Jul 4 – 11, 2012
Melbourne Convention and Exhibition Centre
Australia/Melbourne timezone
ICHEP2012 - 36th International Conference for High Energy Physics

Cosmology and particle physics with POLARBEAR

Jul 7, 2012, 5:00 PM
15m
Room 216 (Melbourne Convention and Exhibition Centre)

Room 216

Melbourne Convention and Exhibition Centre

Melbourne Australia
Parallel Sessions Track 11. Particle Astrophysics and Cosmology Room 216 - Particle Astrophysics and Cosmology -TR11

Speaker

Dr Masaya Hasegawa (KEK (JP))

Description

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 presentation we will describe the current status and prospect of POLARBEAR.

Primary author

Prof. Adrian Lee (University of California, Berkeley)

Co-authors

Collaboration POLARBEAR (UC Berkeley, UCSD, KEK, McGill, Austin, Cardiff, Colorado, Dalhousie, Imperial C., LAC, LBNL, Tsukuba) Dr Masaya Hasegawa (KEK (JP))

Presentation materials