Review of classical thermodynamics

Size: px
Start display at page:

Download "Review of classical thermodynamics"

Transcription

1 Review of lassial thermodynamis Fundamental Laws, roperties and roesses () First Law - Energy Balane hermodynami funtions of state Internal energy, heat and work ypes of paths (isobari, isohori, isothermal, adiabati, yli) Enthalpy, heat apaity, heat of formation, phase transformations Calulation of enthalpy as a funtion of temperature Heats of reations and the Hess s law Reading: Chapters, 6., 6.4 of Gaskell or the same material in any other textbook on thermodynamis MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

2 hermodynami variables What are thermodynamis variables? here are two approahes to desribe properties and behavior of a material:. Mirosopi approah - to desribe the material in terms of mirosopi variables (positions, veloities, harges, et. of all partiles in the system). But there are too many partiles (N A = mol - ) and this approah in unpratial in most ases.. Classial (ontinuum) thermodynamis to desribe the material in terms of average quantities, or thermodynami variables, suh as temperature, internal energy, pressure, et. Statistial thermodynamis provides the onnetion between the lassial thermodynamis and the behavior of the mirosopi onstituents of matter (atoms and moleules). Although in this ourse we will fous on lassial thermodynamis, we will also onsider a few elements of statistial thermodynamis, in partiular in our disussion of heat apaity and entropy. What are state variables and funtions? System at equilibrium an be desribed by a number of thermodynami variables that are independent of the history of the system. Suh variables are alled state variables or state funtions depending on the ontext. We an desribe a system by a set of independent state variables and we an express other variables (state funtions) through this set of independent variables. For example, we an desribe ideal gas by and and use = R/ to define molar volume. For different appliations we an hoose different sets of independent variables that are the most onvenient. MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

3 Intensive and extensive variables hermodynami variables Intensive properties independent of the size of the system, e.g.,. Extensive properties proportional to the quantity of material, e.g.,, C, H, S, G. + = + Example: if = = = then = + but = = We an also onsider derived intensive variables, e.g., Mass/olume or Energy/olume, that do not depend on the size of the system. Internal energy, heat, and work: not very rigorous definitions: It is impossible to give a rigorous definition of energy. (...in physis today, we have no knowledge of what energy is. - the Feynman Letures on hysis). hermodynamis laws do not define energy, thermodynamis is dealing with transfer of energy. In partiular, the st law of thermodynamis postulates the energy onservation. In thermodynamis of materials we usually do not onsider the kineti energy of the enter-of-mass motion of the system or gravitational energy (mgh), only internal energy, intrinsi to the body is onsidered. Internal energy is a sum of all potential and kineti energies in the system (not only of thermal/mehanial origin). hermodynamis is only dealing with hange of. he absolute value of is not defined by the laws of thermodynamis, but an arbitrary zero point is often hosen for onveniene. MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

4 Early theory of heat: the alori fluid Frenh hemist Antoine-Laurent Lavoisier: he substane of heat is a subtle fluid alled alori the quantity of this substane is onstant throughout the universe, and it flows from warmer to older bodies. Based on observations that heat is onserved in some ases (e.g., when mixing hot and old water), Lavoisier proposed in 789 that heat is transferred by weightless, onserved fluid, named alori. Lavoisier's able of Simple Substanes (Elements) While we know that the alori ideas are invalid, we still say things like "heat flows to desribe the heat transfer MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

5 Heat generated from frition in annon boring proess, English physiist Benjamin hompson: Equivalene of heat and work I was struk with the very onsiderable degree of heat whih a brass gun aquires, in a short time, in being bored; [ ] A thorough investigating of these phenomena seemed even to bid fair to give a farther insight into the hidden nature of heat; and to enable us to form some reasonable onjetures respeting the existene, or non-existene, of an igneous fluid: a subjet on whih the opinions of philosophers have, in all ages, been muh divided. B. homson, hilosophial ransations, ol. XIII, 86, 798 Joule's experiment: the mehanial energy an be measured simultaneously with temperature (thermal energy). Joule found that the loss in mehanial energy is proportional to an inrease in temperature of the water and the amount of water used. the onstant or proportionality is 4.4 J/g ºC (modern data is 4.86 J/g ºC) Heat and work an independently produe idential hanges in the system. is not a good measure of heat but heat an be measured through work, and heat apaity an be determined. J.. Joule, On the existene of an equivalent relation between heat and the ordinary forms of mehanial power, hil. Mag. 7, 05, 845. MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

6 Energy, heat, and work (ontinued) Heat is the energy being transferred to a system as a result of temperature differene (work-less transfer of internal energy). Work an be defined as the energy being transferred to a system as a result of a (generalized) fore ating over a (generalized) distane. Examples of work: Mehanial work done by fore F on a body moving from r to r along a ertain trajetory or path: r δw F dr F dr Work due to the volume expansion of a fluid or gas done against an external pressure. Eletri polarization work, where the generalized fore is the strength of the eletri field, E, and the generalized displaement is the polarization of the medium, D. δw E dd Magneti work, where the generalized fore is the strength of the magneti field, H, and the generalized displaement is the total magneti dipole moment, B. δw δw d H db r path integral Work and heat are both funtions of the path of the proess they are not state funtions. Systems never possess heat and work! Heat and work are transient phenomena desribe energy being transferred to/from the system. MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

7 st Law onservation of energy in a thermodynami proess A state funtion, alled the internal energy, exists for any physial system and the hange in the internal energy during any proess is the sum of work done on/by the system and heat transferred to/from the system. = q w or in differential form: d = q - w internal energy (all potential and kineti energies). It is a state funtion depends only on thermodynami state of the system (e.g.,, & for a simple system). q energy added into the system as heat. ositive (+) when the system gains heat from outside (endothermi proess), negative (-) when heat flows out of the system (exothermi proess). w - work done by the system on its surroundings. ositive (+) when work is done by the system, and negative if work done on the system. If body does work, it expends energy and the internal energy of the body must derease. Note, that in some textbooks you will find a plus sign in front of w (work done on the body) or minus sign in front of q (heat flow out of the body). We use notation adapted in Gaskell. Example: pressure: w gas expands, mehanial work is done against an external ext d 0 - ooling by adiabati expansion MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

