AIP Conference Proceedings 2009
DOI: 10.1063/1.3115564
|View full text |Cite
|
Sign up to set email alerts
|

The Peoples Republic of China High-Frequency Gravitational Wave Research Program

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1

Citation Types

0
3
0

Year Published

2017
2017
2023
2023

Publication Types

Select...
2
2
1

Relationship

0
5

Authors

Journals

citations
Cited by 5 publications
(3 citation statements)
references
References 10 publications
0
3
0
Order By: Relevance
“…It is 12 orders of magnitude smaller than the strain sensibility of LIGO's interferometer, which can probe amplitudes up to ∼ 10 −22 in the frequency range from 10 Hz to 10 kHz. Although it seems hopeless to reach such small distances, the Chongqing University detector (currently under development) will be able to probe amplitudes as small as 10 −32 [Baker, 2009] in the high-frequency range 0.1-10 GHz, which is not far from the bound just found. Observe, however, that we have found an upper bound on and not a lower one, thus could be arbitrarily small and not be detectable by the Chongqing detector.…”
Section: Gravitational Wave Backreactionmentioning
confidence: 96%
“…It is 12 orders of magnitude smaller than the strain sensibility of LIGO's interferometer, which can probe amplitudes up to ∼ 10 −22 in the frequency range from 10 Hz to 10 kHz. Although it seems hopeless to reach such small distances, the Chongqing University detector (currently under development) will be able to probe amplitudes as small as 10 −32 [Baker, 2009] in the high-frequency range 0.1-10 GHz, which is not far from the bound just found. Observe, however, that we have found an upper bound on and not a lower one, thus could be arbitrarily small and not be detectable by the Chongqing detector.…”
Section: Gravitational Wave Backreactionmentioning
confidence: 96%
“…It is 12 orders of magnitude smaller than the strain sensibility of LIGO's interferometer, which can probe amplitudes up to ∼ 10 −22 in the frequency range from 10 Hz to 10 kHz. Although it seems hopeless to reach such small distances, the Chongqing University detector (currently under development) will be able to probe amplitudes as small as 10 −32 [22] in the high-frequency range 0.1-10 GHz, which is not far from the bound just found. Observe, however, that we have found an upper bound on and not a lower one, thus could be arbitrarily small and not be detectable by the Chongqing detector.…”
Section: Gravitational Wave Backreactionmentioning
confidence: 96%
“…At the very beginning fraction of a second, there was an infinite force of infinite Shrunk space, we speculate that the infinite force of Shrunk space gave rise to the Big Bang, and caused the rapid growth of space. That process would appear to move very rapidly in the early universe, and was only readily observable by detectors of high-frequency gravitational waves such as the Li-Baker [14][15][16]. After the beginning of the universe, the Shrunk space continues to expand, but in the distant past, the pressure of the shrunk space, and density should have been greater, so the universe must have been expanding more slowly than it is today.…”
Section: Accelerated Expansion Of the Universementioning
confidence: 99%