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INDIAN INSTITUTE OF SCIENCE EDUCATION AND RESEARCH (IISER) PUNE
where tomorrow’s science begins today
An Autonomous Institution, Ministry of Human Resource Development, Govt. of India
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Seminars and Colloquia

Physics

Viewing the beginning of time from the most remote places on Earth 
 
Mon, Jan 28, 2019,   06:30 PM at C.V. Raman Auditorium, LHC

Dr. Zeeshan Ahmed
Kavli Institute for Particle Astrophysics and Cosmology and SLAC National Accelerator Laboratory.

 

Abstract: Shortly after the birth of the universe, space was filled by a plasma that was literally red-hot. The light radiated by that plasma has traveled the vast emptiness of space for billions of years, with the

expansion of the universe slowly stretching its waves until today it appears as microwave radiation.  This is the Cosmic Microwave Background (CMB), a glow still visible in the sky. This glow is almost uniform, but small variations from point to point hold information about the conditions of the universe 13.8 billion years ago. This lecture will introduce the CMB, present the sophisticated cameras we build to observe it, and describe the remote outposts of our planet, including the geographic South Pole, where we deploy these cameras to image the CMB.  As we image the CMB in finer and finer detail, in particular its polarization, we hope to improve our understanding of the beginning of the universe and perhaps of time itself.

Brief intro:

Zeeshan Ahmed is an observational cosmologist at the Kavli Institute for Particle Astrophysics and Cosmology and SLAC National Accelerator Laboratory. He received his PhD from Caltech in 2012 and held a postdoctoral position at Stanford University before being appointed a Panofsky Fellow at SLAC
in 2015. Ahmed is a member of several scientific teams imaging the Cosmic Microwave Background (CMB) from the South Pole and the Atacama Desert in Chile. He spends his time understanding data from these cameras and devising tricks to build more powerful CMB cameras.
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Abstract: Shortly after the birth of the universe, space was filled by a plasma that was literally red-hot. The light radiated by that plasma has traveled the vast emptiness of space for billions of years, with the

expansion of the universe slowly stretching its waves until today it appears as microwave radiation.  This is the Cosmic Microwave Background (CMB), a glow still visible in the sky. This glow is almost uniform, but small variations from point to point hold information about the conditions of the universe 13.8 billion years ago. This lecture will introduce the CMB, present the sophisticated cameras we build to observe it, and describe the remote outposts of our planet, including the geographic South Pole, where we deploy these cameras to image the CMB.  As we image the CMB in finer and finer detail, in particular its polarization, we hope to improve our understanding of the beginning of the universe and perhaps of time itself.

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