8 ypes of paths A simple one-omponent system an be desribed by,, and. hey are onneted by equation of state, e.g. =(,). herefore, two independent variables desribe the system and define the state funtions, e.g. = (,). Let s onsider proesses when one of the two independent variables is fixed. = onst isohori proess No work is done (w = d = 0) and the st law takes form: d = q or = q (internal energy an be hanged only by heat exhange) = onst isobari proess w d d and the st law takes form: = q p ( ) or ( + ) ( + ) = q p q p is heat added at onstant pressure. H = + enthalpy - state funtion (sine,, are state funtions) H H = H = q p hange in enthalpy equals to heat added to the system at onstant pressure MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

9 = onst isothermal proess Example: ideal gas ypes of paths (ontinued) d = 0, therefore, d = q - w = 0 (internal energy of an ideal gas is a funtion only of ). Work done depends on the path, i.e. how the external pressure is hanging during the transformation. For example: Free expansion (no external pressure): w = 0 Reversible isothermal expansion ( ext = gas at all times) (reversible proess system is always at equilibrium) q = w = d = Rd/ per mole of gas Integration between states and gives q = w =R ln( / ) = R ln( / ) Work done by the system = heat absorbed by the system Q = 0 - adiabati proess = -w - no heat exhange, the internal energy an be hanged only by work. Real proesses are often omplex,, and all are hanging. In this ase state funtions an be alulated by breaking proess into a series of reversible isothermal, isobari, or isohori proesses that bring system to orret final state. MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

10 Surfae of a ure Substane MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

11 ypes of thermodynami systems Isolated system No energy and no matter an pass through the boundaries of the system. Closed system Energy an pass through the boundaries (as heat and/or work), but matter annot. Adiabati system No heat an pass through the boundary (neither an matter that an arry heat) ideal thermos. Work an be performed on or by the system. surroundings work heat surroundings work surroundings Open system Both energy and matter may pass through the boundaries. work heat matter surroundings An alternative formulation of the st law of thermodynamis: he work done on a system during an adiabati proess is a state funtion and numerially equal to the hange in internal energy of the system. MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

12 Heat Capaity he heat apaity, C, of a system is the ratio of the heat added to the system, or withdrawn from the system, to the resultant hange in the temperature: C = q/ = q/d [J/deg] his definition is only valid in the absene of phase transitions sually C is given as speifi heat apaity,, per gram or per mol New state of the system is not defined by only, need to speify or onstrain seond variable: C C q d q d - heat apaity at onstant volume - heat apaity at onstant pressure he fat that q is not a state funtion and depends on the path is refleted in the dependene of the heat apaity on the path, p v (note that small is used for the derived intensive quantity, per mass, per volume, or per mole, versus apital C for the extensive quantity. For a system ontaining n moles C p = n p and C v = n v where p and v are molar values). and an be measured experimentally isobari proess: isohori proess: dh = q = d d = q = d H and an be alulated from and MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

13 MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei v vs. p If material is allowed to expand during heating, how this affets its heat apaity? v d δq p H d δq Differentiation with respet to at onstant gives v d d d,, sine therefore v work of expansion at onstant due to the temperature inrease by d work of expansion against internal ohesive fores due to the temperature inrease by d

14 MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

15 Calulation of enthalpy from heat apaity For = onst, dh = d and integration gives: H H dh H H d H H d Example: Let us find enthalpy for opper at 500 K. 4.4 Jmol - K - for opper at atm. From the st law an only alulate the differene H - need a referene enthalpy. Enthalpy at atm and K is alled enthalpy of formation, H. For pure elements in their equilibrium states H = H500 H d 0 4.4d 4.9kJ/mol Enthalpy of substanes other than pure elements an also be alulated. he enthalpy of a ompound at K = standard heat of formation of the substane from the elements. Example: For oxidation of opper at 5 C: CuO CuO Cu O H H H H Cu solid + ½ O gas = CuO solid H CuO -56. kj/mol he reation is exothermi heat and/or work are produed MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

16 Calulation of enthalpy from heat apaity (ontinued) In general, heat apaity is a funtion of temperature. For example, for alumina, Al O 3, the temperature dependene an be desribed by p = Jmol - K - in the range -35 K H AlO AlO3 H d kj/mol d kj/mol he standard heat of formation, Al O H 3, and heat apaity, p (), are measured experimentally and an be found in themohemial tables, e.g. at or at the end of Gaskell s textbook In most ases, thermal treatment of materials is arried out under atmospheri pressure and no work other than work of expansion against the atmosphere is produed. Enthalpy hange is used to desribe suh proesses. MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

17 Enthalpy and phase transformations If the system undergoes a phase transformation (or a hemial reation) then the enthalpy hange due to the phase hange, H trans, has to be inluded into total enthalpy hange. Also, different phases an have different heat apaities, p (). For example, let s find enthalpy for opper at 000 K. solid = Jmol - K - in the solid state for = K (this formula for p () is given at Sine this time we are onsidering a wide range of temperatures, we should aount for the temperature dependene of p ( p 4 Jmol - K - at K, 6 Jmol - K - at 500K, 33 Jmol - K - at 358K) liquid = 3.8 Jmol - K - in the liquid state (nearly independent on ) H m = kj mol - latent heat of melting always positive solid liquid H 000 H p d H m p d kJ - mol MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

18 Heat of formation and phase transformations If the temperature of interest is higher than the melting temperatures for both the metal and its oxide, the enthalpy hange for M liquid + ½ O gas = MO liquid is then H H M m MO,solid p M,solid p O p,gas d H M m MO m M m MO,solid p M,liquid p O p,gas d H MO m MO m MO,liquid p M,liquid p O p,gas d MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei Gaskell, Chapter 6.4

19 Heats of Reations Hess s Law Heat absorbed or released in a given hemial reation ourring under onstant pressure onditions is the same weather the proess ours in one or several steps (Hess, 840). Example: C (graphite) + O (gas) = CO (gas) Q = kj mol - C (graphite) + ½ O (gas) = CO (gas) Q = kj mol - CO (gas) + ½ O (gas) = CO (gas) Q = -83. kj mol - otal: kj mol - Hess s Law allows one to alulate Q for reations that is hard to measure resene of atalysts hange the ativation energy of reation but not the net heat of reation. he Hess s law is just a onsequene of the st law of thermodynamis: for = onst, H = Q. Sine H is a state funtion, total heat is independent of path. MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

