skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Planar Self-similar Antennas for Broadband Millimeter-Wave Measurements

Journal Article · · Journal of Low Temperature Physics
 [1];  [1];  [2];  [2];  [3];  [4];  [4];  [5];  [6];  [7];  [7]
  1. Arizona State Univ., Tempe, AZ (United States)
  2. Columbia Univ., New York, NY (United States)
  3. Stanford Univ., CA (United States)
  4. SLAC National Accelerator Lab., Menlo Park, CA (United States)
  5. NASA Jet Propulsion Lab. (JPL), Pasadena, CA (United States)
  6. Univ. of Michigan, Ann Arbor, MI (United States)
  7. Cardiff Univ. (United Kingdom)

Self-similar antennas offer extremely broadband functionality and easily scalable designs. Self-similar designs with a four-arm layout are also suited for dual polarization through excitations of opposing arms, although there has only been limited use of them for millimeter-wave detectors. These antennas have been used for measurements of the cosmic microwave background (CMB), which encompass a wide frequency range and are now actively focusing more on polarization anisotropies. Here, we analyze multiple planar self-similar antenna designs with simulations in high-frequency structure simulator and ongoing physical testing. They all exhibit broadband operation between 130 and 230 GHz and can couple to both linear polarizations through the previously mentioned four-arm symmetry. Furthermore, simulations include each antenna design coupled to an extended hemispherical, AR-coated lenslet. From these, a basic bowtie-like arm design produced minimal polarization wobble with moderate beam efficiency, while a hybrid trapezoidal design provided high beam efficiency with small polarization wobble. Current fabrication versions of each are being tested, coupled to multichroic microwave kinetic inductance detectors. These planar self-similar antennas, when implemented in CMB and other detectors, could improve observations while simultaneously simplifying fabrication and detector layout.

Research Organization:
SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC); National Science Foundation (NSF)
Grant/Contract Number:
AC02-76SF00515; 1509211; 1711160; 1509078; 1711242; 1506074; 1710624
OSTI ID:
1608338
Journal Information:
Journal of Low Temperature Physics, Vol. 199, Issue 1-2; ISSN 0022-2291
Publisher:
SpringerCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 2 works
Citation information provided by
Web of Science

References (8)

Impedance properties of complementary multiterminal planar structures journal December 1959
A CMB polarization primer journal October 1997
Dual-Polarized Sinuous Antennas on Extended Hemispherical Silicon Lenses journal September 2012
Miniaturized antenna-arrays for combined wideband polarization- and space diversity conference January 2006
Planck 2015 results : I. Overview of products and scientific results journal September 2016
Development of Multi-chroic MKIDs for Next-Generation CMB Polarization Studies journal July 2018
Novel logarithmically periodic planar antennas for broadband polarization diversity reception journal July 2005
Multi-Chroic Dual-Polarization Bolometric Detectors for Studies of the Cosmic Microwave Background journal January 2014

Similar Records

Development of Multi-chroic MKIDs for Next-Generation CMB Polarization Studies
Journal Article · Mon Jul 30 00:00:00 EDT 2018 · Journal of Low Temperature Physics · OSTI ID:1608338

Commercialization of Micro-fabrication of Antenna-Coupled Transition Edge Sensor Bolometer Detectors for Studies of the Cosmic Microwave Background
Journal Article · Mon Apr 09 00:00:00 EDT 2018 · Journal of Low Temperature Physics · OSTI ID:1608338

Large arrays of dual-polarized multichroic TES detectors for CMB measurements with the SPT-3G receiver
Journal Article · Tue Jul 19 00:00:00 EDT 2016 · Proceedings of SPIE - The International Society for Optical Engineering · OSTI ID:1608338