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Entropy

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Entropy. Physics 313. Professor Lee Carkner. Lecture 17. Exercise #16 Entropy. Total entropy change is sum of each kg of water: DS = mc ln (Tf/Ti) mc ln (Tf/Ti) ... – PowerPoint PPT presentation

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Title: Entropy


1
Entropy
  • Physics 313
  • Professor Lee Carkner
  • Lecture 17

2
Exercise 16 Entropy
  • Total entropy change is sum of each kg of water
  • DS mc ln (Tf/Ti) mc ln (Tf/Ti)
  • Final temperature of water 50 C 323 K
  • DS (4186) ln (323/273) 4186 ln (323/373)
    704 602
  • Entropy increases, 2nd law OK
  • Entropy of air compression
  • DS nc ln (Tf/Ti) nR ln (Pf/Pi)
  • DS (34.5)(29.2) ln (330/290) (34.5)(8.31) ln
    (600000/100000) 130.2 514

3
Enthalpy
  • Enthalpy (H) is defined as
  • What is enthalpy?
  • u is the internal energy
  • Used in power generation, refrigerators, steam
    systems

4
Specific Enthalpy
  • Enthalpy per unit mass is the specific enthalpy
  • If we define a flow rate m (kg/s), the total
    power is
  • P mh
  • Both h and s are tabulated and can often be
    looked up

5
Turbines and Compressors
  • Turbine
  • Blades turn which turns shaft
  • Compressor
  • Blades compress a fluid
  • The PE and KE of the fluid are generally low, so
    the energy is dominated by enthalpy

6
Turbines
7
Isentropic Processes
  • This means that si sf
  • May have to extrapolate

8
Isentropic Efficiency
  • How close to maximum efficiency is a process?
  • Called the isentropic efficiency
  • Similar to comparing a engine to a Carnot cycle

9
Isentropic Efficiency Example
  • Turbine
  • A turbines work depends on the enthalpy so
  • where h2 is the actual and isentropic final state
    of the system

10
Cosmic Entropy
  • The second law holds for the entire universe
  • But, even when things get hotter,
  • What about black holes?
  • Where will it all end?

11
Cygnus X-1
12
Black Holes
  • How does entropy apply to a black hole?
  • Energy equals mass (general relativity)
  • If a box of gas is thrown in a black hole, the
    entropy of the universe decreases
  • Violates second law!

13
Black Holes and Entropy
  • Entropy is related to the size of the event
    horizon
  • Hot bodies emit radiation
  • Black holes aint so black!

14
Hawking Radiation
  • How can a black hole emit radiation?
  • You can create something out of nothing if you do
    it so fast the universe does not notice
    (uncertainty principle)
  • Black holes lose mass

15
Black Hole Temperature
  • Since a black hole has entropy, it must have a
    temperature
  • Low mass black holes are hotter than high mass
    ones
  • For a black hole formed in a supernova the
    minimum mass is about 3 solar masses
  • Washed out by 3 K cosmic microwave background

16
Arrows of Time
  • Three arrows of time
  • Thermodynamic
  • Psychological
  • Cosmological

17
Entropy and Memory
  • Memory requires energy dissipation as heat
  • Your head or a hard drive has to get hot

18
Synchronized Arrows
  • Why do all the arrows go in the same direction?
  • Can life exist with a backwards arrow of time?
  • Does life only exist with a forwards arrow of
    time? (anthropic principle)

19
Fate of the Universe
  • If the universe has enough mass, its expansion
    will reverse
  • Cosmological arrow will go backwards
  • Universe seems to be open
  • Universe will probably expand forever

20
Heat Death
  • Entropy keeps increasing
  • Stars burn out
  • Can live off of compact objects, but eventually
    will convert them all to heat
  • Universe becomes completely random radiation
    field
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