Showing posts with label Nickolay Kinev. Show all posts
Showing posts with label Nickolay Kinev. Show all posts

Thursday, November 23, 2017

Abstract-Self-Mixing Spectra of Terahertz Emitters Based on Bi 2 Sr 2 CaCu 2 O 8 + δ Intrinsic Josephson-Junction Stacks


Ya Huang, Hancong Sun, Deyue An, Xianjing Zhou, Min Ji, Fabian Rudau, Raphael Wieland, Johannes S. Hampp, Olcay Kizilaslan, Jie Yuan, Nickolay Kinev, Oleg Kiselev, Valery P. Koshelets, Jun Li, Dieter Koelle, Reinhold Kleiner, Biaobing Jin, Jian Chen, Lin Kang, Weiwei Xu, Huabing Wang, and Peiheng Wu

https://journals.aps.org/prapplied/abstract/10.1103/PhysRevApplied.8.054023

Josephson junctions can serve as mixers for electromagnetic radiation, producing difference frequencies |mfsnfLO| of the signal frequency fs and the local oscillator frequency fLO, where the latter can be provided by ac Josephson currents, and m and n are natural numbers. In order to obtain a better understanding of the purity of the terahertz radiation generated by stacks of intrinsic Josephson junctions (IJJs), we study self-mixing—i.e., fs is also produced by Josephson currents inside the stacks—in the difference-frequency range between 0.1 and 3.0 GHz. Simultaneously, we perform off-chip terahertz emission detection and transport measurements. We find that at high-bias currents, when a hot spot has formed in the stack, the power level of self-mixing can be low and sometimes is even absent at the terahertz emission peak, pointing to a good phase locking among all IJJs. By contrast, at low-bias currents where no hot spot exists, the self-mixing products are pronounced even if the terahertz emission peaks are strong. The mixing products at high operation temperature, at which the temperature variation within the stack is moderate, are minor, indicating that the low junction resistance, perhaps in combination with the lowered Josephson critical current density, may play a similar role for synchronization as the hot spot does at low temperature. While these observations are helpful for the task to synchronize thousands of IJJs, the observation of self-mixing in general may offer a simple method in evaluating the coherence of terahertz radiation produced by the IJJ stacks.

Sunday, August 12, 2012

Abstract-Linewidth dependence of coherent terahertz emission from Bi2Sr2CaCu2O8 intrinsic Josephson junction stacks in the hot-spot regime



http://prb.aps.org/abstract/PRB/v86/i6/e060505
Mengyue Li
1,2, Jie Yuan2,3,*, Nickolay Kinev4, Jun Li2,5, Boris Gross6, Stefan Guénon6, Akira Ishii2, Kazuto Hirata2, Takeshi Hatano2, Dieter Koelle6, Reinhold Kleiner6, Valery P. Koshelets4, Huabing Wang1,2,†, and Peiheng Wu1 
1Research Institute of Superconductor Electronics, Nanjing University, Nanjing 210093, China
2National Institute for Materials Science, Tsukuba 3050047, Japan
3Department of Applied Physics, Wuhan University of Science and Technology, Wuhan 430081, China
4Kotel'nikov Institute of Radio Engineering and Electronics, Moscow 125009, Russia
5Hokkaido University, Hokkaido 0600810, Japan
6Physikalisches Institut and Center for Collective Quantum Phenomena in LISA+, Universität Tübingen, D-72076 Tübingen, Germany
 Received 3 April 2012; revised 20 July 2012; published 8 August 2012
We report on measurements of the linewidth Δf of terahertz radiation emitted from intrinsic Josephson junction stacks, using a Nb/AlN/NbN integrated receiver for detection. Previous resolution-limited measurements indicated that Δf may be below 1 GHz—much smaller than expected from a purely cavity-induced synchronization. While at low bias we found Δf to be not smaller than ∼500 MHz, at high bias, where a hot spot coexists with regions which are still superconducting, Δfturned out to be as narrow as 23 MHz. We attribute this to the hot spot acting as a synchronizing element. Δf decreases with increasing bath temperature, a behavior reminiscent of motional narrowing in NMR or electron spin resonance (ESR), but hard to explain in standard electrodynamic models of Josephson junctions.
©2012 American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevB.86.060505
DOI:
10.1103/PhysRevB.86.060505
PACS:
74.50.+r, 74.72.-h, 85.25.Cp
*phy.wust@gmail.com
hbwang1000@gmail.com