THE CONTENTS OF THIS QUESTION PAPER UNTIL INSTRUCTED

More information

IT IS THEREFORE A SCIENTIFIC LAW.

IT IS THEREFORE A SCIENTIFIC LAW. Now we talk about heat: Zeroth Law of Thermodynamics: (inserted after the 3 Laws, and often not mentioned) If two objects are in thermal equilibrium with a third object, they are in thermal equilibrium

More information

Physics 9 Wednesday, February 5, 2014

Physics 9 Wednesday, February 5, 2014 Physics 9 Wednesday, February 5, 2014 HW3 (fluids) due Friday. I reserved DRL 3W2 from 6:30pm to 9:30pm on Wednesdays (usually Zoey) and Thursdays (usually Bill) for HW help. Quiz #1 (10 minutes at end

More information

Kinetic Theory of Gases

Kinetic Theory of Gases Kinetic Theory of Gases Modern Physics September 7 and 12, 2016 1 Intro In this section, we will relate macroscopic properties of gases (like Pressure, Temperature) to the behavior of the microscopic components

More information

Please read the following instructions:

Please read the following instructions: MIDTERM #1 PHYS 33 (MODERN PHYSICS II) DATE/TIME: February 16, 17 (8:3 a.m. - 9:45 a.m.) PLACE: RB 11 Only non-programmable calculators are allowed. Name: ID: Please read the following instructions: This

More information

PV = n R T = N k T. Measured from Vacuum = 0 Gauge Pressure = Vacuum - Atmospheric Atmospheric = 14.7 lbs/sq in = 10 5 N/m

PV = n R T = N k T. Measured from Vacuum = 0 Gauge Pressure = Vacuum - Atmospheric Atmospheric = 14.7 lbs/sq in = 10 5 N/m PV = n R T = N k T P is the Absolute pressure Measured from Vacuum = 0 Gauge Pressure = Vacuum - Atmospheric Atmospheric = 14.7 lbs/sq in = 10 5 N/m V is the volume of the system in m 3 often the system

More information

Please read the following instructions:

Please read the following instructions: MIDTERM #1 PHYS 33 (MODERN PHYSICS II) DATE/TIME: February 16, 17 (8:3 a.m. - 9:45 a.m.) PLACE: RB 11 Only non-programmable calculators are allowed. Name: ID: Please read the following instructions: This

More information

Physics 231 Lecture 30. Main points of today s lecture: Ideal gas law:

Physics 231 Lecture 30. Main points of today s lecture: Ideal gas law: Physics 231 Lecture 30 Main points of today s lecture: Ideal gas law: PV = nrt = Nk BT 2 N 1 2 N 3 3 V 2 3 V 2 2 P = m v = KE ; KE KE = kbt Phases of Matter Slide 12-16 Ideal Gas: properties Approximate

More information

7. (2) Of these elements, which has the greatest number of atoms in a mole? a. hydrogen (H) b. oxygen (O) c. iron (Fe) d. gold (Au) e. all tie.

7. (2) Of these elements, which has the greatest number of atoms in a mole? a. hydrogen (H) b. oxygen (O) c. iron (Fe) d. gold (Au) e. all tie. General Physics I Exam 5 - Chs. 13,14,15 - Heat, Kinetic Theory, Thermodynamics Dec. 14, 2010 Name Rec. Instr. Rec. Time For full credit, make your work clear to the grader. Show formulas used, essential

More information

KINETIC MOLECULAR DESCRIPTION OF THE STATES OF MATTER

KINETIC MOLECULAR DESCRIPTION OF THE STATES OF MATTER KINETIC MOLECULAR DESCRIPTION OF THE STATES OF MATTER CHAPTER 9 The Gaseous State CHAPTER 10 Solids, Liquids, and Phase Transitions CHAPTER 11 Solutions 392 Gas Liquid Solid 9 THE GASEOUS STATE 9.1 The

More information

The Equipartition Theorem

The Equipartition Theorem Chapter 8 The Equipartition Theorem Topics Equipartition and kinetic energy. The one-dimensional harmonic oscillator. Degrees of freedom and the equipartition theorem. Rotating particles in thermal equilibrium.

More information

Speed Distribution at CONSTANT Temperature is given by the Maxwell Boltzmann Speed Distribution

Speed Distribution at CONSTANT Temperature is given by the Maxwell Boltzmann Speed Distribution Temperature ~ Average KE of each particle Particles have different speeds Gas Particles are in constant RANDOM motion Average KE of each particle is: 3/2 kt Pressure is due to momentum transfer Speed Distribution

More information

L = I ω = const. I = 2 3 MR2. When the balloon shrinks (because the air inside it cools down), the moment of inertia decreases, R = 1. L = I ω = I ω.

