Ultra high pressure supersolid helium

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SUMMARY

The discussion centers on the theoretical implications of pressurizing helium beyond its supersolid state, exploring the potential for helium to exhibit properties similar to metallic hydrogen under extreme pressures. Participants speculate on the transition pressures required for helium-4 to behave as a degenerate gas with superfluid and superconducting characteristics. The conversation references a phase diagram of helium-4, highlighting the complexities of achieving such states and the challenges posed by material and engineering limitations.

PREREQUISITES
  • Understanding of phase diagrams, specifically for helium-4.
  • Knowledge of supersolid and superfluid states in quantum mechanics.
  • Familiarity with the properties of metallic hydrogen and degenerate gases.
  • Basic principles of high-pressure physics and material science.
NEXT STEPS
  • Research the phase diagram of helium-4 and its implications for state transitions.
  • Investigate the properties and formation conditions of metallic hydrogen.
  • Explore the behavior of superfluid helium under varying pressure conditions.
  • Study the engineering challenges associated with high-pressure experiments on helium.
USEFUL FOR

Physicists, materials scientists, and researchers interested in quantum states of matter, particularly those studying high-pressure phenomena and the properties of helium under extreme conditions.

andrew848
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TL;DR
I was wondering what would happened if you cooled helium to near absolute zero and kept pressurizing it.
Assuming you could get around the material and engineering problems with anything at high pressures what would happen if you kept pressurizing helium past a super solid state. If the pressures where high enough would you have a similar effect to metallic hydrogen with it behaving as a degenerate gas with superfluid and superconductor properties?
 
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There is a phase diagram of helium 4 here
https://i.stack.imgur.com/pymYA.jpg
I presume all materials become 'metallic' at some pressure (possibly not fermions like He-3??), the question is what that pressure is predicted to be and if there is ever a physically real situation where it might get there?
 

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