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The evolution of pore fluid pressure ( Pf$P_{\mathrm{f}}$) in the most seaward portion of a subduction accretionary prism plays an essential role in the cycle of tsunamigenic earthquakes. Based on recent geophysical observations, here we propose a testable conceptual model for this evolution for northern Cascadia offshore of Washington.
Tianhaozhe Sun, Kelin Wang
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Abstract The South Asian summer monsoon has exhibited a pronounced Northwest India‐Indo‐Gangetic Plains rainfall dipole since 1999, with northwest India experiencing a 24.6% increase, while rainfall in the Indo‐Gangetic Plain has decreased by 4.4%.
Nimmakanti Mahendra +5 more
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ABSTRACT Since 2000, archaeological excavations have brought to light the sanctuary of Athena in Castro (Apulia, Italy), including terracotta roofs dated between the 6th and 4th centuries bce. Based on their morphological and stylistic features, it is suggested that the terracotta items were manufactured in the Greek colony of Taras (modern Taranto ...
M. M. N. Franceschini +7 more
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Hierarchical mergers of stellar-mass black holes and their gravitational-wave signatures
Nature Astronomy, 2021While most of the compact-binary mergers detected by LIGO and Virgo are expected to consist of first-generation black holes formed from the collapse of stars, others might instead be of second (or higher) generation, containing the remnants of previous ...
D. Gerosa, M. Fishbach
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Concepts and status of Chinese space gravitational wave detection projects
Nature Astronomy, 2021Gravitational wave (GW) detection in space probes the GW spectrum that is inaccessible from the Earth. In addition to the LISA project led by the European Space Agency, and the DECIGO detector proposed by the Japan Aerospace Exploration Agency, two ...
Y. Gong, Jun Luo, Bin Wang
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Gravitational Waves and Gravitational-wave Sourcestwo
Chinese Astronomy and Astrophysics, 2018Abstract The recent discovery of gravitational-wave burst GW150914 marks the coming of a new era of gravitational-wave astronomy, which provides a new window to study the physics of strong gravitational field, extremely massive stars, extremely high energy processes, and extremely early universe.
Zhao Wen +21 more
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Physical Review, 1959
The field equations of the general theory of relativity are solved in the linear approximation for all cases of spherical waves with quadrupole symmetry. Energy is radiated outward by all these waves as determined by the canonical expression for the energy flux.
Boardman, John, Bergmann, Peter G.
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The field equations of the general theory of relativity are solved in the linear approximation for all cases of spherical waves with quadrupole symmetry. Energy is radiated outward by all these waves as determined by the canonical expression for the energy flux.
Boardman, John, Bergmann, Peter G.
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Squeezing the quantum noise of a gravitational-wave detector below the standard quantum limit
ScienceThe Heisenberg uncertainty principle dictates that the position and momentum of an object cannot be simultaneously measured with arbitrary precision, giving rise to an apparent limitation known as the standard quantum limit (SQL).
W. Jia +170 more
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Gravitational wave observatory
Applied Optics, 1990This brief report from NSF discusses the Foundation's hope to construct a gravitational wave observatory and provide a long-sought test for Einstein's theory of relativity.
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