L = I ω = const. I = 2 3 MR2. When the balloon shrinks (because the air inside it cools down), the moment of inertia decreases, R = 1. L = I ω = I ω. PHY 30 K. Solutions for mid-term test #3. Problem 1: Out in space, there are no forces acting on the balloon except gravity and hence no torques (with respect to an axis through the center of mass). Consequently,

More information

An ideal gas. Ideal gas equation.

An ideal gas. Ideal gas equation. S t r o n a 1 Autor: Ryszard Świda An ideal gas. Ideal gas equation. To facilitate the application of physical theories, various physicals models are created and used. A physical model is a hypothetical

More information

A 1.6 N kg 1. B 5.0 N kg 1. C 10 N kg 1. D 20 N kg 1. Two stars of mass M and 4M are at a distance d between their centres.

A 1.6 N kg 1. B 5.0 N kg 1. C 10 N kg 1. D 20 N kg 1. Two stars of mass M and 4M are at a distance d between their centres. 1 planet has a radius half the Earth s radius and a mass a quarter of the Earth s mass. What is the approximate gravitational field strength on the surface of the planet? 1.6 N kg 1 5.0 N kg 1 10 N kg

More information

Molecular Motion and Gas Laws

Molecular Motion and Gas Laws Molecular Motion and Gas Laws What is the connection between the motion of molecules (F = ma and K = mv 2 /2) and the thermodynamics of gases (pv = nrt and U = 3nRT/2)? In this lab, you will discover how

More information

Kinetic Theory 1 / Probabilities

Kinetic Theory 1 / Probabilities Kinetic Theory 1 / Probabilities 1. Motivations: statistical mechanics and fluctuations 2. Probabilities 3. Central limit theorem 1 The need for statistical mechanics 2 How to describe large systems In

More information

Exam 2. May 21, 2008, 8:00am

Exam 2. May 21, 2008, 8:00am PHYSICS 101: Fundamentals of Physics Exam 2 Exam 2 Name TA/ Section # May 21, 2008, 8:00am Recitation Time You have 1 hour to complete the exam. Please answer all questions clearly and completely, and

More information

SAIOH Tutorial Ventilation 1 pressures and basic air flow calculations

SAIOH Tutorial Ventilation 1 pressures and basic air flow calculations SAIOH Tutorial Ventilation 1 pressures and basic air flow calculations Acknowledgement This tutorial was provided by SAIOH as an assessment support aid for prospective candidates. The tutorial is free

More information

4. All questions are NOT ofequal value. Marks available for each question are shown in the examination paper.

4. All questions are NOT ofequal value. Marks available for each question are shown in the examination paper. THE UNIVERSITY OF NEW SOUTH WALES SCHOOL OF PHYSICS \1111~11\llllllllllllftllll~flrllllllllll\11111111111111111 >014407892 PHYS2060 THER1\1AL PHYSICS FINAL EXAMINATION SESSION 2 - NOVEMBER 2010 I. Time

More information

BCIT Fall Chem Exam #1

BCIT Fall Chem Exam #1 BCIT Fall 2012 Chem 3615 Exam #1 Name: Attempt all questions in this exam. Read each question carefully and give a complete answer in the space provided. Part marks given for wrong answers with partially

More information

Equations: q trans = 2 mkt h 2. , Q = q N, Q = qn N! , < P > = kt P = , C v = < E > V 2. e 1 e h /kt vib = h k = h k, rot = h2.

Equations: q trans = 2 mkt h 2. , Q = q N, Q = qn N! , < P > = kt P = , C v = < E > V 2. e 1 e h /kt vib = h k = h k, rot = h2. Constants: R = 8.314 J mol -1 K -1 = 0.08206 L atm mol -1 K -1 k B = 0.697 cm -1 /K = 1.38 x 10-23 J/K 1 a.m.u. = 1.672 x 10-27 kg 1 atm = 1.0133 x 10 5 Nm -2 = 760 Torr h = 6.626 x 10-34 Js For H 2 O

More information

Chemical Thermodynamics : Georg Duesberg

Chemical Thermodynamics : Georg Duesberg The Properties of Gases Kinetic gas theory Maxwell Boltzman distribution, Collisions Real (non-ideal) gases fugacity, Joule Thomson effect Mixtures of gases Entropy, Chemical Potential Liquid Solutions

More information

Stuff. ---Tonight: Lecture 3 July Assignment 1 has been posted. ---Presentation Assignment on Friday.

