scholarly journals Amplified and tunable transverse and longitudinal spin-photon coupling in hybrid circuit-QED

2018 ◽  
Vol 97 (12) ◽  
Author(s):  
Neill Lambert ◽  
Mauro Cirio ◽  
Matthieu Delbecq ◽  
Giles Allison ◽  
Marian Marx ◽  
...  
2013 ◽  
Vol 103 (1) ◽  
pp. 17005 ◽  
Author(s):  
Neill Lambert ◽  
Christian Flindt ◽  
Franco Nori

2011 ◽  
Vol 51 (5) ◽  
pp. 1482-1490 ◽  
Author(s):  
Qin-Qin Wu ◽  
Lan Xu ◽  
Qing-Shou Tan ◽  
Lin-Ling Yan

2014 ◽  
Vol 53 (9) ◽  
pp. 3078-3088 ◽  
Author(s):  
Juju Hu ◽  
Jianhua Huang ◽  
Haijiang Hu ◽  
Yinghua Ji

2013 ◽  
Vol 15 (9) ◽  
pp. 095008 ◽  
Author(s):  
L D Contreras-Pulido ◽  
C Emary ◽  
T Brandes ◽  
Ramón Aguado

2020 ◽  
Vol 117 (11) ◽  
pp. 114001
Author(s):  
T. Cubaynes ◽  
L. C. Contamin ◽  
M. C. Dartiailh ◽  
M. M. Desjardins ◽  
A. Cottet ◽  
...  

ChemPhysChem ◽  
2021 ◽  
Vol 22 (12) ◽  
pp. 1148-1148
Author(s):  
Ewoud Vaneeckhaute ◽  
Sophie De Ridder ◽  
Jean‐Max Tyburn ◽  
James G. Kempf ◽  
Francis Taulelle ◽  
...  

2021 ◽  
Vol 2021 (6) ◽  
Author(s):  
Anson Hook ◽  
Gustavo Marques-Tavares ◽  
Clayton Ristow

Abstract We present the supernova constraints on an axion-photon-dark photon coupling, which can be the leading coupling to dark sector models and can also lead to dramatic changes to axion cosmology. We show that the supernova bound on this coupling has two unusual features. One occurs because the scattering that leads to the trapping regime converts axions and dark photons into each other. Thus, if one of the two new particles is sufficiently massive, both production and scattering become suppressed and the bounds from bulk emission and trapped (area) emission both weaken exponentially and do not intersection The other unusual feature occurs because for light dark photons, longitudinal modes couple more weakly than transverse modes do. Since the longitudinal mode is more weakly coupled, it can still cause excessive cooling even if the transverse mode is trapped. Thus, the supernova constraints for massive dark photons look like two independent supernova bounds super-imposed on top of each other.


2021 ◽  
Vol 103 (4) ◽  
Author(s):  
A. Ciani ◽  
B. M. Terhal
Keyword(s):  

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