20 Calulation of heat of transition from heats of reations Let s find if an allotropi transition from diamond to graphite under ambient onditions results in the release or absorption of heat. C (graphite) + O (gas) = CO (gas) H = kj mol - C (diamond) + O (gas) = CO (gas) H = kj mol - hen for reation C (diamond) C (graphite) H = = -.9 kj mol - ransition of diamond to graphite is an exothermi reation Graphitization of a surfae region of diamond at elevated temperature Figure from a omputer simulation MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

21 Summary Make sure you understand language and onepts: hermodynami funtions of state (no dependene on path/history): volume temperature pressure omposition internal energy enthalpy Heat and work are not state funtions ypes of paths isobari isohori isothermal adiabati ypes of systems open losed isolated adiabati Calulation of enthalpy as a funtion of temperature Enthalpy and phase transformations Heat of formation Standard heat of formation Heats of reations and the Hess s law MSE 3050, hermodynamis and Kinetis of Materials, Leonid Zhigilei

Chapter 8 Thermodynamic Relations

Chapter 8 Thermodynamic Relations Chapter 8 Thermodynami Relations 8.1 Types of Thermodynami roperties The thermodynami state of a system an be haraterized by its properties that an be lassified as measured, fundamental, or deried properties.

More information

Physical Laws, Absolutes, Relative Absolutes and Relativistic Time Phenomena

Physical Laws, Absolutes, Relative Absolutes and Relativistic Time Phenomena Page 1 of 10 Physial Laws, Absolutes, Relative Absolutes and Relativisti Time Phenomena Antonio Ruggeri modexp@iafria.om Sine in the field of knowledge we deal with absolutes, there are absolute laws that

More information

University of Washington Department of Chemistry Chemistry 452/456 Summer Quarter 2011

University of Washington Department of Chemistry Chemistry 452/456 Summer Quarter 2011 Homework Assignment #4: Due at 500 pm Monday 8 July,. University of Washington Department of Chemistry Chemistry 45/456 Summer Quarter 0 ) o a very good approximation, ammonia obeys the Bertholet equation

More information

Relativity in Classical Physics

Relativity in Classical Physics Relativity in Classial Physis Main Points Introdution Galilean (Newtonian) Relativity Relativity & Eletromagnetism Mihelson-Morley Experiment Introdution The theory of relativity deals with the study of

More information

General Equilibrium. What happens to cause a reaction to come to equilibrium?

General Equilibrium. What happens to cause a reaction to come to equilibrium? General Equilibrium Chemial Equilibrium Most hemial reations that are enountered are reversible. In other words, they go fairly easily in either the forward or reverse diretions. The thing to remember

More information

Journal of Theoretics Vol.5-2 Guest Commentary Relativistic Thermodynamics for the Introductory Physics Course

Journal of Theoretics Vol.5-2 Guest Commentary Relativistic Thermodynamics for the Introductory Physics Course Journal of heoretis Vol.5- Guest Commentary Relatiisti hermodynamis for the Introdutory Physis Course B.Rothenstein bernhard_rothenstein@yahoo.om I.Zaharie Physis Department, "Politehnia" Uniersity imisoara,

More information

THEORETICAL PROBLEM No. 3 WHY ARE STARS SO LARGE?

THEORETICAL PROBLEM No. 3 WHY ARE STARS SO LARGE? THEORETICAL PROBLEM No. 3 WHY ARE STARS SO LARGE? The stars are spheres of hot gas. Most of them shine beause they are fusing hydrogen into helium in their entral parts. In this problem we use onepts of

More information

Research Article Substance Independence of Efficiency of a Class of Heat Engines Undergoing Two Isothermal Processes

Research Article Substance Independence of Efficiency of a Class of Heat Engines Undergoing Two Isothermal Processes hermodynamis olume 0, Artile ID 6797, 5 pages doi:0.55/0/6797 Researh Artile Substane Independene of Effiieny of a Class of Heat Engines Undergoing wo Isothermal roesses Y. Haseli Department of Mehanial

More information

Chapter 14. The Concept of Equilibrium and the Equilibrium Constant. We have for the most part depicted reactions as going one way.

Chapter 14. The Concept of Equilibrium and the Equilibrium Constant. We have for the most part depicted reactions as going one way. Chapter 14 The Conept of Equilibrium and the Equilibrium Constant In hapter 1 we dealt with Physial Equilibrium Physial Changes HO 2 (l) HO 2 (g) In hapter 14 we will learn about Chemial Equilibrium. We

More information

Four-dimensional equation of motion for viscous compressible substance with regard to the acceleration field, pressure field and dissipation field

Four-dimensional equation of motion for viscous compressible substance with regard to the acceleration field, pressure field and dissipation field Four-dimensional equation of motion for visous ompressible substane with regard to the aeleration field, pressure field and dissipation field Sergey G. Fedosin PO box 6488, Sviazeva str. -79, Perm, Russia

More information

JF Physical Chemistry JF CH 1101: Introduction to Physical Chemistry.

JF Physical Chemistry JF CH 1101: Introduction to Physical Chemistry. JF Physial Chemistry 010-011. JF CH 1101: Introdution to Physial Chemistry. Dr Mike Lyons. Shool of Chemistry Trinity College Dublin. melyons@td.ie A ompendium of past examination questions set on Physial

More information

KINETICS OF IRON OXIDE DIRECT REDUCTION BY COAL E.R. ABRIL 1

KINETICS OF IRON OXIDE DIRECT REDUCTION BY COAL E.R. ABRIL 1 KINETICS OF IRON OXIDE DIRECT REDUCTION BY COAL E.R. ABRIL 1 CIMM- Av.Velez Sarsfield 1561 C.P.5000 Córdoba, Argentina. aabril@intiemor.gov.ar Abstrat - A new interpretation to the kinetis of iron oxide

More information

2 How far? Equilibrium Answers

2 How far? Equilibrium Answers How far? Equilibrium Answers ratie: pages 37 39 1 Answer is D. Only a hange in temperature harges the value of the equilibrium onstant. Answer is D. [B] /[A] so [B] [A] or [B] [A] 1/ 3 Answer is B. Amounts

More information

CHAPTER 26 The Special Theory of Relativity

CHAPTER 26 The Special Theory of Relativity CHAPTER 6 The Speial Theory of Relativity Units Galilean-Newtonian Relativity Postulates of the Speial Theory of Relativity Simultaneity Time Dilation and the Twin Paradox Length Contration Four-Dimensional

More information

Determination of the reaction order

Determination of the reaction order 5/7/07 A quote of the wee (or amel of the wee): Apply yourself. Get all the eduation you an, but then... do something. Don't just stand there, mae it happen. Lee Iaoa Physial Chemistry GTM/5 reation order