Stuff. ---Tonight: Lecture 3 July Assignment 1 has been posted. ---Presentation Assignment on Friday. Stuff ---Tonight: Lecture 3 July 0 ---Assignment 1 has been posted. Work from gravitational forces: h F gravity dx = h 0 0 mgh mg dx Where m (kg) and g is gravitational constant 9.8 m/s ---Presentation

More information

Physics 111. Lecture 34 (Walker 17.2,17.4-5) Kinetic Theory of Gases Phases of Matter Latent Heat

Physics 111. Lecture 34 (Walker 17.2,17.4-5) Kinetic Theory of Gases Phases of Matter Latent Heat Physics 111 Lecture 34 (Walker 17.2,17.4-5) Kinetic Theory of Gases Phases of Matter Latent Heat Dec. 7, 2009 Kinetic Theory Pressure is the result of collisions between gas molecules and walls of container.

More information

QuickCheck. Collisions between molecules. Collisions between molecules

QuickCheck. Collisions between molecules. Collisions between molecules Collisions between molecules We model molecules as rigid spheres of radius r as shown at the right. The mean free path of a molecule is the average distance it travels between collisions. The average time

More information

Physics 213 Spring 2009 Midterm exam. Review Lecture

Physics 213 Spring 2009 Midterm exam. Review Lecture Physics 213 Spring 2009 Midterm exam Review Lecture The next two questions pertain to the following situation. A container of air (primarily nitrogen and oxygen molecules) is initially at 300 K and atmospheric

More information

Announcements 13 Nov 2014

Announcements 13 Nov 2014 Announcements 13 Nov 2014 1. Prayer 2. Exam 3 starts on Tues Nov 25 a. Covers Ch 9-12, HW 18-24 b. Late fee on Wed after Thanksgiving, 3 pm c. Closes on Thursday after Thanksgiving, 3 pm d. Jerika review

More information

Relationship between POTENTIAL ENERGY and FORCE

Relationship between POTENTIAL ENERGY and FORCE PH-211 Relationship between POTENTIAL ENERGY and FORCE Knowing F at every place, we defined the corresponding potential energy function U. Here we explore: Given U, how to find F? A. La Rosa = Becomes

More information

Chapter 3 First Law of Thermodynamics and Energy Equation

Chapter 3 First Law of Thermodynamics and Energy Equation Fundamentals of Thermodynamics Chapter 3 First Law of Thermodynamics and Energy Equation Prof. Siyoung Jeong Thermodynamics I MEE0-0 Spring 04 Thermal Engineering Lab. 3. The energy equation Thermal Engineering

More information

Ch 18. Kinetic Theory of Gases

Ch 18. Kinetic Theory of Gases Physics 5D: Heat, Thermo, Kinetics Ch 18. Kinetic Theory of Gases Prof. Joel Primack 318 ISB 459-2580 joel@physics.ucsc.edu Text Copyright Text 2009 Pearson Text Education, Text Inc. Neuschwanstein Bavaria

More information

Massachusetts Institute of Technology - Physics Department

Massachusetts Institute of Technology - Physics Department Massachusetts Institute of Technology - Physics Department Physics - 8.01 Assignment #4 October 6, 1999. It is strongly recommended that you read about a subject before it is covered in lectures. Lecture

More information

Physics 4230 Final Examination 10 May 2007

Physics 4230 Final Examination 10 May 2007 Physics 43 Final Examination May 7 In each problem, be sure to give the reasoning for your answer and define any variables you create. If you use a general formula, state that formula clearly before manipulating

More information

Collisions between molecules

Collisions between molecules Collisions between molecules We model molecules as rigid spheres of radius r as shown at the right. The mean free path of a molecule is the average distance it travels between collisions. The average time

More information

Thermal Physics. 1) Thermodynamics: Relates heat + work with empirical (observed, not derived) properties of materials (e.g. ideal gas: PV = nrt).

