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AMALIA SHOLEHAH JURUSAN TEKNIK METALURGI FT – UNTIRTA THERMODYNAMICS.

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Presentation on theme: "AMALIA SHOLEHAH JURUSAN TEKNIK METALURGI FT – UNTIRTA THERMODYNAMICS."— Presentation transcript:

1 AMALIA SHOLEHAH JURUSAN TEKNIK METALURGI FT – UNTIRTA THERMODYNAMICS

2 Overview General ChemistryPhysical Chemistry First Law: The internal energy of an isolated system is constant Zeroth Law: If two thermodynamics systems are in thermal equilibrium with a third, they are also in thermal equilibrium with each other First Law: The energy of an isolated system is constant. It implies that energy can never be created or destroyed, it can only change its form. For a system U = q + w ; Where (U) represents a change in internal energy, (q) is the change in thermal energy and (w) is the work done Second Law: A spontaneous change is accompanied by an increase in the total entropy of the system and its surroundings Second Law: Whenever a spontaneous event takes place it is accompanied by an increase in the entropy of the universe Third Law: For a pure crystalline substance, S = 0 at 0°K

3 Study of the patterns of energy change " thermo"  energy "dynamics"  the patterns of change Deals mainly with (A) energy conversion (B) the stability of molecules (C) direction of change

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5 Laws of Thermodynamics They control interactions of everything in the universe - regardless of scale Classical physics is, from a certain perspective, entirely based on Newton's Laws of motion  only applicable in certain conditions Development of the Laws of Thermodynamics actually began thousands of years ago The largest advancements in developing the Laws of Thermodynamics occurred in the mid-1800s  Joule’s experiment  First Law of Thermodynamics

6 Not long after  Clausius theory  Second Law of Thermodynamics Around 1906  Nernst theory  Third Law of Thermodynamics

7 State of a System System  physical universe that is under consideration System is separated from rest of universe by Real / Imaginary boundary Surroundings  part of universe outside the boundary

8 Thermodynamics Properties Extensive properties  Depend on the size of the system  Ex : Volume (V), mass Intensive properties  Not depend on the size of the ystem  Ex : Pressure (P), Temperature (T), density

9 Thermodynamics Process P – V conjugate pair  transfer of mechanical or dynamic energy as the result of work  Isobaric process  occurs on constant pressure (dynamically connected)  Isochoric / isometric process  occurs on constant volume (dynamically insulated)

10 T – S conjugate pair  transfer of thermal energy as the result of heating  Isothermal process  occurs on constant temperature (thermally connected)  Isentropic process  occurs on constant entropy  Adiabatic process  no energy added or subtracted from the system by heating or cooling (thermally insulated)

11 State Variables (Thermodynamic Coordinates) When a system is at equilibrium  its state defined entirely by the state variable  not depend on history of system Ex : pressure (P), temperature (T), internal energy (U), enthalpy (H), enthropy (S), and Gibbs energy (G)

12 Zeroth Law “ If two thermodynamics systems are in thermal equilibrium with a third, they are also in thermal equilibrium with each other ” A B C

13 A system in thermal equilibrium is a system whose macroscopic properties (like pressure, temperature, volume, etc.) are not changing in time When two systems are in thermal equilibrium:  both of the systems are in a state of equilibrium,  they remain so when they are brought into contact, where 'contact' is meant to imply the possibility of exchanging heat, but not work or particles

14 If a fluid is in thermal equilibrium with another system:  it has only one independent variable  the macroscopic properties have certain values

15 Isotherm Plot

16 Boyle’s Law  PV = f( θ ) Gay-Lussac’s Law  (PV) 1 (PV) 2 =  (  1,  2 ) (PV) 1 (PV) 2 = T1T1 T2T2 = T2T2 (PV) 1 T1T1

17 Ideal gas R = ideal gas constant (PV) T = nR


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