More information

Chapter 3. Volumetric Properties of Pure Fluids

Chapter 3. Volumetric Properties of Pure Fluids Chapter 3. olumetri roperties of ure Fluids Introdution hermodynami properties (U, H and thus Q, W) are alulated from data data are important for sizing vessels and pipelines Subjets behavior of pure fluids

More information

STATISTICAL MECHANICS & THERMODYNAMICS

STATISTICAL MECHANICS & THERMODYNAMICS UVA PHYSICS DEPARTMENT PHD QUALIFYING EXAM PROBLEM FILE STATISTICAL MECHANICS & THERMODYNAMICS UPDATED: NOVEMBER 14, 212 1. a. Explain what is meant by the density of states, and give an expression for

More information

Where as discussed previously we interpret solutions to this partial differential equation in the weak sense: b

Where as discussed previously we interpret solutions to this partial differential equation in the weak sense: b Consider the pure initial value problem for a homogeneous system of onservation laws with no soure terms in one spae dimension: Where as disussed previously we interpret solutions to this partial differential

More information

The Thomas Precession Factor in Spin-Orbit Interaction

The Thomas Precession Factor in Spin-Orbit Interaction p. The Thomas Preession Fator in Spin-Orbit Interation Herbert Kroemer * Department of Eletrial and Computer Engineering, Uniersity of California, Santa Barbara, CA 9306 The origin of the Thomas fator

More information

Introduction to Quantum Chemistry

Introduction to Quantum Chemistry Chem. 140B Dr. J.A. Mak Introdution to Quantum Chemistry Without Quantum Mehanis, how would you explain: Periodi trends in properties of the elements Struture of ompounds e.g. Tetrahedral arbon in ethane,

More information

Particle-wave symmetry in Quantum Mechanics And Special Relativity Theory

Particle-wave symmetry in Quantum Mechanics And Special Relativity Theory Partile-wave symmetry in Quantum Mehanis And Speial Relativity Theory Author one: XiaoLin Li,Chongqing,China,hidebrain@hotmail.om Corresponding author: XiaoLin Li, Chongqing,China,hidebrain@hotmail.om

More information

On the Quantum Theory of Radiation.

On the Quantum Theory of Radiation. Physikalishe Zeitshrift, Band 18, Seite 121-128 1917) On the Quantum Theory of Radiation. Albert Einstein The formal similarity between the hromati distribution urve for thermal radiation and the Maxwell

More information

ELECTROMAGNETIC WAVES WITH NONLINEAR DISPERSION LAW. P. М. Меdnis

ELECTROMAGNETIC WAVES WITH NONLINEAR DISPERSION LAW. P. М. Меdnis ELECTROMAGNETIC WAVES WITH NONLINEAR DISPERSION LAW P. М. Меdnis Novosibirs State Pedagogial University, Chair of the General and Theoretial Physis, Russia, 636, Novosibirs,Viljujsy, 8 e-mail: pmednis@inbox.ru

More information

Classical Diamagnetism and the Satellite Paradox

Classical Diamagnetism and the Satellite Paradox Classial Diamagnetism and the Satellite Paradox 1 Problem Kirk T. MDonald Joseph Henry Laboratories, Prineton University, Prineton, NJ 08544 (November 1, 008) In typial models of lassial diamagnetism (see,

More information

Performance of an irreversible Diesel cycle under variable stroke length and compression ratio

Performance of an irreversible Diesel cycle under variable stroke length and compression ratio Marsland Press Journal of Amerian Siene 00;6():58-6 Performane of an irreversible iesel yle under variable stroke length and ompression ratio epartment of Agriulture Mahine Mehanis, Shahrekord University,

More information

KINETIC THEORY OF GASES

KINETIC THEORY OF GASES Kineti Theory of Gases 10 KINETIC THEORY OF GASES As you have studied in the previous lessons, at standard temperature and pressure, matter exists in three states solid, liquid and gas. These are omposed

More information

Chapter 15: Chemical Equilibrium

Chapter 15: Chemical Equilibrium Chapter 5: Chemial Equilibrium ahoot!. At eq, the rate of the forward reation is the rate of the reverse reation. equal to, slower than, faster than, the reverse of. Selet the statement that BEST desribes

More information

Line Radiative Transfer

Line Radiative Transfer http://www.v.nrao.edu/ourse/astr534/ineradxfer.html ine Radiative Transfer Einstein Coeffiients We used armor's equation to estimate the spontaneous emission oeffiients A U for À reombination lines. A

More information

Heat exchangers: Heat exchanger types:

Heat exchangers: Heat exchanger types: Heat exhangers: he proess of heat exhange between two fluids that are at different temperatures and separated by a solid wall ours in many engineering appliations. he devie used to implement this exhange

More information

Maximum Entropy and Exponential Families

Maximum Entropy and Exponential Families Maximum Entropy and Exponential Families April 9, 209 Abstrat The goal of this note is to derive the exponential form of probability distribution from more basi onsiderations, in partiular Entropy. It

More information

The gravitational phenomena without the curved spacetime

The gravitational phenomena without the curved spacetime The gravitational phenomena without the urved spaetime Mirosław J. Kubiak Abstrat: In this paper was presented a desription of the gravitational phenomena in the new medium, different than the urved spaetime,

More information

Relativistic Dynamics

Relativistic Dynamics Chapter 7 Relativisti Dynamis 7.1 General Priniples of Dynamis 7.2 Relativisti Ation As stated in Setion A.2, all of dynamis is derived from the priniple of least ation. Thus it is our hore to find a suitable

More information

8.333: Statistical Mechanics I Problem Set # 4 Due: 11/13/13 Non-interacting particles

8.333: Statistical Mechanics I Problem Set # 4 Due: 11/13/13 Non-interacting particles 8.333: Statistial Mehanis I Problem Set # 4 Due: 11/13/13 Non-interating partiles 1. Rotating gas: Consider a gas of N idential atoms onfined to a spherial harmoni trap in three dimensions, i.e. the partiles

More information

III. SURFACE PROPERTIES III.A. SURFACE TENSION SURFACE PROPERTIES

III. SURFACE PROPERTIES III.A. SURFACE TENSION SURFACE PROPERTIES III. SURFACE PROPERTIES III.A. SURFACE TENSION GOAL: To investigate the influene of the solution onentration and/or the kind of the solute on the surfae tension INTRODUCTION Liquids tend to adopt shapes

