_unraveling-the-tiny-wrinkles-in-cosmic-microwave-background-radiation-j-s-bagla-harish-chandra-research-institute.jpg "Unraveling the tiny wrinkles in Cosmic Microwave Background Radiation - J. S. Bagla Harish, Chandra Research Institute from bagla à ¦›à §‡à ¦²à §‡ Video Screenshot Preview")
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⏲ Duration: 13 min 37 sec
✓ Published: 28-Oct-2011
✓ Published: 28-Oct-2011
Description:
Unraveling the tiny wrinkles in Cosmic Microwave Background Radiation: Determining the past and future evolution of the Universe nnJ. S. Bagla Harish, Chandra Research Institute nnThe cosmic microwave background radiation, or CMBR as it is often referred to is radiation received from all directions of the sky, with the characteristic spectrum corresponding to 2.7 degrees Kelvin. CMBR was discovered by Penzias and Wilson in 1965, and the cosmological interpretation was arrived at in the same year
Unraveling the tiny wrinkles in Cosmic Microwave Background Radiation: Determining the past and future evolution of the Universe nnJ. S. Bagla Harish, Chandra Research Institute nnThe cosmic microwave background radiation, or CMBR as it is often referred to is radiation received from all directions of the sky, with the characteristic spectrum corresponding to 2.7 degrees Kelvin. CMBR was discovered by Penzias and Wilson in 1965, and the cosmological interpretation was arrived at in the same year
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