Thermal Physics. 1) Thermodynamics: Relates heat + work with empirical (observed, not derived) properties of materials (e.g. ideal gas: PV = nrt). Thermal Physics 1) Thermodynamics: Relates heat + work with empirical (observed, not derived) properties of materials (e.g. ideal gas: PV = nrt). 2) Statistical Mechanics: Uses models (can be more complicated)

More information

UNIVERSITY OF OSLO FACULTY OF MATHEMATICS AND NATURAL SCIENCES

UNIVERSITY OF OSLO FACULTY OF MATHEMATICS AND NATURAL SCIENCES UNIVERSITY OF OSLO FCULTY OF MTHEMTICS ND NTURL SCIENCES Exam in: FYS430, Statistical Mechanics Day of exam: Jun.6. 203 Problem :. The relative fluctuations in an extensive quantity, like the energy, depends

More information

Chapter 6 Free Electron Fermi Gas

Chapter 6 Free Electron Fermi Gas Chapter 6 Free Electron Fermi Gas Free electron model: The valence electrons of the constituent atoms become conduction electrons and move about freely through the volume of the metal. The simplest metals

More information

Lecture 25 Goals: Chapter 18 Understand the molecular basis for pressure and the idealgas

Lecture 25 Goals: Chapter 18 Understand the molecular basis for pressure and the idealgas Lecture 5 Goals: Chapter 18 Understand the molecular basis for pressure and the idealgas law. redict the molar specific heats of gases and solids. Understand how heat is transferred via molecular collisions

More information

Alternate Midterm Examination Physics 100 Feb. 20, 2014

Alternate Midterm Examination Physics 100 Feb. 20, 2014 Alternate Midterm Examination Physics 100 Feb. 20, 2014 Name/Student #: Instructions: Formulas at the back (you can rip that sheet o ). Questions are on both sides. Calculator permitted. Put your name

More information

Chapter 10. Thermal Physics

Chapter 10. Thermal Physics Chapter 10 Thermal Physics Thermal Physics Thermal physics is the study of Temperature Heat How these affect matter Thermal Physics, cont Descriptions require definitions of temperature, heat and internal

More information

A Study of the Thermal Properties of a One. Dimensional Lennard-Jones System

A Study of the Thermal Properties of a One. Dimensional Lennard-Jones System A Study of the Thermal Properties of a One Dimensional Lennard-Jones System Abstract In this study, the behavior of a one dimensional (1D) Lennard-Jones (LJ) system is simulated. As part of this research,

More information

KINETIC THEORY OF GASES

KINETIC THEORY OF GASES LECTURE 8 KINETIC THEORY OF GASES Text Sections 0.4, 0.5, 0.6, 0.7 Sample Problems 0.4 Suggested Questions Suggested Problems Summary None 45P, 55P Molecular model for pressure Root mean square (RMS) speed

More information

fiziks Institute for NET/JRF, GATE, IIT JAM, JEST, TIFR and GRE in PHYSICAL SCIENCES Kinetic Theory, Thermodynamics OBJECTIVE QUESTIONS IIT-JAM-2005

fiziks Institute for NET/JRF, GATE, IIT JAM, JEST, TIFR and GRE in PHYSICAL SCIENCES Kinetic Theory, Thermodynamics OBJECTIVE QUESTIONS IIT-JAM-2005 Institute for NE/JRF, GAE, II JAM, JES, IFR and GRE in HYSIAL SIENES Kinetic heory, hermodynamics OBJEIE QUESIONS II-JAM-005 5 Q. he molar specific heat of a gas as given from the kinetic theory is R.

More information

PHYS 352 Homework 2 Solutions

PHYS 352 Homework 2 Solutions PHYS 352 Homework 2 Solutions Aaron Mowitz (, 2, and 3) and Nachi Stern (4 and 5) Problem The purpose of doing a Legendre transform is to change a function of one or more variables into a function of variables

More information

Introduction Statistical Thermodynamics. Monday, January 6, 14

Introduction Statistical Thermodynamics. Monday, January 6, 14 Introduction Statistical Thermodynamics 1 Molecular Simulations Molecular dynamics: solve equations of motion Monte Carlo: importance sampling r 1 r 2 r n MD MC r 1 r 2 2 r n 2 3 3 4 4 Questions How can

More information

CH10007/87. Thermodynamics. Dr Toby Jenkins

CH10007/87. Thermodynamics. Dr Toby Jenkins CH10007/87 Thermodynamics Dr Toby Jenkins 1 Objectives To introduce the basic concepts of thermodynamics To apply them to chemical systems To develop competence in thermodynamics calculations 2 Equilibrium

More information

Kinetic Theory: Atomic and Molecular Explanation of Pressure and Temperature

Kinetic Theory: Atomic and Molecular Explanation of Pressure and Temperature Kinetic Theory: Atomic and Molecular Explanation of Pressure and Temperature Bởi: OpenStaxCollege We have developed macroscopic definitions of pressure and temperature. Pressure is the force divided by

