2010
DOI: 10.1103/physrevd.82.123002
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Limits on the time variation of the Fermi constantGFbased on type Ia supernova observations

Abstract: The light curve of a type Ia supernova decays at a rate set by the β-decay lifetimes of the 56 Ni and 56 Co produced in the explosion. This makes such a light curve sensitive

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Cited by 10 publications
(8 citation statements)
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“…Important results obtained by cluster dynamical mean-field methods have included the demonstration that in an appropriate doping and interaction range the two-dimensional Hubbard model can exhibit a pseudogap, 30,31 "Fermi arcs", [32][33][34][35][36] and a variation in electronic properties around the Fermi surface ("nodalantinodal differentiation"). [31][32][33][37][38][39] The methods have been shown to yield a multistage approach to the Mott transition with the insulating phase being separated from the weakly correlated metallic phase by a "sectorselective" phase where some regions of the Brillouin zone are gapped and others are not 37,38,40,41 and a number of physical properties were shown to be in good agreement with experiment. 38,39,42 Despite these successes, uncertainties remain.…”
Section: Introductionmentioning
confidence: 99%
“…Important results obtained by cluster dynamical mean-field methods have included the demonstration that in an appropriate doping and interaction range the two-dimensional Hubbard model can exhibit a pseudogap, 30,31 "Fermi arcs", [32][33][34][35][36] and a variation in electronic properties around the Fermi surface ("nodalantinodal differentiation"). [31][32][33][37][38][39] The methods have been shown to yield a multistage approach to the Mott transition with the insulating phase being separated from the weakly correlated metallic phase by a "sectorselective" phase where some regions of the Brillouin zone are gapped and others are not 37,38,40,41 and a number of physical properties were shown to be in good agreement with experiment. 38,39,42 Despite these successes, uncertainties remain.…”
Section: Introductionmentioning
confidence: 99%
“…While precise details of the explosion itself remain to be understood, the fading luminosity of a supernova days to months after the explosion is governed by beta decays of 56 Ni and 56 Co, as it has been confirmed in 2014 by direct observations [3,4]. This fact has been used [5,6] to constrain spacetime variations of the decay rates, which are determined by the Fermi constant G F . In the Standard Model, this "constant" is directly related to the vacuum expectation value v of the Brout-Englert-Higgs scalar field.…”
Section: Introductionmentioning
confidence: 96%
“…The relation between the amount of decaying isotopes and the supernova luminosity is not direct and we refer the reader to previous studies [5,6] for discussions of this point.…”
Section: Introductionmentioning
confidence: 99%
“…25.Jb The mechanism of interlayer (c-axis) transport in cuprate high temperature superconductors remains an actively debated subject. A qualitative difference between metallic in-plane and non-metallic out-of-plane resistivities [1] is a strong indication for predominantly incoherent nature of c-axis transport, which is achieved by interlayer hopping or tunneling [2][3][4][5][6][7]. The tunneling nature of c-axis transport leads to appearance of the intrinsic Josephson effect between CuO 2 planes in layered Bi 2 Sr 2 CaCu 2 O 8+δ (Bi-2212) cuprates at temperatures below T c [8].…”
mentioning
confidence: 99%