2010
DOI: 10.1143/ptps.184.153
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From the Frenkel-Kontorova Model to Josephson Junction Arrays

Abstract: The Frenkel-Kontorova (FK) model is known to exhibit so-called Aubry's transition which is a jamming or frictional transition at zero temperature. Recently we found similar transition at zero and finite temperatures in a superconducting Josephson junction array (JJA) on a square lattice under external magnetic field. In the present paper we discuss how these problems are related.at North Dakota State University on July 6, 2015 http://ptps.oxfordjournals.org/ Downloaded from * ) The FK model with fixed volume (… Show more

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Cited by 15 publications
(34 citation statements)
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“…It is most efficient to populate the highest possible L z state, i.e., m = l. For m < l, τ −1 SR is much smaller. Thus in the following discussion, we take m = l. The superradiance process keeps producing particles until the self-interaction among these bosons becomes important, which leads to non-linear region [34,35,[38][39][40]. In this region, one needs to take into account the whole potential in the effective Lagrangian…”
Section: Superradiance and Bosenovamentioning
confidence: 99%
See 1 more Smart Citation
“…It is most efficient to populate the highest possible L z state, i.e., m = l. For m < l, τ −1 SR is much smaller. Thus in the following discussion, we take m = l. The superradiance process keeps producing particles until the self-interaction among these bosons becomes important, which leads to non-linear region [34,35,[38][39][40]. In this region, one needs to take into account the whole potential in the effective Lagrangian…”
Section: Superradiance and Bosenovamentioning
confidence: 99%
“…When the Compton wavelength of an axion is at the same order of a rotating black hole size, the axion is expected to develop a large density near the horizon, forming an axion cloud through the superradiance mechanism [25][26][27][28][29][30][31][32] (for a review see [33]). Such superradiance process can be tested by black hole spin measurements [34][35][36][37], gravitational wave signals from bosenova [34,35,[38][39][40][41][42] or electromagnetic emission from the axion cloud [43]. In this letter, we propose a novel way of detecting axion cloud around SMBH by using the polari-metric measurements of the EHT.…”
Section: Introductionmentioning
confidence: 99%
“…At a certain threshold force the particles start to move, and for high forces the velocity slowly merges into the free velocity. Such a continuous depinning scenario seems to be a universal feature, since it can be found in many different systems ranging from classical colloids to quantum systems as mentioned in the Introduction [13,[19][20][21][22][23][24].…”
Section: B Transportmentioning
confidence: 97%
“…A continuous depinning at finite temperatures, as in the colloidal model systems [13,19], can also be found in quantum systems, such as the domain-wall motion in spin systems on nanofibers [20,21] or the dynamics in Josephson junction arrays [22][23][24].…”
Section: Introductionmentioning
confidence: 97%
“…The question then arises as to what is expected as the final fate of an unstable black hole? A stable hairy black hole [5,6,28] or an explosion event called bosenova [30,31] are two possible candidates describing the final state of a superradiantly unstable system both in GR or alternatively in F (R) theories of gravity [8].…”
Section: Introductionmentioning
confidence: 99%