Imperial College London
Alternate

Professor Andrew H Jaffe

Faculty of Natural Sciences, Department of Physics

Professor of Astrophysics and Cosmology
 
 
 
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Contact

 

+44 (0)20 7594 7526a.jaffe Website

 
 
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Assistant

 

Miss Louise Hayward +44 (0)20 7594 7679

 
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Location

 

1018BBlackett LaboratorySouth Kensington Campus

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Summary

 

Publications

Citation

BibTex format

@inproceedings{Hasegawa:2012,
author = {Hasegawa, M and Ade, PAR and Anthony, AE and Arnold, K and Barron, D and Boettger, D and Borrill, J and Chapman, S and Chinone, Y and Dobbs, MA and Errard, J and Fabbian, G and Flanigan, D and Fuller, G and Ghribi, A and Grainger, W and Halverson, N and Hattori, K and Hazumi, M and Holzapfel, WL and Howard, J and Hyland, P and Jaffe, A and Keating, B and Kermish, Z and Kisner, T and Le, Jeune M and Lee, AT and Linder, E and Lungu, M and Matsuda, F and Matsumura, T and Miller, NJ and Meng, X and Morii, H and Moyerman, S and Myers, MJ and Nishino, H and Paar, H and Quealy, E and Reichardt, C and Richards, PL and Ross, C and Shimizu, A and Chimmin, C and Shimon, M and Sholl, M and Siritanasak, P and Spieler, H and Stebor, N and Steinbach, B and Stompor, R and Suzuki, A and Tomaru, T and Tucker, C and Zahn, O},
title = {Cosmology and particle physics with POLARBEAR},
year = {2012}
}
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RIS format (EndNote, RefMan)

TY  - CPAPER
AB  - Cosmic inflation predicts that primordial gravitational waves were created during the inflationary era. Measurements of polarization of the Cosmic Microwave Background (CMB) radiation are known as the best probe to detect the primordial gravitational waves. POLARBEAR is a telescope designed to detect the CMB B-mode with very sensitive polarimeters based on superconductive transition edge sensor (TES) detector technology. Its large primary mirror with a diameter of 3.5m also allows us to constrain or measure the sum of neutrino masses beyond the limit obtained so far. POLARBEAR is located on the Chajnantor plateau in the Atacama desert in northern Chile at an altitude of 5,200m. We received the first light in January 2012 and are taking CMB data at 150 GHz. In this paper we will describe the current status and prospect of POLARBEAR.
AU  - Hasegawa,M
AU  - Ade,PAR
AU  - Anthony,AE
AU  - Arnold,K
AU  - Barron,D
AU  - Boettger,D
AU  - Borrill,J
AU  - Chapman,S
AU  - Chinone,Y
AU  - Dobbs,MA
AU  - Errard,J
AU  - Fabbian,G
AU  - Flanigan,D
AU  - Fuller,G
AU  - Ghribi,A
AU  - Grainger,W
AU  - Halverson,N
AU  - Hattori,K
AU  - Hazumi,M
AU  - Holzapfel,WL
AU  - Howard,J
AU  - Hyland,P
AU  - Jaffe,A
AU  - Keating,B
AU  - Kermish,Z
AU  - Kisner,T
AU  - Le,Jeune M
AU  - Lee,AT
AU  - Linder,E
AU  - Lungu,M
AU  - Matsuda,F
AU  - Matsumura,T
AU  - Miller,NJ
AU  - Meng,X
AU  - Morii,H
AU  - Moyerman,S
AU  - Myers,MJ
AU  - Nishino,H
AU  - Paar,H
AU  - Quealy,E
AU  - Reichardt,C
AU  - Richards,PL
AU  - Ross,C
AU  - Shimizu,A
AU  - Chimmin,C
AU  - Shimon,M
AU  - Sholl,M
AU  - Siritanasak,P
AU  - Spieler,H
AU  - Stebor,N
AU  - Steinbach,B
AU  - Stompor,R
AU  - Suzuki,A
AU  - Tomaru,T
AU  - Tucker,C
AU  - Zahn,O
PY  - 2012///
TI  - Cosmology and particle physics with POLARBEAR
ER  -
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