View on Cold in 17th Century

Slides:



Advertisements
Similar presentations
Chapter 2 Statistical Thermodynamics. 1- Introduction - The object of statistical thermodynamics is to present a particle theory leading to an interpretation.
Advertisements

Temperature 1.  Temperature is defined as the degree of hotness or coldness of a body measured on a definite scale  Temperature is the driving force.
Reference Book is. TEMPERATURE AND THE ZEROTH LAW OF THERMODYNAMICS TEMPERATURE AND THE ZEROTH LAW OF THERMODYNAMICS * Two objects are in Thermal contact.
Chapter 18 Temperature, Heat, and the First Law of Thermodynamics.
Chapter 5 Temperature and Heat Another Kind of Energy.
Chapter 16 Temperature and the Kinetic Theory of Gases.
Too many particles… can’t keep track! Use pressure (p) and volume (V) instead. Temperature (T) measures the tendency of an object to spontaneously give.
Kinetic Molecular Theory of Matter
1 Thermal Physics Chapter Thermodynamics Concerned with the concepts of energy transfers between a system and its environment and the resulting.
Chapter-18 Temperature, Heat and the First Law of Thermodynamics.
Dr.Salwa Al Saleh Lecture 11 Thermodynamic Systems Specific Heat Capacities Zeroth Law First Law.
STATES OF MATTER Unit 6 Ch 3.2 Ppt Describing the states of matter… Materials can be classified as solids, liquids, or gases based on whether their shapes.
Kinetic Molecular Theory and the Gas Laws Phases of Matter, Kinetic Molecular Theory, and Temperature Gas Laws Phase Changes.
Temperature and Kinetic Theory Atomic Theory of Matter Temperature and Thermometers Thermal Equilibrium and the Zeroth Law of Thermodynamics Thermal Expansion.
Physics 101 Lecture 11. Thermal Physics Thermodynamics.
View on Cold in 17 th Century …while the sources of heat were obvious – the sun, the crackle of a fire, the life force of animals and human beings – cold.
Thermal Physics Chapter 10. Thermodynamics Concerned with the concepts of energy transfers between a system and its environment and the resulting temperature.
Too many particles… can’t keep track! Use pressure (p) and volume (V) instead. Thermal Physics.
Physics 101 Lecture 10. Thermal Physics Applications of Newton’s Laws to Large Number of Particles Can’t apply Newton’s Laws to large number of particles.
CHAPTER 12 SOLIDS, LIQUIDS, AND GASES HONORS CHEMISTRY.
KINETIC THEORY AND TEMPERATURE. Kinetic Theory Kinetic Theory: all particles of matter are in constant motion Kinetic energy: the energy that comes from.
Chemistry 231 Thermochemistry.
Section 1 The Kinetic-Molecular Theory of Matter
Temperature and Kinetic Theory
Thermal Physics Too many particles… can’t keep track!
“Teach A Level Maths” Statistics 1
Temperature.
Chapter 7 Lesson Starter
Kinetic theory and temperature
“Teach A Level Maths” Statistics 1
and Statistical Physics
States of Matter Chapter 3 pg. 68 – 97 Chapter
Temperature.
CHAPTER 8 - FLUID MECHANICS
Heat versus Temperature
What is Temperature? Observation: When objects are placed near each other, they may change, even if no work is done. (Example: when you put water from.
Temperature, Heat, and the First Law of Thermodynamics
THERMODYNAMICS AND ENERGY
Thermodynamic.
Changing States of Matter
Possible Changes of State
Chapter 7: Thermal Properties of Matter
PURE SUBSTANCE Pure substance: A substance that has a fixed chemical composition throughout. Air is a mixture of several gases, but it is considered to.
Lecture 8-- CALM Explain as succinctly as you can, and in your own words, why, of all possible heat engines acting between two reservoirs of fixed temperature.
Temperature & the Laws of Thermodynamics Lecture Notes
Section 3.5: Temperature.
Changing States of Matter
Chapter 16 Temperature and Heat.
S-94 List and define the three states of matter..
Thermal Physics Too many particles… can’t keep track!
Temperature, Heat and the First Law of Thermodynamics
Kinetic Theory and a Model for Gases
The Nature of Energy 1.
“Teach A Level Maths” Statistics 1
Thermal Physics Too many particles… can’t keep track!
Bernoulli's choice: Heads or Tails?
Possible Changes of State
Chapter 13 Phase Changes Notes #8b.
Temperature, Heat, and the First Law of Thermodynamics
Unit 1 Introduction to Matter
View on Cold in 17th Century
Pascal’s Arithmetic Triangle
Notes Ch Changes of State
States of Matter Chapter 13.
72 24) 20/ ) S = {hhh, hht, hth, thh, tth, tht, htt, ttt} 10%
13.4 Sublimation The change of a substance from a solid to a vapor without passing through the liquid state is called sublimation. Sublimation occurs.
Thermal Equilibrium Temperature Scale Practical Thermometers
Unit 1 Introduction to Matter
Chapter 3 Review.
Temperature Kelvin Scale Fahrenheit Scale Celsius Scale.
Presentation transcript:

