Detecting the cosmic gravitational wave background with the Big Bang Observer
Vincent Corbin,Neil J. Cornish +1 more
TLDR
In this paper, the authors considered the cross-correlation of two Michelson channels by calculating the optimal signal-to-noise ratio that can be achieved by combining the full set of interferometry variables that are available with a six link triangular interferometer.Abstract:
The detection of the cosmic microwave background radiation (CMB) was one of the most important cosmological discoveries of the last century. With the development of interferometric gravitational wave detectors, we may be in a position to detect the gravitational equivalent of the CMB in this century. The cosmic gravitational background (CGB) is likely to be isotropic and stochastic, making it difficult to distinguish from instrument noise. The contribution from the CGB can be isolated by cross-correlating the signals from two or more independent detectors. Here we extend previous studies that considered the cross-correlation of two Michelson channels by calculating the optimal signal-to-noise ratio that can be achieved by combining the full set of interferometry variables that are available with a six link triangular interferometer. In contrast to the two channel case, we find that the relative orientation of a pair of coplanar detectors does not affect the signal-to-noise ratio. We apply our results to the detector design described in the Big Bang Observer (BBO) mission concept study and find that the BBO could detect a background with Ωgw > 2.2 × 10−17.read more
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Gravitational wave production by collisions: more bubbles
TL;DR: In this paper, the authors re-examine the production of gravitational waves by bubble collisions during a first-order phase transition and find that the spectrum rises as f3.0 for small frequencies and decreases as f−1.5 for high frequencies.
Journal ArticleDOI
Science with the space-based interferometer LISA. IV: probing inflation with gravitational waves
Nicola Bartolo,Chiara Caprini,Valerie Domcke,Daniel G. Figueroa,Juan Garcia-Bellido,Maria Chiara Guzzetti,Michele Liguori,Sabino Matarrese,Marco Peloso,Antoine Petiteau,Angelo Ricciardone,Mairi Sakellariadou,Lorenzo Sorbo,Gianmassimo Tasinato +13 more
TL;DR: In this paper, the LISA space-based interferometer was used to detect the stochastic gravitational wave background produced from different mechanisms during inflation, focusing on well-motivated scenarios.
Journal ArticleDOI
Gravitational Waves Induced by Non-Gaussian Scalar Perturbations
Rong-Gen Cai,Shi Pi,Misao Sasaki +2 more
TL;DR: In this article, the power spectrum of the curvature perturbation has a narrow peak at some small scale, with a local-type non-Gaussianity, and the density parameter per logarithmic frequency interval is calculated.
Journal ArticleDOI
Gravitational wave background from reheating after hybrid inflation
TL;DR: In this paper, the authors show that the fraction of energy density today in these primordial gravitational waves could be significant for grand unified theory (GUT)-scale models of inflation, although well beyond the frequency range sensitivity of gravitational wave observatories like LIGO, LISA, or BBO.
Journal ArticleDOI
Probing the early universe with inflationary gravitational waves
Latham Boyle,Paul J. Steinhardt +1 more
TL;DR: In this paper, a new GWB transfer function was derived that incorporates a number of physical effects that were treated less accurately, less generally, or were missing altogether in previous treatments.
References
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Detecting a stochastic background of gravitational radiation: Signal processing strategies and sensitivities
TL;DR: In this paper, the authors derived expressions for the optimal filter function and signal-to-noise ratio for the cross-correlation of the outputs of two gravity-wave detectors, and the sensitivity levels required for detection are then calculated.
Journal ArticleDOI
Beyond LISA: Exploring future gravitational wave missions
Jeff Crowder,Neil J. Cornish +1 more
TL;DR: In this paper, the authors compared the capabilities of the Advanced Laser Interferometer Antenna in Stereo (ALIAS) and the Big Bang Observer (BBO) and found that the initial deployment phase of the BBO would be sufficient to detect the Gravitational Wave Background, while still providing detailed information about foreground sources.
Journal ArticleDOI
Angular resolution of the LISA gravitational wave detector
TL;DR: In this article, the angular resolution of the planned LISA detector, a space-based laser interferometer for measuring low-frequency gravitational waves from galactic and extragalactic sources, was calculated.
Journal ArticleDOI
Sensitivity of the laser interferometer gravitational wave observatory to a stochastic background, and its dependence on the detector orientations
TL;DR: The broadband sensitivity of a network of interferometer gravitational-wave detectors to the stochastic background of a detector pair which are far apart is essentially determined by their relative rotation, and the optimal configuration is for each detector to have its arms make an angle with the arc of the great circle that joins them.
Journal ArticleDOI
Direct detection of the inflationary gravitational-wave background
TL;DR: In this article, a range of slow-roll inflationary models consistent with constraints from the CMB and large-scale structure (LSS) are surveyed. But the authors focus on the detectability of the inflationary gravitational-wave background at BBO/DECIGO frequencies.
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Vajente,G. Valdes,Michele Vallisneri,N. van Bakel,M. van Beuzekom,J. F. J. van den Brand,C. Van Den Broeck,D. C. Vander-Hyde,L. van der Schaaf,J. V. van Heijningen,A. A. van Veggel,M. Vardaro,S. Vass,M. Vasúth,Ruslan Vaulin,Alberto Vecchio,G. Vedovato,John Veitch,P. J. Veitch,K. Venkateswara,D. Verkindt,F. Vetrano,A. Viceré,Serena Vinciguerra,D. J. Vine,J-Y. Vinet,Salvatore Vitale,T. Vo,H. Vocca,C. Vorvick,D. V. Voss,W. D. Vousden,Sergey P. Vyatchanin,A. R. Wade,L. E. Wade,Madeline Wade,S. J. Waldman,Michelle E. Walker,L. Wallace,S. Walsh,G. Wang,Hua Wang,Meng Wang,X. F. Wang,Yanzhi Wang,H. Ward,R. L. Ward,J. Warner,M. Was,B. A. Weaver,L.-W. Wei,L.-W. Wei,M. Weinert,A. J. Weinstein,Rainer Weiss,Timothy A Welborn,Linqing Wen,Peter Weßels,T. Westphal,K. Wette,James Whelan,S. E. Whitcomb,D. J. White,Bernard F. Whiting,K. Wiesner,C. Wilkinson,Phil Willems,L. Williams,Roy Williams,A. R. Williamson,Joshua L. Willis,Benno Willke,M. H. Wimmer,Lutz Winkelmann,Walter Winkler,C. C. Wipf,A. G. Wiseman,H. Wittel,Graham Woan,John Worden,J. L. Wright,G. Wu,Joshua Yablon,I. Yakushin,William Yam,H. Yamamoto,C. C. Yancey,M. J. Yap,Haocun Yu,M. Yvert,A. K. Zadrożny,L. Zangrando,Michele Zanolin,J. P. Zendri,M. Zevin,Fan Zhang,Lei Zhang,Mi Zhang,Y.-H. Zhang,C. Zhao,Minchuan Zhou,Zifan Zhou,Xing-Jiang Zhu,Michael E Zucker,S. E. Zuraw,J. Zweizig +1011 more