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Thesis

Development of new generation receivers for experimental cosmology with the cosmic microwave background and systematic effect studies

Abstract:

Most of current and future Cosmic Microwave Background (CMB) Radiation experiments are targeting the polarized B-mode signal. The small amplitude of this signal makes a successful measurement challenging for current technologies. Therefore, very accurate studies to mitigate and control possible systematic effects are vital to achieve a successful observation. An additional challenge is coming from the presence of polarized Galactic foreground signals that contaminate the cosmological signa...

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Institution:
University of Oxford
Division:
MPLS
Department:
Physics
Sub department:
Astrophysics
Oxford college:
Exeter College
Role:
Author
ORCID:
https://orcid.org/0000-0003-4175-7010

Contributors

Institution:
High Energy Accelerator Research Organization (KEK)
Role:
Supervisor
Institution:
Kavli IPMU - The University of Tokyo
Role:
Supervisor
Institution:
University of Oxford
Role:
Supervisor
Institution:
University of Oxford
Role:
Supervisor
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Name:
Kavli IPMU
Programme:
Kavli/IPMU PhD Studentship
Type of award:
DPhil
Level of award:
Doctoral
Awarding institution:
University of Oxford
Language:
English
Deposit date:
2020-11-26

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