scholarly journals Model-based cross-correlation search for gravitational waves from Scorpius X-1

2015 ◽  
Vol 91 (10) ◽  
Author(s):  
John T. Whelan ◽  
Santosh Sundaresan ◽  
Yuanhao Zhang ◽  
Prabath Peiris
2017 ◽  
Vol 847 (1) ◽  
pp. 47 ◽  
Author(s):  
B. P. Abbott ◽  
R. Abbott ◽  
T. D. Abbott ◽  
F. Acernese ◽  
K. Ackley ◽  
...  

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

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

2016 ◽  
Vol 25 (11) ◽  
pp. 1640013 ◽  
Author(s):  
Stephon Alexander

A decade ago, the first leptogenesis model based on inflation was proposed, where the complex phase of the inflaton field carries lepton number [S. H. S. Alexander, M. E. Peskin and M. M. Sheikh-Jabbari, Phys. Rev. Lett. 96 (2006) 081301, arXiv:hep-th/0403069 ]. If the inflaton field is an axion, it can couple to gravitational waves and gauge fields via Chern–Simons invariants. Due to these couplings, birefringent gravitational and gauge primordial perturbations are created during inflation to generate a lepton asymmetry, establishing a possible connection between nonvanishing TB-parity-violating polarization cross-correlations and leptogenesis. We also discuss the prospect for a subset of these models which can directly source circular (V-mode) polarization in the CMB.


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

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