scholarly journals Cross-correlation search for continuous gravitational waves from a compact object in SNR 1987A in LIGO Science run 5

2016 ◽  
Vol 94 (8) ◽  
Author(s):  
L. Sun ◽  
A. Melatos ◽  
P. D. Lasky ◽  
C. T. Y. Chung ◽  
N. S. Darman
2011 ◽  
Vol 84 (8) ◽  
Author(s):  
Sanjeev Dhurandhar ◽  
Hideyuki Tagoshi ◽  
Yuta Okada ◽  
Nobuyuki Kanda ◽  
Hirotaka Takahashi

2017 ◽  
Vol 847 (1) ◽  
pp. 47 ◽  
Author(s):  
B. P. Abbott ◽  
R. Abbott ◽  
T. D. Abbott ◽  
F. Acernese ◽  
K. Ackley ◽  
...  

2008 ◽  
Vol 77 (8) ◽  
Author(s):  
Sanjeev Dhurandhar ◽  
Badri Krishnan ◽  
Himan Mukhopadhyay ◽  
John T. Whelan

2012 ◽  
Vol 363 ◽  
pp. 012040
Author(s):  
Yuta Okada ◽  
Nobuyuki Kanda ◽  
Sanjeev Dhurandhar ◽  
Hideyuki Tagoshi ◽  
Hirotaka Takahashi

2015 ◽  
Vol 91 (10) ◽  
Author(s):  
John T. Whelan ◽  
Santosh Sundaresan ◽  
Yuanhao Zhang ◽  
Prabath Peiris

2013 ◽  
Vol 28 (35) ◽  
pp. 1350161 ◽  
Author(s):  
SUNANDAN GANGOPADHYAY ◽  
ANIRBAN SAHA ◽  
SWARUP SAHA

Interaction of linearized gravitational waves with a otherwise free particle has been studied quantum mechanically in a noncommutative (NC) phase-space to examine whether the particle's response to the gravitational wave gets modified due to spatial and/or momentum noncommutativity. The result shows that momentum noncommutativity introduces a oscillatory noise with a specific frequency determined by the fundamental momentum scale and particle mass. Because of the global nature of the phase-space noncommutativity such noise will have similar characteristics for all detector sites and thus will stand out in a data cross-correlation procedure. If detected, this noise will provide evidence of momentum noncommutativity and also an estimation of the relevant noncommutative parameter.


2018 ◽  
Vol 97 (4) ◽  
Author(s):  
Grant David Meadors ◽  
Badri Krishnan ◽  
Maria Alessandra Papa ◽  
John T. Whelan ◽  
Yuanhao Zhang

2020 ◽  
Vol 35 (31) ◽  
pp. 2050205
Author(s):  
Aung Naing Win ◽  
Yu-Ming Chu ◽  
Hasrat Hussain Shah ◽  
Syed Zaheer Abbas ◽  
Munawar Shah

A Satellite Fermi GBM detected recent putative short Gamma Ray Bursts (GRBs) in coincident with the gravitational wave signal GW 150914 produced by the merger of binary black hole (BH). If at least one BH possess magnetic monopole charge in the binary BH system then the short-duration GRBs may produce during the final phase of a binary BH merger. The detection of gravitational waves GW 150914, GW 151226 and LVT 151012 by LIGO gave the evidence that merging of the compact object like binary BH often happens in our universe. In this paper, we report the qualitative model to discuss the generation of electromagnetic radiation from the merging of two BHs with equal masses and at least one BH carrying the magnetic monopole charge in the binary system. In this model, BH possess a magnetic monopole charge that may not be neutralized before the coalescence. During the inspiralling process, the magnetic monopole charge on the BH would produced the electric dipole moment. Short duration GRB would produce by the rapidly evolution of the electric dipole moment which may detectable on Earth. We predict that this model would be beneficial in the future to explain the generation of gravitational wave (GW) plus a electromagnetic signal of multi-wavelength from mergers of magnetically charged BHs.


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