he current status of the quest for ultra-low frequency Gravitational Waves and the roadmap for future technical and scientific challenges is to be the main focus of the meeting.
“These waves are wrinkles in space-time produced by two massive black holes, each revolving around the other. Such black holes, which weigh billion times more than our Sun, are found in the centres of colliding galaxies. These waves affect radio pulses from 10km size stars called radio pulsars by changing ever so slightly the period of radio pulsation of these stars
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Unknown title this status by the conclusion of the upcoming meeting. We are expecting eighty international members apart from the twenty persons who will be representing our country,” informed Dr. Solanki. T<span>he current status of the quest for ultra-low frequency Gravitational Waves and the roadmap for future technical and scientific challenges is to be the main focus of the meeting. “These waves are wrinkles in space-time produced by two massive black holes, each revolving around the other. Such black holes, which weigh billion times more than our Sun, are found in the centres of colliding galaxies. These waves affect radio pulses from 10km size stars called radio pulsars by changing ever so slightly the period of radio pulsation of these stars,” said Prof. Yashwant Gupta, centre director, NCRA. He said that measuring these periods to a precision of 10 seconds of a nano-second may help the IPTA experiment to discover Gravitati Summary
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