More information

The Concept of Mass as Interfering Photons, and the Originating Mechanism of Gravitation D.T. Froedge

The Concept of Mass as Interfering Photons, and the Originating Mechanism of Gravitation D.T. Froedge The Conept of Mass as Interfering Photons, and the Originating Mehanism of Gravitation D.T. Froedge V04 Formerly Auburn University Phys-dtfroedge@glasgow-ky.om Abstrat For most purposes in physis the onept

More information

Thermal Mechanisms of Stable Macroscopic Penetration of Applied Currents in High Temperature Superconductors and their Instability Conditions

Thermal Mechanisms of Stable Macroscopic Penetration of Applied Currents in High Temperature Superconductors and their Instability Conditions 1 The Open Applied Physis Journal, 212, 5, 1-33 Open Aess Thermal Mehanisms of Stable Marosopi Penetration of Applied Currents in High Temperature Superondutors and their Instability Conditions V R Romanovskii

More information

The First Principle of Thermodynamics under Relativistic Conditions and Temperature

The First Principle of Thermodynamics under Relativistic Conditions and Temperature New Horizons in Mathematial Physis, Vol., No., September 7 https://dx.doi.org/.66/nhmp.7. 37 he First Priniple of hermodynamis under Relativisti Conditions and emperature Emil Veitsman Independent Researher

More information

A No-Shape-Substance is the foundation. all Physics laws depend on

A No-Shape-Substance is the foundation. all Physics laws depend on A No-Shape-Substane is the foundation all Physis laws depend on The Seond Part of New Physis Ji Qi,Yinling Jiang Department of physis, Shool of Eletroni Engineering, Northeast Petroleum University, No.

More information

Part G-4: Sample Exams

Part G-4: Sample Exams Part G-4: Sample Exams 1 Cairo University M.S.: Eletronis Cooling Faulty of Engineering Final Exam (Sample 1) Mehanial Power Engineering Dept. Time allowed 2 Hours Solve as muh as you an. 1. A heat sink

More information

ELECTROMAGNETIC NORMAL MODES AND DISPERSION FORCES.

ELECTROMAGNETIC NORMAL MODES AND DISPERSION FORCES. ELECTROMAGNETIC NORMAL MODES AND DISPERSION FORCES. All systems with interation of some type have normal modes. One may desribe them as solutions in absene of soures; they are exitations of the system

More information

Test bank chapter (14)

Test bank chapter (14) Test bank hater (14) Choose the most orret answer 1. Whih is the orret equilibrium onstant exression for the following reation? Fe 2 O 3 (s) + 3H 2 (g) 2Fe(s) + 3H 2 O(g) a) K = [Fe 2 O 3 ] [H 2 ] 3 /[Fe]

More information

Millennium Relativity Acceleration Composition. The Relativistic Relationship between Acceleration and Uniform Motion

Millennium Relativity Acceleration Composition. The Relativistic Relationship between Acceleration and Uniform Motion Millennium Relativity Aeleration Composition he Relativisti Relationship between Aeleration and niform Motion Copyright 003 Joseph A. Rybzyk Abstrat he relativisti priniples developed throughout the six

More information

Aharonov-Bohm effect. Dan Solomon.

Aharonov-Bohm effect. Dan Solomon. Aharonov-Bohm effet. Dan Solomon. In the figure the magneti field is onfined to a solenoid of radius r 0 and is direted in the z- diretion, out of the paper. The solenoid is surrounded by a barrier that

More information

A simple expression for radial distribution functions of pure fluids and mixtures

A simple expression for radial distribution functions of pure fluids and mixtures A simple expression for radial distribution funtions of pure fluids and mixtures Enrio Matteoli a) Istituto di Chimia Quantistia ed Energetia Moleolare, CNR, Via Risorgimento, 35, 56126 Pisa, Italy G.

More information

Improvements in the Modeling of the Self-ignition of Tetrafluoroethylene

Improvements in the Modeling of the Self-ignition of Tetrafluoroethylene Exerpt from the Proeedings of the OMSOL onferene 010 Paris Improvements in the Modeling of the Self-ignition of Tetrafluoroethylene M. Bekmann-Kluge 1 *,. errero 1, V. Shröder 1, A. Aikalin and J. Steinbah

More information

Chemistry (Physical chemistry) Lecture 10.

Chemistry (Physical chemistry) Lecture 10. Chemistry (Physial hemistry) Leture 0. EPM, semester II by Wojieh Chrzanowsi, PhD, DS Wyłady współfinansowane ze środów Unii Europejsiej w ramah EFS, UDA-POKL 04.0.02.-00-37/-00 Absolwent Wydziału Chemiznego

More information

23.1 Tuning controllers, in the large view Quoting from Section 16.7:

23.1 Tuning controllers, in the large view Quoting from Section 16.7: Lesson 23. Tuning a real ontroller - modeling, proess identifiation, fine tuning 23.0 Context We have learned to view proesses as dynami systems, taking are to identify their input, intermediate, and output

More information

PHYSICS 212 FINAL EXAM 21 March 2003

PHYSICS 212 FINAL EXAM 21 March 2003 PHYSIS INAL EXAM Marh 00 Eam is losed book, losed notes. Use only the provided formula sheet. Write all work and answers in eam booklets. The baks of pages will not be graded unless you so ruest on the

More information

Sample Teaching Sequence (Hong Kong Secondary 4 6 Chemistry)

Sample Teaching Sequence (Hong Kong Secondary 4 6 Chemistry) Revised (1 Sept 009 Sample Teahing Suene (Hong Kong Seondary 4 6 Chemistry Topi: Chemial Equilibrium Teahing Suene Content 1.1 Reversible reations Examples of reversible reation; forward reation; reverse

More information

BINARY RANKINE CYCLE OPTIMIZATION Golub, M., Koscak-Kolin, S., Kurevija, T.

