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Probing Primordial Gravitational Waves: Ali CMB Polarization Telescope

Cosmology and Nongalactic Astrophysics 2018-02-27 v2 Instrumentation and Methods for Astrophysics General Relativity and Quantum Cosmology High Energy Physics - Experiment High Energy Physics - Phenomenology

Abstract

In this paper, we will give a general introduction to the project of Ali CMB Polarization Telescope (AliCPT), which is a Sino-US joint project led by the Institute of High Energy Physics (IHEP) and has involved 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 Waves Program. The main scientific goal of AliCPT project is to probe the primordial gravitational waves (PGWs) originated 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 with an altitude of 5,250 meters. Once completed, it will be the worldwide highest ground-based CMB observatory and open a new window for probing PGWs in northern hemisphere. AliCPT-1 telescope is designed to have about 7,000 TES detectors at 90GHz and 150GHz. The second stage is to have a more sensitive telescope (AliCPT-2) with the number of detectors more than 20,000. Our simulations show that AliCPT will improve the current constraint on the tensor-to-scalar ratio rr by one order of magnitude with 3 years' observation. Besides the PGWs, the AliCPT will also enable a precise measurement on the CMB rotation angle and provide a precise test on the CPT symmetry. We show 3 years' observation will improve the current limit by two order of magnitude.

Keywords

Cite

@article{arxiv.1710.03047,
  title  = {Probing Primordial Gravitational Waves: Ali CMB Polarization Telescope},
  author = {Hong Li and Si-Yu Li and Yang Liu and Yong-Ping Li and Yifu Cai and Mingzhe Li and Gong-Bo Zhao and Cong-Zhan Liu and Zheng-Wei Li and He Xu and Di Wu and Yong-Jie Zhang and Zu-Hui Fan and Yong-Qiang Yao and Chao-Lin Kuo and Fang-Jun Lu and Xinmin Zhang},
  journal= {arXiv preprint arXiv:1710.03047},
  year   = {2018}
}

Comments

11 pages, 7 figures, 2 tables