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Let's Know Things

Cold Fusion

Let's Know Things

Colin Wright

News Commentary, News

4.8593 Ratings

🗓️ 11 June 2019

⏱️ 38 minutes

🧾️ Download transcript

Summary

This week we talk about isotopes, the Fleischmann-Pons experiment, and pathological science.


We also discuss free energy suppression conspiracy theories, Google’s X Development, and the cold case of cold fusion.



This is a public episode. If you'd like to discuss this with other subscribers or get access to bonus episodes, visit letsknowthings.substack.com/subscribe

Transcript

Click on a timestamp to play from that location

0:00.0

Cold fusion is a broad term for a type of controlled nuclear fusion that can be induced and sustained at room

0:22.9

temperature. It's called cold fusion, because normal room temperature, or somewhere thereabouts,

0:29.3

is quite cold compared to the environment in which fusion reactions typically take place.

0:34.1

The pressure and heat are often quite extreme, as both are generally required, to force

0:38.7

elements that typically would not combine to combine, which is the fusion part of cold fusion,

0:44.9

and that combination of elements is what creates energy. Early research in this space actually

0:50.2

began back in the 1920s, when a couple of Austrian scientists seemed to have witnessed

0:55.5

hydrogen converting into helium. So the element with an atomic number of one, changing into the element

1:01.9

with an atomic number of two, implying that the process they were experimenting with, which involved

1:07.1

dividing pieces of palladium into tiny bits, in turn causing those bits to absorb hydrogen,

1:12.6

actually caused that hydrogen to combine into helium.

1:16.6

Which, well, that would have been amazing, except that that's not what happened.

1:20.6

Those scientists later retracted their report, indicating that the helium they had detected

1:25.6

was actually naturally occurring helium

1:28.1

from the air that they had interpreted as being otherwise, as being the consequence of this

1:33.6

thing that they were doing. Several other fairly big-name researchers and institutions invested

1:39.0

their time in resources in this field soon after, attempting various approaches to see if they could combine elements

1:45.1

in this way to create a new element, but also, and this was the real goal for most of these

1:51.1

projects, to create energy as a byproduct of that combination process. Because that energy

1:57.3

creation, the same type that takes place in stars, including our sun, by the way.

2:03.2

If we could make that happen at something closer to room temperature rather than star temperature,

2:08.6

we might be able to create abundant, clean energy, with few or even zero harmful byproducts.

...

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