Probing primordial gravitational waves: Ali CMB Polarization Telescope

Author:

Li Hong1,Li Si-Yu1,Liu Yang23,Li Yong-Ping23,Cai Yifu4,Li Mingzhe5,Zhao Gong-Bo67,Liu Cong-Zhan1,Li Zheng-Wei1,Xu He1,Wu Di1,Zhang Yong-Jie1,Fan Zu-Hui8,Yao Yong-Qiang6,Kuo Chao-Lin9,Lu Fang-Jun1,Zhang Xinmin23

Affiliation:

1. Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China

2. Theoretical Physics Division, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China

3. University of Chinese Academy of Sciences, Beijing 100049, China

4. CAS Key Laboratory for Researches in Galaxies and Cosmology, Department of Astronomy, University of Science and Technology of China, Hefei 230026, China

5. Interdisciplinary Center for Theoretical Study, University of Science and Technology of China, Hefei 230026, China

6. National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China

7. Institute of Cosmology & Gravitation, University of Portsmouth, Portsmouth PO1 3FX, UK

8. Department of Astronomy, School of Physics, Peking University, Beijing 100871, China

9. Physics Department, Stanford University, Stanford, CA 94305, USA

Abstract

Abstract In this paper, we will give a general introduction to the Ali CMB Polarization Telescope (AliCPT) project, which is a Sino–US joint project led by the Institute of High Energy Physics and involves many different institutes in China. It is the first ground-based Cosmic Microwave Background (CMB) polarization experiment in China and an integral part of China's Gravitational-wave Program. The main scientific goal of the AliCPT project is to probe the primordial gravitational waves (PGWs) originating from the very early Universe. The AliCPT project includes two stages. The first stage, referred to as AliCPT-1, is to build a telescope in the Ali region of Tibet at an altitude of 5250 meters. Once completed, it will be the highest ground-based CMB observatory in the world and will open a new window for probing PGWs in the northern hemisphere. The AliCPT-1 telescope is designed to have about 7000 transition-edge sensor detectors at 95 GHz and 150 GHz. The second stage is to have a more sensitive telescope (AliCPT-2) with more than 20 000 detectors. Our simulations show that AliCPT will improve the current constraint on the tensor-to-scalar ratio r by one order of magnitude with three years' observation. Besides the PGWs, AliCPT will also enable a precise measurement of the CMB rotation angle and provide a precise test of the CPT symmetry. We show that three years' observation will improve the current limit by two orders of magnitude.

Funder

National Natural Science Foundation of China

CAS pilot B project

Sino–US cooperation project

Publisher

Oxford University Press (OUP)

Subject

Multidisciplinary

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