BINARY RANKINE CYCLE OPTIMIZATION Golub, M., Koscak-Kolin, S., Kurevija, T. BINARY RANKINE CYCLE OPTIMIZATION Golub, M., Kosak-Kolin, S., Kurevija, T. Faulty of Mining, Geology and Petroleum Engineering Department of Petroleum Engineering Pierottijeva 6, Zagreb 0 000, Croatia

More information

The Electromagnetic Radiation and Gravity

The Electromagnetic Radiation and Gravity International Journal of Theoretial and Mathematial Physis 016, 6(3): 93-98 DOI: 10.593/j.ijtmp.0160603.01 The Eletromagneti Radiation and Gravity Bratianu Daniel Str. Teiului Nr. 16, Ploiesti, Romania

More information

Effect of magnetization process on levitation force between a superconducting. disk and a permanent magnet

Effect of magnetization process on levitation force between a superconducting. disk and a permanent magnet Effet of magnetization proess on levitation fore between a superonduting disk and a permanent magnet L. Liu, Y. Hou, C.Y. He, Z.X. Gao Department of Physis, State Key Laboratory for Artifiial Mirostruture

More information

The Hanging Chain. John McCuan. January 19, 2006

The Hanging Chain. John McCuan. January 19, 2006 The Hanging Chain John MCuan January 19, 2006 1 Introdution We onsider a hain of length L attahed to two points (a, u a and (b, u b in the plane. It is assumed that the hain hangs in the plane under a

More information

Green s function for the wave equation

Green s function for the wave equation Green s funtion for the wave equation Non-relativisti ase January 2019 1 The wave equations In the Lorentz Gauge, the wave equations for the potentials are (Notes 1 eqns 43 and 44): 1 2 A 2 2 2 A = µ 0

More information

New Potential of the. Positron-Emission Tomography

New Potential of the. Positron-Emission Tomography International Journal of Modern Physis and Appliation 6; 3(: 39- http://www.aasit.org/journal/ijmpa ISSN: 375-387 New Potential of the Positron-Emission Tomography Andrey N. olobuev, Eugene S. Petrov,

More information

Chapter 13, Chemical Equilibrium

Chapter 13, Chemical Equilibrium Chapter 13, Chemial Equilibrium You may have gotten the impression that when 2 reatants mix, the ensuing rxn goes to ompletion. In other words, reatants are onverted ompletely to produts. We will now learn

More information

3 Tidal systems modelling: ASMITA model

3 Tidal systems modelling: ASMITA model 3 Tidal systems modelling: ASMITA model 3.1 Introdution For many pratial appliations, simulation and predition of oastal behaviour (morphologial development of shorefae, beahes and dunes) at a ertain level

More information

The homopolar generator: an analytical example

The homopolar generator: an analytical example The homopolar generator: an analytial example Hendrik van Hees August 7, 214 1 Introdution It is surprising that the homopolar generator, invented in one of Faraday s ingenious experiments in 1831, still

More information

POROUS CARBON PARTICLE COMBUSTION IN AIR

POROUS CARBON PARTICLE COMBUSTION IN AIR MCS 7 Chia Laguna, Cagliari, Sardinia, taly, 11-15, 11 POOUS CABON PATCLE COMBUSTON N A V. M. Gremyahkin grema@ipmnet.ru nstitute for Problems in Mehanis, AS, Mosow, ussia Abstrat Theoretial investigation

More information

Critical Reflections on the Hafele and Keating Experiment

Critical Reflections on the Hafele and Keating Experiment Critial Refletions on the Hafele and Keating Experiment W.Nawrot In 1971 Hafele and Keating performed their famous experiment whih onfirmed the time dilation predited by SRT by use of marosopi loks. As

More information

22.54 Neutron Interactions and Applications (Spring 2004) Chapter 6 (2/24/04) Energy Transfer Kernel F(E E')

22.54 Neutron Interactions and Applications (Spring 2004) Chapter 6 (2/24/04) Energy Transfer Kernel F(E E') 22.54 Neutron Interations and Appliations (Spring 2004) Chapter 6 (2/24/04) Energy Transfer Kernel F(E E') Referenes -- J. R. Lamarsh, Introdution to Nulear Reator Theory (Addison-Wesley, Reading, 1966),

More information

The Laws of Acceleration

The Laws of Acceleration The Laws of Aeleration The Relationships between Time, Veloity, and Rate of Aeleration Copyright 2001 Joseph A. Rybzyk Abstrat Presented is a theory in fundamental theoretial physis that establishes the

More information

Modeling of Threading Dislocation Density Reduction in Heteroepitaxial Layers

Modeling of Threading Dislocation Density Reduction in Heteroepitaxial Layers A. E. Romanov et al.: Threading Disloation Density Redution in Layers (II) 33 phys. stat. sol. (b) 99, 33 (997) Subjet lassifiation: 6.72.C; 68.55.Ln; S5.; S5.2; S7.; S7.2 Modeling of Threading Disloation

More information

Subject: Modeling of Thermal Rocket Engines; Nozzle flow; Control of mass flow. p c. Thrust Chamber mixing and combustion

Subject: Modeling of Thermal Rocket Engines; Nozzle flow; Control of mass flow. p c. Thrust Chamber mixing and combustion 16.50 Leture 6 Subjet: Modeling of Thermal Roket Engines; Nozzle flow; Control of mass flow Though onetually simle, a roket engine is in fat hysially a very omlex devie and diffiult to reresent quantitatively

More information

Physics 2D Lecture Slides Lecture 7: Jan 14th 2004

Physics 2D Lecture Slides Lecture 7: Jan 14th 2004 Quiz is This Friday Quiz will over Setions.-.6 (inlusive) Remaining material will be arried over to Quiz Bring Blue Book, hek alulator battery Write all answers in indelible ink else no grade! Write answers

More information

arxiv:gr-qc/ v7 14 Dec 2003

arxiv:gr-qc/ v7 14 Dec 2003 Propagation of light in non-inertial referene frames Vesselin Petkov Siene College, Conordia University 1455 De Maisonneuve Boulevard West Montreal, Quebe, Canada H3G 1M8 vpetkov@alor.onordia.a arxiv:gr-q/9909081v7

More information

Surface tension in a reactive binary mixture of incompressible fluids

Surface tension in a reactive binary mixture of incompressible fluids Surfae tension in a reative binary mixture of inompressible fluids Henning Struhtrup Institute for Mathematis and its Appliations, 400 Lind Hall, 07 Churh Street S.E, Minneapolis MN55455 John Dold Mathematis

More information

ES 247 Fracture Mechanics Zhigang Suo

ES 247 Fracture Mechanics Zhigang Suo ES 47 Frature Mehanis Zhigang Suo The Griffith Paper Readings. A.A. Griffith, The phenomena of rupture and flow in solids. Philosophial Transations of the Royal Soiety of London, Series A, Volume 1 (191)

