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The nuclear fusion method comprises the following steps:
1. bringing hydrogen in a gaseous state into contact with a hydrogen transfer catalyst configured to cause a transition of the hydrogen from the gaseous state to an ultra-dense state;
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Because hydrogen is well known for doing that in the first place.
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2. collecting the hydrogen in the ultra-dense state on a carrier configured to substantially confine the hydrogen in the ultra-dense state within a fuel collection portion of the carrier;
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'Collect the hydrogen' written unnecessary long.
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3. transporting the carrier to an irradiation location; and subjecting, at the irradiation location, the hydrogen in the ultra-dense state to irradiation having sufficient energy to achieve break-even in energy generation by nuclear fusion.
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Because that is so easy. The pressure and temperature inside the sun are actually not high enought to overcome the Coulomb barrier... let that sink in for a moment.
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These materials are probably both superfluid and superconductive at room temperature, as predicted for ultra-dense deuterium and confirmed in recent experiments.
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My sides....