View on Cold in 17th Century …while the sources of heat were obvious – the sun, the crackle of a fire, the life force of animals and human beings – cold was a mystery without an obvious source, a chill associated with death, inexplicable, too fearsome to investigate. “Absolute Zero and the Conquest of Cold” by T. Shachtman Heat “energy in transit” flows from hot to cold: (Thot > Tcold) Thermal equilibrium “thermalization” is when Thot = Tcold Arrow of time, irreversibility, time reversal symmetry breaking

Zeroth law of thermodynamics B Diathermal wall If two systems are separately in thermal equilibrium with a third system, they are in thermal equilibrium with each other. C can be considered the thermometer. If C is at a certain temperature then A and B are also at the same temperature.

Simplified constant-volume gas thermometer Pressure (P = gh) is the thermometric property that changes with temperature and is easily measured.

Temperature scales Assign arbitrary numbers to two convenient temperatures such as melting and boiling points of water. 0 and 100 for the Celsius (or Celcius) scale. Take a certain property of a material and say that it varies linearly with temperature. X = aT + b For a gas thermometer: P = aT + b

Gas Pressure Thermometer Ice point LN2 Steam point

Gas Pressure Thermometer Celsius scale P = a[T(oC) + 273.15] Ice point Steam point LN2

Phase diagram of water The single combination of pressure and temperature at which liquid water, solid ice, and water vapour can coexist in a stable equilibrium occurs at exactly 273.16 K (0.01 °C) and a partial vapour pressure of 611.73 pascals (ca. 6.1173 millibars, 0.0060373057 atm). At that point, it is possible to change all of the substance to ice, water, or vapor on making arbitrarily small changes in pressure and temperature. Note that even if the total pressure of a system is well above triple point of water, provided the partial pressure of the water vapour is 611.73 pascals then the system can still be brought to the triple point of water. Strictly speaking, the surfaces separating the different phases should also be perfectly flat, to abnegate the effects of surface tensions. Water has an unusual and complex phase diagram, although this does not affect general comments about the triple point. At high temperatures, increasing pressure results first in liquid and then solid water. (Above around 109 Pa a crystalline form of ice forms that is denser than liquid water.) At lower temperatures under compression, the liquid state ceases to appear, and water passes directly from gas to solid. At constant pressures above the triple point, heating ice causes it to pass from solid to liquid to gas, or steam, also known as water vapour. At pressures below the triple point, such as those that occur in outer space, where the pressure is near zero, liquid water cannot exist. In a process known as sublimation, ice skips the liquid stage and becomes steam when heated. Near triple point can have ice, water, or vapor on making arbitrarily small changes in pressure and temperature.

