Beilstein J. Nanotechnol.2024,15, 26–36, doi:10.3762/bjnano.15.3
We consider properties of dichroicantenna arrays on a silicon substrate with integrated cold-electron bolometers to detect radiation at frequencies of 210 and 240 GHz. This frequency range is widely used in cosmic microwave background experiments in space, balloon, and ground-based missions such as
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Keywords: cosmic microwave background; B mode; cold-electron bolometer; dichroicantenna array; dipole bow-tie antenna; Josephson junction; LSPE; Introduction
The cosmic microwave background (CMB) radiation contains a lot of information about origin and evolution of our universe. The temperature and
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Figure 1:
(a) A view of the matrix of dipole antennas with integrated CEBs. (b) Enlarged view of the receivin...
Beilstein J. Nanotechnol.2022,13, 865–872, doi:10.3762/bjnano.13.77
of 1.1 × 10−16 W/Hz1/2. This was achieved by replacing one of two superconductor–insulator–normal tunnel junctions with a superconductor–normal metal contact.
Keywords: cosmic microwave background (CMB); cold-electron bolometer; dichroicantenna; dipole antenna; LSPE-SWIPE; waveguide horn
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Figure 1:
The front part and the constriction of the back-to-back horn of the LSPE-SWIPE receiving system [3] us...