More information

Atoms, electrons and Solids

Atoms, electrons and Solids Atoms, electrons and Solids Shell model of an atom negative electron orbiting a positive nucleus QM tells that to minimize total energy the electrons fill up shells. Each orbit in a shell has a specific

More information

PhysicsAndMathsTutor.com 1 2 (*) (1)

PhysicsAndMathsTutor.com 1 2 (*) (1) PhysicsAndMathsTutor.com 1 1. (a) pressure (*) Pa or N m volume m (*) (*) (not allow kpa) number of moles mol (or none) molar gas constant J K 1 mol 1 (mol 1 implies molar) temperature K 4 (b) (i) W(=

More information

Welcome Back! Physics Coulomb s Law. Charles-Augustin de Coulomb Physics 1308: General Physics II - Professor Jodi Cooley

Welcome Back! Physics Coulomb s Law. Charles-Augustin de Coulomb Physics 1308: General Physics II - Professor Jodi Cooley Welcome Back! Physics 1308 Coulomb s Law Charles-Augustin de Coulomb 1736-1806 Announcements Assignments for Tuesday, August 28th: - Reading: Chapter 22.1-22.2 - Watch Video: https://youtu.be/tzq79csdttw

More information

17-1 Ideal Gases. Gases are the easiest state of matter to describe - All ideal gases exhibit similar behavior.

17-1 Ideal Gases. Gases are the easiest state of matter to describe - All ideal gases exhibit similar behavior. 17-1 Ideal Gases Gases are the easiest state of matter to describe - All ideal gases exhibit similar behavior. An ideal gas is one that is thin enough, that the interactions between molecules can be ignored.

More information

Chem 105 Friday 3 Dec 2010

Chem 105 Friday 3 Dec 2010 Chem 105 Friday 3 Dec 010 Today: Kinetic-molecular theory Diffusion and effusion Course Questionnaires Real gases & Van der Waals equation Hour Exam 4 (Chap 9, 10, 11) Friday. Dec 10 A practice exam will

More information

Kinetic Theory of Aether Particles

Kinetic Theory of Aether Particles Chapter 2 Kinetic Theory of Aether Particles 2.1 Basic Concepts and Assumptions This chapter will derive energy density and pressure from particles collision on a surface based on kinetic theory. Kinetic

More information

Physics A - PHY 2048C

Physics A - PHY 2048C Kinetic Mechanical Physics A - PHY 2048C and 11/01/2017 My Office Hours: Thursday 2:00-3:00 PM 212 Keen Building Warm-up Questions Kinetic Mechanical 1 How do you determine the direction of kinetic energy

More information

Newton s Gravitational Law

Newton s Gravitational Law 1 Newton s Gravitational Law Gravity exists because bodies have masses. Newton s Gravitational Law states that the force of attraction between two point masses is directly proportional to the product of

More information

Order of Magnitude Astrophysics - a.k.a. Astronomy 111. Photon Opacities in Matter

Order of Magnitude Astrophysics - a.k.a. Astronomy 111. Photon Opacities in Matter 1 Order of Magnitude Astrophysics - a.k.a. Astronomy 111 Photon Opacities in Matter If the cross section for the relevant process that scatters or absorbs radiation given by σ and the number density of

More information

PHYSICS 126 Fall 2010 Midterm 1

PHYSICS 126 Fall 2010 Midterm 1 PHYSICS 16 Fall 010 Midterm 1 Name: SOLUTIONS Student ID: Section Number: Closed book with one sheet of notes and a calculator. Answer the questions in spaces provided on each sheet. If you run out of

More information

Physics 2010 Work and Energy Recitation Activity 5 (Week 9)

Physics 2010 Work and Energy Recitation Activity 5 (Week 9) Physics 2010 Work and Energy Recitation Activity 5 (Week 9) Name Section Tues Wed Thu 8am 10am 12pm 2pm 1. The figure at right shows a hand pushing a block as it moves through a displacement Δ! s. a) Suppose

More information

Perfect Guide. Notes. 2nd Edition. Ryan Bong

Perfect Guide. Notes. 2nd Edition. Ryan Bong Perfect Guide `O Level PHYSICS PHYSICS Notes 2nd Edition Ryan Bong 72 Preface PERFECT GUIDE TO O LEVEL PHYSICS NOTES (2nd Edition) is a study aid for the G.C.E. O Level Physics examination. With comprehensive