Concept of Absolute Zero (1703) Guillaume Amonton first derived mathematically the idea of absolute zero based on Boyle-Mariotte’s law in 1703. For a fixed amount of gas in a fixed volume, p = kT Amonton’s absolute zero ≈ 33 K

Other Types of Thermometer Metal resistor : R = aT + b Semiconductor : R = R0exp(-Eg/kBT) Thermocouple : E = aT + bT2 Low Temperature Thermometry

Platinum resistance thermometer

CERNOX thermometer Insensitive to magnetic fields !

International Temperature Scale of 1990 1. Units of Temperature The unit of the fundamental physical quantity known as thermodynamic temperature, symbol T, is the kelvin, symbol K, defined as the fraction 1/273.16 of the thermodynamic temperature of the triple point of water1. Because of the way earlier temperature scales were defined, it remains common practice to express a temperature in terms of its difference from 273.15 K, the ice point. A thermodynamic temperature, T, expressed in this way is known as a Celsius temperature, symbol t, defined by: t / °C = T/K - 273.15 .     (1) The unit of Celsius temperature is the degree Celsius, symbol °C, which is by definition equal in magnitude to the kelvin. A difference of temperature may be expressed in kelvins or degrees Celsius. The International Temperature Scale of 1990 (ITS-90) defines both International Kelvin Temperatures, symbol T90, and International Celsius Temperatures, symbol t90. The relation between T90 and t90, is the same as that between T and t, i.e.: t90 / °C = T90/K - 273.15 .     (2) The unit of the physical quantity T90 is the kelvin, symbol K, and the unit of the physical quantity t90, is the degree Celsius, symbol °C, as is the case for the thermodynamic temperature T and the Celsius temperature t.

Bernoulli's choice: Heads or Tails? N = # of slots, # of macrostates  = multiplicity, # of microstates Pascal’s triangle N 1 2 3 4 5 =2N 20 21 22 23 24 25 1 1 1 1 2 1 1 3 3 1 1 4 6 4 1 1 5 10 10 5 1 Example: For N=4 fair coin tosses there are N+1=5 macrostates each containing n heads where n = 0, 1, 2, 3, 4. Each macrostate has 4Cn occurrences of n heads with a total # of microstates equal to the multiplicity .

16 different configurations (microstates), 5 different macrostates Prob. (microstate) Macrostates: n,m Macrostate: n-m hhhh 1/16 4, 0 4 thhh 3, 1 2 hthh hhth hhht tthh 2, 2 thth htht hhtt htth thht httt 1, 3 -2 thtt ttht ttth tttt 0, 4 -4 16 different configurations (microstates), 5 different macrostates

Most likely macrostate the system will find itself in is the one with the maximum number of microstates. (50h for 100 tosses) Number of Microstates () Macrostate

Ensemble: All the parts of a thing taken together, so that each part is considered only in relation to the whole.

The most likely macrostate the system will find itself in is the one with the maximum number of microstates. E1 1(E1) E2 2(E2)

Microcanonical ensemble: Total system ‘1+2’ contains 20 energy quanta and 100 levels. Subsystem ‘1’ containing 60 levels with total energy x is in equilibrium with subsystem ‘2’ containing 40 levels with total energy 20-x. At equilibrium (max), x=12 energy quanta in ‘1’ and 8 energy quanta in ‘2’

Microcanonical ensemble: An ensemble of snapshots of a system with the same N, V, and E A collection of systems that each have the same fixed energy. E (E)

Canonical ensemble: An ensemble of snapshots of a system with the same N, V, and T (red box with energy  << E. Exchange of energy with reservoir. E- (E-)  I()

1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1 1

Canonical ensemble: P()  (E-)1  exp[-/kBT] Log10 (P()) Total system ‘1+2’ contains 20 energy quanta and 100 levels. x-axis is # of energy quanta in subsystem ‘1’ in equilibrium with ‘2’ y-axis is log10 of corresponding multiplicity of reservoir ‘2’