Fully Superconducting Josephson Bolometers for Gigahertz Astronomy

The origin and the evolution of the universe are concealed in the evanescent diffuse extragalactic background radiation (DEBRA). To reveal these signals, the development of innovative ultra-sensitive bolometers operating in the gigahertz band is required. Here, we review the design and experimental...

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Main Authors: Federico Paolucci, Nadia Ligato, Gaia Germanese, Vittorio Buccheri, Francesco Giazotto
Format: Article
Language:English
Published: MDPI AG 2021-01-01
Series:Applied Sciences
Subjects:
Online Access:https://www.mdpi.com/2076-3417/11/2/746
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author Federico Paolucci
Nadia Ligato
Gaia Germanese
Vittorio Buccheri
Francesco Giazotto
author_facet Federico Paolucci
Nadia Ligato
Gaia Germanese
Vittorio Buccheri
Francesco Giazotto
author_sort Federico Paolucci
collection DOAJ
description The origin and the evolution of the universe are concealed in the evanescent diffuse extragalactic background radiation (DEBRA). To reveal these signals, the development of innovative ultra-sensitive bolometers operating in the gigahertz band is required. Here, we review the design and experimental realization of two bias-current-tunable sensors based on one dimensional fully superconducting Josephson junctions: the nanoscale transition edge sensor (nano-TES) and the Josephson escape sensor (JES). In particular, we cover the theoretical basis of the sensors operation, the device fabrication, their experimental electronic and thermal characterization and the deduced detection performance. Indeed, the nano-TES promises a state-of-the-art noise equivalent power (NEP) of about <inline-formula><math display="inline"><semantics><mrow><mn>5</mn><mo>×</mo><msup><mn>10</mn><mrow><mo>−</mo><mn>20</mn></mrow></msup></mrow></semantics></math></inline-formula> W<inline-formula><math display="inline"><semantics><mrow><mo>/</mo><msqrt><mi>Hz</mi></msqrt></mrow></semantics></math></inline-formula>, while the JES active region is expected to show an unprecedented NEP of the order of <inline-formula><math display="inline"><semantics><msup><mn>10</mn><mrow><mo>−</mo><mn>25</mn></mrow></msup></semantics></math></inline-formula> W<inline-formula><math display="inline"><semantics><mrow><mo>/</mo><msqrt><mi>Hz</mi></msqrt></mrow></semantics></math></inline-formula>. Therefore, the nano-TES and JES are strong candidates to push radio astronomy to the next level.
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spelling doaj.art-28d551031b8c41eaaf48a073c2fd25202023-12-03T13:13:03ZengMDPI AGApplied Sciences2076-34172021-01-0111274610.3390/app11020746Fully Superconducting Josephson Bolometers for Gigahertz AstronomyFederico Paolucci0Nadia Ligato1Gaia Germanese2Vittorio Buccheri3Francesco Giazotto4NEST, Istituto Nanoscienze-CNR and Scuola Normale Superiore, I-56127 Pisa, ItalyNEST, Istituto Nanoscienze-CNR and Scuola Normale Superiore, I-56127 Pisa, ItalyNEST, Istituto Nanoscienze-CNR and Scuola Normale Superiore, I-56127 Pisa, ItalyNEST, Istituto Nanoscienze-CNR and Scuola Normale Superiore, I-56127 Pisa, ItalyNEST, Istituto Nanoscienze-CNR and Scuola Normale Superiore, I-56127 Pisa, ItalyThe origin and the evolution of the universe are concealed in the evanescent diffuse extragalactic background radiation (DEBRA). To reveal these signals, the development of innovative ultra-sensitive bolometers operating in the gigahertz band is required. Here, we review the design and experimental realization of two bias-current-tunable sensors based on one dimensional fully superconducting Josephson junctions: the nanoscale transition edge sensor (nano-TES) and the Josephson escape sensor (JES). In particular, we cover the theoretical basis of the sensors operation, the device fabrication, their experimental electronic and thermal characterization and the deduced detection performance. Indeed, the nano-TES promises a state-of-the-art noise equivalent power (NEP) of about <inline-formula><math display="inline"><semantics><mrow><mn>5</mn><mo>×</mo><msup><mn>10</mn><mrow><mo>−</mo><mn>20</mn></mrow></msup></mrow></semantics></math></inline-formula> W<inline-formula><math display="inline"><semantics><mrow><mo>/</mo><msqrt><mi>Hz</mi></msqrt></mrow></semantics></math></inline-formula>, while the JES active region is expected to show an unprecedented NEP of the order of <inline-formula><math display="inline"><semantics><msup><mn>10</mn><mrow><mo>−</mo><mn>25</mn></mrow></msup></semantics></math></inline-formula> W<inline-formula><math display="inline"><semantics><mrow><mo>/</mo><msqrt><mi>Hz</mi></msqrt></mrow></semantics></math></inline-formula>. Therefore, the nano-TES and JES are strong candidates to push radio astronomy to the next level.https://www.mdpi.com/2076-3417/11/2/746radio astronomyJosephson effecttransition edge sensorJosephson escape sensornanodevicesgigahertz detection
spellingShingle Federico Paolucci
Nadia Ligato
Gaia Germanese
Vittorio Buccheri
Francesco Giazotto
Fully Superconducting Josephson Bolometers for Gigahertz Astronomy
Applied Sciences
radio astronomy
Josephson effect
transition edge sensor
Josephson escape sensor
nanodevices
gigahertz detection
title Fully Superconducting Josephson Bolometers for Gigahertz Astronomy
title_full Fully Superconducting Josephson Bolometers for Gigahertz Astronomy
title_fullStr Fully Superconducting Josephson Bolometers for Gigahertz Astronomy
title_full_unstemmed Fully Superconducting Josephson Bolometers for Gigahertz Astronomy
title_short Fully Superconducting Josephson Bolometers for Gigahertz Astronomy
title_sort fully superconducting josephson bolometers for gigahertz astronomy
topic radio astronomy
Josephson effect
transition edge sensor
Josephson escape sensor
nanodevices
gigahertz detection
url https://www.mdpi.com/2076-3417/11/2/746
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AT nadialigato fullysuperconductingjosephsonbolometersforgigahertzastronomy
AT gaiagermanese fullysuperconductingjosephsonbolometersforgigahertzastronomy
AT vittoriobuccheri fullysuperconductingjosephsonbolometersforgigahertzastronomy
AT francescogiazotto fullysuperconductingjosephsonbolometersforgigahertzastronomy