More information

Classical Field Theory

Classical Field Theory Preprint typeset in JHEP style - HYPER VERSION Classial Field Theory Gleb Arutyunov a a Institute for Theoretial Physis and Spinoza Institute, Utreht University, 3508 TD Utreht, The Netherlands Abstrat:

More information

Analysis of discretization in the direct simulation Monte Carlo

Analysis of discretization in the direct simulation Monte Carlo PHYSICS OF FLUIDS VOLUME 1, UMBER 1 OCTOBER Analysis of disretization in the diret simulation Monte Carlo iolas G. Hadjionstantinou a) Department of Mehanial Engineering, Massahusetts Institute of Tehnology,

More information

In this case it might be instructive to present all three components of the current density:

In this case it might be instructive to present all three components of the current density: Momentum, on the other hand, presents us with a me ompliated ase sine we have to deal with a vetial quantity. The problem is simplified if we treat eah of the omponents of the vet independently. s you

More information

Bäcklund Transformations: Some Old and New Perspectives

Bäcklund Transformations: Some Old and New Perspectives Bäklund Transformations: Some Old and New Perspetives C. J. Papahristou *, A. N. Magoulas ** * Department of Physial Sienes, Helleni Naval Aademy, Piraeus 18539, Greee E-mail: papahristou@snd.edu.gr **

More information

+Ze. n = N/V = 6.02 x x (Z Z c ) m /A, (1.1) Avogadro s number

+Ze. n = N/V = 6.02 x x (Z Z c ) m /A, (1.1) Avogadro s number In 1897, J. J. Thomson disovered eletrons. In 1905, Einstein interpreted the photoeletri effet In 1911 - Rutherford proved that atoms are omposed of a point-like positively harged, massive nuleus surrounded

More information

CRITICAL EXPONENTS TAKING INTO ACCOUNT DYNAMIC SCALING FOR ADSORPTION ON SMALL-SIZE ONE-DIMENSIONAL CLUSTERS

CRITICAL EXPONENTS TAKING INTO ACCOUNT DYNAMIC SCALING FOR ADSORPTION ON SMALL-SIZE ONE-DIMENSIONAL CLUSTERS Russian Physis Journal, Vol. 48, No. 8, 5 CRITICAL EXPONENTS TAKING INTO ACCOUNT DYNAMIC SCALING FOR ADSORPTION ON SMALL-SIZE ONE-DIMENSIONAL CLUSTERS A. N. Taskin, V. N. Udodov, and A. I. Potekaev UDC

More information

Equilibrium 07 M07_CHSL_SB_IBD_9069_U07.indd /07/ :21

Equilibrium 07 M07_CHSL_SB_IBD_9069_U07.indd /07/ :21 07 Equilibrium Essential ideas 7.1 Many reations are reversible. These reations will reah a state of equilibrium when the rates of the forward reation and reverse reation are equal. The position of equilibrium

More information

The concept of the general force vector field

The concept of the general force vector field The onept of the general fore vetor field Sergey G. Fedosin PO box 61488, Sviazeva str. 22-79, Perm, Russia E-mail: intelli@list.ru A hypothesis is suggested that the lassial eletromagneti and gravitational

More information

Dynamics of the Electromagnetic Fields

Dynamics of the Electromagnetic Fields Chapter 3 Dynamis of the Eletromagneti Fields 3.1 Maxwell Displaement Current In the early 1860s (during the Amerian ivil war!) eletriity inluding indution was well established experimentally. A big row

More information

arxiv: v1 [physics.class-ph] 14 Dec 2010

arxiv: v1 [physics.class-ph] 14 Dec 2010 Classial relativisti ideal gas in thermodynami equilibrium in a uniformly aelerated referene frame arxiv:11.363v1 [physis.lass-ph] 14 De 1 Domingo J. Louis-Martinez Department of Physis and Astronomy,

More information

2. Mass transfer takes place in the two contacting phases as in extraction and absorption.

2. Mass transfer takes place in the two contacting phases as in extraction and absorption. PRT 11- CONVECTIVE MSS TRNSFER 2.1 Introdution 2.2 Convetive Mass Transfer oeffiient 2.3 Signifiant parameters in onvetive mass transfer 2.4 The appliation of dimensional analysis to Mass Transfer 2.4.1

More information

arxiv: v1 [physics.plasm-ph] 5 Aug 2012

arxiv: v1 [physics.plasm-ph] 5 Aug 2012 Classial mirosopi derivation of the relativisti hydrodynamis equations arxiv:1208.0998v1 [physis.plasm-ph] 5 Aug 2012 P. A. Andreev Department of General Physis, Physis Faulty, Mosow State University,

More information

Gravitation is a Gradient in the Velocity of Light ABSTRACT

Gravitation is a Gradient in the Velocity of Light ABSTRACT 1 Gravitation is a Gradient in the Veloity of Light D.T. Froedge V5115 @ http://www.arxdtf.org Formerly Auburn University Phys-dtfroedge@glasgow-ky.om ABSTRACT It has long been known that a photon entering

More information

Class Test 1 ( ) Subject Code :Applied Physics (17202/17207/17210) Total Marks :25. Model Answer. 3. Photon travels with the speed of light

Class Test 1 ( ) Subject Code :Applied Physics (17202/17207/17210) Total Marks :25. Model Answer. 3. Photon travels with the speed of light Class Test (0-) Sujet Code :Applied Physis (70/707/70) Total Marks :5 Sem. :Seond Model Answer Q Attempt any FOUR of the following 8 a State the properties of photon Ans:.Photon is eletrially neutral.

More information

arxiv:physics/ v1 14 May 2002

arxiv:physics/ v1 14 May 2002 arxiv:physis/0205041 v1 14 May 2002 REPLY TO CRITICISM OF NECESSITY OF SIMULTANEOUS CO-EXISTENCE OF INSTANTANEOUS AND RETARDED INTERACTIONS IN CLASSICAL ELECTRODYNAMICS by J.D.Jakson ANDREW E. CHUBYKALO

More information

Towards an Absolute Cosmic Distance Gauge by using Redshift Spectra from Light Fatigue.

Towards an Absolute Cosmic Distance Gauge by using Redshift Spectra from Light Fatigue. Towards an Absolute Cosmi Distane Gauge by using Redshift Spetra from Light Fatigue. Desribed by using the Maxwell Analogy for Gravitation. T. De Mees - thierrydemees @ pandora.be Abstrat Light is an eletromagneti

More information

SOLVED QUESTIONS 1 / 2. in a closed container at equilibrium. What would be the effect of addition of CaCO 3 on the equilibrium concentration of CO 2?

