Unravelling the Mystery of Free Energy

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SUMMARY

The discussion centers on the concept of free energy, particularly in relation to water dissociation into H+ and OH- ions. Participants clarify that while energy is required to dissociate water, the energy released when these ions recombine is equal to the energy input, adhering to the conservation of energy principle. The conversation also explores the potential of infrared to electric converters as a means to harness energy, but emphasizes the limitations imposed by thermodynamics and the low intensity of ambient infrared radiation. Ultimately, the feasibility of extracting usable energy from ambient sources remains highly questionable.

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  • Understanding of thermodynamics and conservation of energy principles
  • Knowledge of water dissociation and electrolysis processes
  • Familiarity with infrared radiation and its properties
  • Basic concepts of photovoltaic cells and their operation
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  • Research the principles of thermodynamics and their implications for energy extraction
  • Study the electrolysis of water and its applications in energy generation
  • Explore advancements in infrared to electric conversion technologies
  • Investigate the efficiency and economics of solar energy systems
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Researchers, engineers, and students interested in renewable energy technologies, thermodynamics, and the practical applications of energy conversion methods.

  • #91


A impressively quick reply!

I have read K. Browne’s paper and in a nut shell he shows that for the two geometries studied, the target had a larger surface area than the sending object. Consequently the targets emitted all that they received from the emitter without raising their temperatures. My design is different in that the target is smaller than the emitter and so will receive a concentration of photons as envisaged by Sudhir Panse. Browne does not cover this eventuality even though he says that other geometries may be found, This is why I am still pursing it. Unless I learn something new that explains why it shouldn’t work, I will continue making the device. I expect to complete the device in the next 2 months when all my questions will be answered. If it doesn't work I shall still be looking for answers LOL

I have often heard the answer that the second law of thermodynamics says it can’t be done. People who say this have been unable to tell me why it won’t work or have some spurious illogical answer. There may well be a reason deep down in the realm of quantum mechanics why it won’t work but I have not heard it yet.

I suggest that the second law of thermodynamics was created from 300 or so years of empirical observation and is not tied to any mathematical proof. This leaves it open to future findings.

Your suggestions are welcome and may save me a great deal of work and expense.

As I said, my math may be wrong but here goes :
I used this site to compute the energy collected at the emitter :
http://hyperphysics.phy-astr.gsu.edu/Hbase/thermo/stefan.html#c3
As I only want the energy emitted, not the net difference between two bodies, I used a T cold of 0K and a T hot of 300K with a collector area of 153.94 sq mm

(oops found my error - I put in 153.94 sq cm not 153.94 sq mm)

Collector collects 0.0707037 watts

I would need 1,000,000 / 153.94 collectors to get 1 sq m = 6,496.12 collectors

# of collectors * watts per collector = 0.0707037 * 6,496.12 = 459.27 watts or 0.62 HP

That certainly looks more reasonable, thanks for the pointer.

At this (now corrected ) rate it looks like the emitted energy is just under half that of the solar energy per unit area. The difference however is that radiant energy runs 24/7 and is not reliant on latitude or cloud cover and so is still a very attractive goal.
 
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  • #92


It is trivially easy to prove that this idea of yours is false - anyone who owns a telescope could point it at a wall and expect to be able to burn a hole in a piece of paper!
 
  • #93


You are correct. The telescope won’t burn a hole in a piece of paper. That is simply because the telescope would not focus ALL the radiant energy from the wall, only those minuscule small number of rays that travel in a parallel manner towards the telescope.

I like your site and am particularly impressed with the Hubble image.
 
Last edited by a moderator:
  • #94


Habanabasa said:
As I only want the energy emitted, not the net difference between two bodies, I used a T cold of 0K and a T hot of 300K with a collector area of 153.94 sq mm

Isn't this a problem? I have to admit I don't follow all of the arguments above, but think about what is keeping your emitter at the temperature of 300K. Isn't it just all of the 'random' radiant energy bouncing around between the emitter and its surroundings?
 
  • #95


Habanabasa said:
You are correct. The telescope won’t burn a hole in a piece of paper. That is simply because the telescope would not focus ALL the radiant energy from the wall, only those minuscule small number of rays that travel in a parallel manner towards the telescope.
Unless the telescope is right up against the wall, the amount of radiation that is not parallel will be miniscule! Besides - even if it misses a quarter or half the radiation, it can still focus light to thousands of times the intensity with which it was emitted: looking at a wall with a telescope as big as mine would be painful to your eyes.
I like your site and am particularly impressed with the Hubble image.
Thanks!
 
  • #96


Anyway, sorry, but this discussion is explicitly against forum guidelines. We deal only in established science here.
 

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