First Law of Thermodynamics: Principles, Applications, and Examples - Prof. Serdf, Schemes and Mind Maps of Mathematical Methods

A comprehensive overview of the first law of thermodynamics, exploring its fundamental principles, key concepts, and practical applications. It delves into the conservation of energy, mechanisms of energy transfer, and the relationship between internal energy, enthalpy, and specific heats. The document also includes illustrative examples to solidify understanding and demonstrate the application of the first law in various engineering contexts.

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Chapter Three
The First Law of Thermodynamics
Engineering Thermodynamics I
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Chapter Three

The First Law of Thermodynamics

Engineering Thermodynamics I

The First Law of Thermodynamics

  • (^) The first law is usually referred to as the law of
conservation of energy, i.e.
energy can neither be created nor destroyed, but rather
transformed from one state to another.
  • (^) The energy balance is maintained within the system.
  • (^) The various energies associated are then being
observed as they cross the boundaries of the system.

The First Law of Thermodynamics [Cont…]

  • The^ total energy of the system,^ E system

, is given

as

system

E = Internal Energy + Kinetic Energy + Potential Energy

system E = U + KE + PE

  • (^) Any change in the total energy of the system is

due to energy crossing the boundaries

The First Law of Thermodynamics [Cont…]

  • (^) If the system does not move with a velocity and has
no change in elevation, it is called a stationary
system , and the conservation of energy equation
reduces to

in out E  E U

Energy Balance

  • (^) The energy balance can be written more explicitly as , , ( ) ( ) ( ) in out in out in out mass in mass out System E  E  Q  Q  W  W  E  E E  (^) in out  (^) Net energy transfer  (^) System (^) Change in internal, kinetic,  by heat, work and mass (^) potential, etc..energies E  E  E kJ
  • (^) Or on a rate form, as

The first law and a closed system

  • (^) For the closed system where the mass never crosses the system boundary, then the energy balance is      in out in out system Q -Q + W -W = E

The first law and a closed system [Cont…]

  • (^) If the total energy is a combination of internal energy, kinetic energy and potential energy
  • (^) For negligible changes in kinetic and potential energy E U  KE  PE   2 2 2 1 12 12 2 1 2 1
m V V
Q W U U mg Z Z

  12 2 1 12 Q  U  U W

Internal energy and Enthalpy

  • (^) Internal energy
    • (^) The internal energy includes some complex forms of energy show up due to translation, rotation and vibration of molecules.
    • (^) It is designated by U and it is extensive property.
    • (^) Or per unit mass as, specific internal energy,
  • (^) If we take two phase as liquid and vapor at a given
saturation pressure or temperature

U u m  f g U U  U f f g g mu m u m u f fg u u xu

Specific Heat

  • (^) It defined as; the energy required to raise the
temperature of a unit mass of a substance by one
degree.
  • (^) It is an intensive property of a substance that will
enable us to compare the energy storage capability of
various substances. The unit is.
  • (^) In thermodynamics, we are interested in two kinds of
specific heats: specific heat at constant volume and
specific heat at constant pressure.

KJ (^) or KJ Kg KgK

  • (^) The specific heat at constant volume can be viewed
as the energy required to raise the temperature of the
unit mass of a substance by one degree as the volume
is maintained constant.
  • (^) Here the boundary work is zero because the volume is
constant
  • (^) From first law
  • (^) Per unit mass δQ dU  q du v  q C dT v C dT du v v du C dT       

Internal Energy, Enthalpy, and Specific Heats of Ideal Gases

  • (^) We defined an ideal gas as a gas whose temperature, pressure, and specific volume are related by
  • (^) From the specific heat relation
  • (^) Or taking average value of specific heat for narrow temperature difference Pv RT v du C dT
u 2  u 1 C dTv

u 2  u 1 C (^) ave v (^) , ( T 2  T 1 )

dh C p T dT

2 1 p h  h  C dT  h 2  h 1 C (^) ave p (^) , (T 2  T 1 )

Relation between C P and C V for Ideal Gases

  • (^) Replacing by and by we have
  • (^) At this point, we introduce another ideal-gas property called the specific heat ratio k, defined as h u  RT dh^ du^ RdT
dh

p

C dT du^ C dTv

p v C dT C dT RdT p v C C R p v C K C  p v C KC KCv^ C^ v^ R 1 v R C K   p p C C R K   1 p K C R K  

Examples

Examples

1. The initial pressure and volume of a piston-

cylinder arrangement is 200kPa and 1m

3

respectively. 2000kJ of heat is transferred to

the system and the final volume is 2m

3

Determine the change in the internal energy

of the fluid.