SOLVED QUESTIONS 1 / 2. in a closed container at equilibrium. What would be the effect of addition of CaCO 3 on the equilibrium concentration of CO 2? SOLVED QUESTIONS Multile Choie Questions. and are the veloity onstants of forward and bakward reations. The equilibrium onstant k of the reation is (A) (B) (C) (D). Whih of the following reations will

More information

Chapter 15 Equilibrium. Reversible Reactions & Equilibrium. Reversible Reactions & Equilibrium. Reversible Reactions & Equilibrium 2/3/2014

Chapter 15 Equilibrium. Reversible Reactions & Equilibrium. Reversible Reactions & Equilibrium. Reversible Reactions & Equilibrium 2/3/2014 Amount of reatant/produt //01 quilibrium in Chemial Reations Lets look bak at our hypothetial reation from the kinetis hapter. A + B C Chapter 15 quilibrium [A] Why doesn t the onentration of A ever go

More information

A generalized equation of state with an application to the Earth s Mantle

A generalized equation of state with an application to the Earth s Mantle Geofísia Internaional 49 (), 77-8 (010) A generalized equation of state with an appliation to the Earth s Mantle J. A. Robles-Gutiérrez 1, J. M. A. Robles-Domínguez 1 and C. Lomnitz 1 Universidad Autónoma

More information

arxiv:physics/ v1 [physics.class-ph] 8 Aug 2003

arxiv:physics/ v1 [physics.class-ph] 8 Aug 2003 arxiv:physis/0308036v1 [physis.lass-ph] 8 Aug 003 On the meaning of Lorentz ovariane Lszl E. Szab Theoretial Physis Researh Group of the Hungarian Aademy of Sienes Department of History and Philosophy

More information

The concept of the general force vector field

The concept of the general force vector field OALib Journal, Vol. 3, P. 1-15 (16). http://dx.doi.org/1.436/oalib.11459 The onept of the general fore vetor field Sergey G. Fedosin PO box 61488, Sviazeva str. -79, Perm, Russia E-mail: intelli@list.ru

More information

Gluing Potential Energy Surfaces with Rare Event Simulations

Gluing Potential Energy Surfaces with Rare Event Simulations This is an open aess artile published under an ACS AuthorChoie Liense, whih permits opying and redistribution of the artile or any adaptations for non-ommerial purposes. pubs.as.org/jctc Gluing Potential

More information

The Unified Geometrical Theory of Fields and Particles

The Unified Geometrical Theory of Fields and Particles Applied Mathematis, 014, 5, 347-351 Published Online February 014 (http://www.sirp.org/journal/am) http://dx.doi.org/10.436/am.014.53036 The Unified Geometrial Theory of Fields and Partiles Amagh Nduka

More information

Numerical Tests of Nucleation Theories for the Ising Models. Abstract

Numerical Tests of Nucleation Theories for the Ising Models. Abstract to be submitted to Physial Review E Numerial Tests of Nuleation Theories for the Ising Models Seunghwa Ryu 1 and Wei Cai 2 1 Department of Physis, Stanford University, Stanford, California 94305 2 Department

More information

Brazilian Journal of Physics, vol. 29, no. 3, September, Classical and Quantum Mechanics of a Charged Particle

Brazilian Journal of Physics, vol. 29, no. 3, September, Classical and Quantum Mechanics of a Charged Particle Brazilian Journal of Physis, vol. 9, no. 3, September, 1999 51 Classial and Quantum Mehanis of a Charged Partile in Osillating Eletri and Magneti Fields V.L.B. de Jesus, A.P. Guimar~aes, and I.S. Oliveira

More information

Properties of Quarks

Properties of Quarks PHY04 Partile Physis 9 Dr C N Booth Properties of Quarks In the earlier part of this ourse, we have disussed three families of leptons but prinipally onentrated on one doublet of quarks, the u and d. We

More information

Thermochemistry and Calorimetry

Thermochemistry and Calorimetry WHY? ACTIVITY 06-1 Thermohemitry and Calorimetry Chemial reation releae or tore energy, uually in the form of thermal energy. Thermal energy i the kineti energy of motion of the atom and moleule ompriing

More information

Metric of Universe The Causes of Red Shift.

Metric of Universe The Causes of Red Shift. Metri of Universe The Causes of Red Shift. ELKIN IGOR. ielkin@yande.ru Annotation Poinare and Einstein supposed that it is pratially impossible to determine one-way speed of light, that s why speed of

More information

Physics 486. Classical Newton s laws Motion of bodies described in terms of initial conditions by specifying x(t), v(t).

Physics 486. Classical Newton s laws Motion of bodies described in terms of initial conditions by specifying x(t), v(t). Physis 486 Tony M. Liss Leture 1 Why quantum mehanis? Quantum vs. lassial mehanis: Classial Newton s laws Motion of bodies desribed in terms of initial onditions by speifying x(t), v(t). Hugely suessful

More information

The Reason of Photons Angular Distribution at Electron-Positron Annihilation in a Positron-Emission Tomograph

The Reason of Photons Angular Distribution at Electron-Positron Annihilation in a Positron-Emission Tomograph Advanes in Natural Siene ol 7, No,, pp -5 DOI: 3968/66 ISSN 75-786 [PRINT] ISSN 75-787 [ONLINE] wwwsanadanet wwwsanadaorg The Reason of Photons Angular Distribution at Eletron-Positron Annihilation in

More information

REVIEW QUESTIONS Chapter 15

REVIEW QUESTIONS Chapter 15 hemistry 10 ANSWER EY REVIEW QUESTIONS hapter 15 1. A mixture of 0.10 mol of NO, 0.050 mol of H and 0.10 mol of HO is plaed in a 1.0-L flask and allowed to reah equilibrium as shown below: NO (g) + H (g)

More information

Fig 1: Variables in constant (1+1)D acceleration. speed of time. p-velocity & c-time. velocities (e.g. v/c) & times (e.g.

Fig 1: Variables in constant (1+1)D acceleration. speed of time. p-velocity & c-time. velocities (e.g. v/c) & times (e.g. Proper veloity and frame-invariant aeleration in speial relativity P. Fraundorf Department of Physis & Astronomy University of Missouri-StL, St. Louis MO (November, 99) We examine here a possible endpoint

More information