More information

Physics 8 Wednesday, November 9, 2011

Physics 8 Wednesday, November 9, 2011 Physics 8 Wednesday, November 9, 2011 For HW8 problems to sketch out in class, I got 5 requests for # 9 3 requests for # 3 2 requests for # 14 1 request each for # 2, 7, 10, 11, 15, 19 I will be in DRL

More information

(b) Explain how the principle of conservation of momentum is a natural consequence of Newton s laws of motion. [3]

(b) Explain how the principle of conservation of momentum is a natural consequence of Newton s laws of motion. [3] Physics A Unit: G484: The Newtonian World 1(a) State Newton s second law of motion. The force acting on an object equals the rate of change of momentum of the object. In part (a) equals should have been

More information

What is Work? W = Fd. Whenever you apply a force to an object and the object moves in the direction of the force, work is done.

What is Work? W = Fd. Whenever you apply a force to an object and the object moves in the direction of the force, work is done. Year 10 Physics What is Work? Whenever you apply a force to an object and the object moves in the direction of the force, work is done. If force is measured in newtons (N) and distance moved in metres,

More information

Wiley Plus Reminder! Assignment 1

Wiley Plus Reminder! Assignment 1 Wiley Plus Reminder! Assignment 1 6 problems from chapters and 3 Kinematics Due Monday October 5 Before 11 pm! Chapter 4: Forces and Newton s Laws Force, mass and Newton s three laws of motion Newton s

More information

PA02. General Certificate of Education June 2006 Advanced Subsidiary Examination

PA02. General Certificate of Education June 2006 Advanced Subsidiary Examination Surname Centre Number Other Names Candidate Number Leave blank Candidate Signature General Certificate of Education June 2006 Advanced Subsidiary Examination PHYSICS (SPECIFICATION A) Unit 2 Mechanics

More information

Slide 1-2. Slide 3-4. Slide 5-6. Review from Physics 114. Gasses. Three possible mechanisms that explain how the alcohol disappears

Slide 1-2. Slide 3-4. Slide 5-6. Review from Physics 114. Gasses. Three possible mechanisms that explain how the alcohol disappears Slide 1-2 Review from Physics 114 Gasses Physics 115 Eyres Draw force diagrams (FBDs) (Section 2.1). Use Newton's second and third laws to analyze interactions of objects (Section 2.8). Use the impulse-momentum

More information

Chapter 17 Temperature & Kinetic Theory of Gases 1. Thermal Equilibrium and Temperature

Chapter 17 Temperature & Kinetic Theory of Gases 1. Thermal Equilibrium and Temperature Chapter 17 Temperature & Kinetic Theory of Gases 1. Thermal Equilibrium and Temperature Any physical property that changes with temperature is called a thermometric property and can be used to measure

More information

PHYSICS 100. Introduction to Physics. Bridges the gap between school science and Physics 101, Physics 120, Physics 125 or Physics 140

PHYSICS 100. Introduction to Physics. Bridges the gap between school science and Physics 101, Physics 120, Physics 125 or Physics 140 PHYSICS 100 Introduction to Physics Bridges the gap between school science and Physics 101, Physics 120, Physics 125 or Physics 140 Only for those WITHOUT Physics 12 or equiv. (C+ or better). If you have

More information

Chapter 16 Simple Kinetic Theory of Matter

Chapter 16 Simple Kinetic Theory of Matter Chapter 16 Simple Kinetic Theory of Matter MCQ 1: Air trapped inside a single-piston-cylinder exerts a pressure of 760 mmhg. If its volume is increased by 30% at a constant temperature, then the pressure

More information

Lecture 25 Thermodynamics, Heat and Temp (cont.)

Lecture 25 Thermodynamics, Heat and Temp (cont.) Lecture 25 Thermodynamics, Heat and Temp (cont.) Heat and temperature Gases & Kinetic theory http://candidchatter.files.wordpress.com/2009/02/hell.jpg Specific Heat Specific Heat: heat capacity per unit

More information

Physics 161 Lecture 14 Kinetic Theory of Gas. October 18, 2018

Physics 161 Lecture 14 Kinetic Theory of Gas. October 18, 2018 Physics 161 Lecture 14 Kinetic Theory of Gas October 18, 2018 1 Exam 1, Thursday 18 Oct The exam will start promptly at 10:00pm. You will be permitted to open your exam at 10:00pm. You will have until

More information