2020
DOI: 10.1007/s10909-020-02538-8
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$$^3$$He Universe 2020

Abstract: The latest news from $$^3$$ 3 He Universe are presented together with the extended map of the Universe.

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Cited by 16 publications
(18 citation statements)
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“…Of crucial importance for the spectrum of generated gravitational waves are the lifetime of the metastable phase and the propagation speed of the expanding phase boundary during the transition [5,6]. The simplest model, the homogeneous nucleation via thermal fluctuations by Cahn and Hilliard [7] and Langer [8], predicts a lifetime of the metastable supercooled 3 He-A longer than the age of the Universe under relevant experimental conditions [9,10]. The required large critical radius of the B-phase bubble (R c = 2σ AB /∆F AB ∼ 1 µm), at which the gain in bulk free energy density ∆F AB overcomes the surface tension σ AB and leads to an expanding bubble, is the underlying reason for this.…”
Section: Introductionmentioning
confidence: 99%
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“…Of crucial importance for the spectrum of generated gravitational waves are the lifetime of the metastable phase and the propagation speed of the expanding phase boundary during the transition [5,6]. The simplest model, the homogeneous nucleation via thermal fluctuations by Cahn and Hilliard [7] and Langer [8], predicts a lifetime of the metastable supercooled 3 He-A longer than the age of the Universe under relevant experimental conditions [9,10]. The required large critical radius of the B-phase bubble (R c = 2σ AB /∆F AB ∼ 1 µm), at which the gain in bulk free energy density ∆F AB overcomes the surface tension σ AB and leads to an expanding bubble, is the underlying reason for this.…”
Section: Introductionmentioning
confidence: 99%
“…Experimentally the phase transition between the A and B phases, usually from supercooled 3 He-A into 3 He-B, is routinely observed. This has led to proposals and studies of various heterogeneous nucleation mechanisms.…”
Section: Introductionmentioning
confidence: 99%
“…There is an ongoing search for a crystalline topological superconductor [13][14][15][16][17][18] and YbRh 2 Si 2 [19] is a candidate material that requires temperatures below a few mK. When cooling below 2.5 mK 3 He provides a benchmark for topological superconductivity, displaying a wealth of phenomena in the surface and edge states that arise from bulk-surface correspondence [20][21][22][23]. Strongly correlated electron systems exhibit quantum criticality [24][25][26], which is essentially a T = 0 phenomenon.…”
Section: Introductionmentioning
confidence: 99%
“…Topological superfluid phases of liquid 3 He provide many connections with the Standard Model of particle physics and gravity [1,2]. Here, we consider the symmetries and degeneracy of the Minkowski vacuum from the point of view of the symmetry breaking in the B-phase of superfluid 3 He [3].…”
Section: Introductionmentioning
confidence: 99%