Concept Study of Optical Configurations for High-Frequency Telescope for LiteBIRD

被引：0

作者：

T. Hasebe

S. Kashima

P. A. R. Ade

Y. Akiba

D. Alonso

K. Arnold

J. Aumont

C. Baccigalupi

D. Barron

S. Basak

S. Beckman

J. Borrill

F. Boulanger

M. Bucher

E. Calabrese

Y. Chinone

H.-M. Cho

A. Cukierman

D. W. Curtis

T. de Haan

M. Dobbs

A. Dominjon

T. Dotani

L. Duband

A. Ducout

J. Dunkley

J. M. Duval

T. Elleflot

H. K. Eriksen

J. Errard

J. Fischer

T. Fujino

T. Funaki

U. Fuskeland

K. Ganga

N. Goeckner-Wald

J. Grain

N. W. Halverson

T. Hamada

M. Hasegawa

K. Hattori

M. Hattori

L. Hayes

M. Hazumi

N. Hidehira

C. A. Hill

G. Hilton

J. Hubmayr

K. Ichiki

T. Iida

机构：

[1] Aoyama Gakuin University,Astronomical Institute, Graduate School of Science

[2] Tohoku University,AstroParticule et Cosmologie (APC)

[3] Univ Paris Diderot,Center for Astrophysics and Space Astronomy

[4] CNRS/IN2P3,Computational Cosmology Center

[5] CEA/Irfu,DAMTP

[6] Obs de Paris,Department of Astronomy

[7] University of Colorado,Department of Astrophysical and Planetary Sciences

[8] CNRS,Department of Astrophysical Sciences

[9] IRAP,School of Physics

[10] Lawrence Berkeley National Laboratory,Department of Physics

[11] University of Cambridge,Department of Physics

[12] The University of Tokyo,Department of Physics

[13] University of Colorado,Department of Physics

[14] Princeton University,Department of Physics

[15] Indian Institute of Science Education and Research Thiruvananthapuram,Department of Physics

[16] Okayama University,CEA, INAC

[17] Stanford University,SBT

[18] The University of Tokyo,Institut d’Astrophysique Spatiale (IAS), CNRS, UMR 8617

[19] University of California,Institute of Physics

[20] University of California,Institute of Space and Astronautical Science (ISAS)

[21] University of Colorado,Research and Development Directorate

[22] University of Grenoble Alpes,Institute of Theoretical Astrophysics

[23] High Energy Accelerator Research Organization (KEK),Kavli Institute for Particle Astrophysics and Cosmology (KIPAC)

[24] Université Paris-Sud 11,Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU, WPI), UTIAS

[25] Academia Sinica,Kobayashi

[26] Japan Aerospace Exploration Agency (JAXA),Maskawa Institute for the Origin of Particle and the Universe

[27] Japan Aerospace Exploration Agency (JAXA),Laboratoire de l’Accélérateur Linéaire (LAL), Univ. Paris

[28] University of Oslo,Sud, CNRS/IN2P3

[29] International School for Advanced Studies (SISSA),Physics Department

[30] Kansei Gakuin University,Physics Division

[31] Kavli Institute for Cosmology Cambridge,Radio Astronomy Laboratory

[32] SLAC National Accelerator Laboratory,School of Physics and Astronomy

[33] The University of Tokyo,Space Sciences Laboratory

[34] Kitazato University,Division of Physics, Faculty of Pure and Applied Sciences

[35] Nagoya University,undefined

[36] Université Paris-Saclay,undefined

[37] Max-Planck-Institut for Astrophysics,undefined

[38] National Astronomical Observatory of Japan (NAOJ),undefined

[39] National Institute for Fusion Science (NIFS),undefined

[40] National Institute of Advanced Industrial Science and Technology (AIST),undefined

[41] National Institute of Information and Communications Technology (NICT),undefined

[42] National Institute of Standards and Technology (NIST),undefined

[43] Osaka Prefecture University,undefined

[44] Osaka University,undefined

[45] Oxford Astrophysics,undefined

[46] McGill University,undefined

[47] Lawrence Berkeley National Laboratory,undefined

[48] University of California,undefined

[49] RIKEN,undefined

[50] Saitama University,undefined

来源：

Journal of Low Temperature Physics | 2018年 / 193卷

关键词：

Cosmic microwave background radiation; Inflation; Satellite; Telescope;

D O I：

暂无

中图分类号：

学科分类号：

摘要：

The high-frequency telescope for LiteBIRD is designed with refractive and reflective optics. In order to improve sensitivity, this paper suggests the new optical configurations of the HFT which have approximately 7 times larger focal planes than that of the original design. The sensitivities of both the designs are compared, and the requirement of anti-reflection (AR) coating on the lens for the refractive option is derived. We also present the simulation result of a sub-wavelength AR structure on both surfaces of silicon, which shows a band-averaged reflection of 1.1–3.2% at 101–448 GHz.

引用

页码：841 / 850

页数：9

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