Global EditionASIA 中文雙語Fran?ais
    China
    Home / China / Innovation

    With gravity waves, every second makes a difference

    By QUAN XIAOSHU | China Daily | Updated: 2018-03-28 09:10
    Share
    Share - WeChat

    When a gravitational wave reaches Earth, every second counts. So data processing speed is crucial when it comes to how much astronomers can learn from these space-time ripples.

    "In an era of multimessenger astronomy, we have to shorten the time as much as possible so as to trigger the alert quickly enough for follow-up observations," said computer scientist Cao Junwei, who leads the Chinese team collaborating at the international Laser Interferometer Gravitational-Wave Observatory (LIGO).

    In October, scientists from the LIGO Scientific Collaboration, together with astronomers around the world, declared they had detected a gravitational wave from the collision of binary neutron stars and corresponding electromagnetic signals-the first such direct observation ever made.

    The discovery was achieved through high data processing speed. Just 1.7 seconds after the wave detection network received the signal, a gamma ray burst was detected by the Fermi space telescope. LIGO and Fermi immediately triggered alerts around the astronomical community, bringing about 70 ground and space detectors into follow-up observations of electromagnetic signals at various wavelengths, which helped locate the source of the wave more precisely.

    Cao joined the LIGO Lab at the Massachusetts Institute of Technology as a computer scientist in 2004. On returning to China, he led a team from Tsinghua University's Research Institute of Information Technology in joining the LIGO collaboration in 2009.

    "We were the only Chinese group in the collaboration. None of us specialized in astrophysics, but we were accepted," said Cao, who is vice-dean of the institute at Tsinghua.

    In the first five years, the Chinese team mainly helped build the computing platform and analyzed data. Then they began devoting most of their efforts to speeding up data processing.

    The faster, the better

    Few understood the importance of speed at the beginning.

    "We suggested, from the outset, that fast computing would serve multimessenger astronomy, which requires follow-up observations as soon as a gravitational wave signal is confirmed," Cao said. "The faster, the better."

    In 2015, LIGO first detected gravitational waves from the collision of binary black holes, which verified the general relativity theory that Albert Einstein proposed a century ago. But it took scientists months to vet, validate and interpret the discovery before it was publicly announced.

    LIGO detectors collect more than 16,000 data samples per second. To confirm that a signal is generated by gravitational waves, scientists remove "noise" from the data, and then compare the data patterns with templates of gravitational waves.

    More than 1,000 scientists are working in the LIGO Scientific Collaboration, more than half of them on data analysis. The data quality categories are defined by multiple analysis groups: compact binary coalescence, burst, continuous waves, stochastic and others.

    "Our team, which is only a small group in the collaboration, is now focusing on graphics processing unit acceleration for searches and exploring the application of machine learning to real-time data analysis," Cao says.

    Their accomplishments include a set of new data processing pipelines, in cooperation with the University of Western Australia.

    "The new pipelines help speed up data filtering, so we can finish comparing data patterns with tens of thousands of templates within a second," Tsinghua Associate Professor Du Zhihui said.

    "Now, the time between the arrival of a signal and the confirmation of it as gravitational waves has been shortened from several minutes to dozens of seconds. Next, we hope to shrink the time to three to five seconds," Du said.

    Scientists began to enhance LIGO's detectors in 2008. The Advanced LIGO finished its second run in August 2017, and is expected to start its third run in the middle of this year. Scientists will further upgrade its detectors between the two runs to improve its sensitivity, which should greatly increase the odds of discovering gravitational waves.

    "With a higher sensitivity, the number of signals that are detected may soar from a few a year to several a day. We will fall far behind if we don't accelerate data processing," Cao said.

    He hopes the Chinese work at LIGO will contribute to the country's own gravitational wave detection projects.

    "China will participate in international cooperation actively to foster talent and accumulate experience," he said.

    Top
    BACK TO THE TOP
    English
    Copyright 1995 - . All rights reserved. The content (including but not limited to text, photo, multimedia information, etc) published in this site belongs to China Daily Information Co (CDIC). Without written authorization from CDIC, such content shall not be republished or used in any form. Note: Browsers with 1024*768 or higher resolution are suggested for this site.
    License for publishing multimedia online 0108263

    Registration Number: 130349
    FOLLOW US
     
    少妇人妻无码精品视频app| 无码人妻精品中文字幕| 公和熄小婷乱中文字幕| 亚洲精品无码不卡| A级毛片无码久久精品免费| 色综合中文字幕| 少妇人妻综合久久中文字幕| 无码精品一区二区三区免费视频| 人妻少妇看A偷人无码电影| 无码人妻黑人中文字幕| 人妻少妇无码视频在线| 台湾无码一区二区| 亚洲级αV无码毛片久久精品| 国产中文字幕乱人伦在线观看 | 中文字幕av无码专区第一页| 国产在线精品一区二区中文| 免费AV一区二区三区无码| 青青草无码免费一二三区| 亚洲AV无码欧洲AV无码网站| 国产成人无码一区二区三区在线| 精选观看中文字幕高清无码| 中文字幕av无码专区第一页| 亚洲成a人在线看天堂无码| 黑人无码精品又粗又大又长 | 久久中文字幕精品| 亚洲av无码专区在线观看下载| 99无码熟妇丰满人妻啪啪| 久久久久久国产精品无码超碰 | 国产成A人亚洲精V品无码性色 | 午夜精品久久久久久久无码| V一区无码内射国产| 毛片一区二区三区无码| 97精品人妻系列无码人妻| 久久国产亚洲精品无码| 99精品一区二区三区无码吞精| 欧洲Av无码放荡人妇网站| 97碰碰碰人妻视频无码| 亚洲色偷拍区另类无码专区| 制服丝袜人妻中文字幕在线| 亚洲中文字幕无码久久精品1| 国产乱码精品一区二区三区中文 |