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BibliografiaTesi.bib
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@article{Rezzolla_2016,
title={Gravitational-wave signal from binary neutron stars: A systematic analysis of the spectral properties},
volume={93},
ISSN={2470-0029},
url={http://dx.doi.org/10.1103/PhysRevD.93.124051},
DOI={10.1103/physrevd.93.124051},
number={12},
journal={Physical Review D},
publisher={American Physical Society (APS)},
author={Rezzolla, Luciano and Takami, Kentaro},
year={2016},
month={Jun}
}
@article{Abbott_2017a,
title={GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral},
volume={119},
ISSN={1079-7114},
url={http://dx.doi.org/10.1103/PhysRevLett.119.161101},
DOI={10.1103/physrevlett.119.161101},
number={16},
journal={Physical Review Letters},
publisher={American Physical Society (APS)},
author={Abbott, B. P. and Abbott, R. and Abbott, T. D. and Acernese, F. and Ackley, K. and Adams, C. and Adams, T. and Addesso, P. and Adhikari, R. X. and Adya, V. B. and et al.},
year={2017},
month={Oct}
}
@article{Klimenko_2008,
title={A coherent method for detection of gravitational wave bursts},
volume={25},
ISSN={1361-6382},
url={http://dx.doi.org/10.1088/0264-9381/25/11/114029},
DOI={10.1088/0264-9381/25/11/114029},
number={11},
journal={Classical and Quantum Gravity},
publisher={IOP Publishing},
author={Klimenko, S and Yakushin, I and Mercer, A and Mitselmakher, G},
year={2008},
month={May},
pages={114029}
}
@article{Abbott_2017b,
title={Search for Post-merger Gravitational Waves from the Remnant of the Binary Neutron Star Merger GW170817},
volume={851},
ISSN={2041-8213},
url={http://dx.doi.org/10.3847/2041-8213/aa9a35},
DOI={10.3847/2041-8213/aa9a35},
number={1},
journal={The Astrophysical Journal},
publisher={American Astronomical Society},
author={Abbott, B. P. and Abbott, R. and Abbott, T. D. and Acernese, F. and Ackley, K. and Adams, C. and Adams, T. and Addesso, P. and Adhikari, R. X. and Adya, V. B. and et al.},
year={2017},
month={Dec},
pages={L16}
}
@article{Klimenko_2016,
title={Method for detection and reconstruction of gravitational wave transients with networks of advanced detectors},
volume={93},
ISSN={2470-0029},
url={http://dx.doi.org/10.1103/PhysRevD.93.042004},
DOI={10.1103/physrevd.93.042004},
number={4},
journal={Physical Review D},
publisher={American Physical Society (APS)},
author={Klimenko, S. and Vedovato, G. and Drago, M. and Salemi, F. and Tiwari, V. and Prodi, G. A. and Lazzaro, C. and Ackley, K. and Tiwari, S. and Da Silva, C. F. and et al.},
year={2016},
month={Feb}
}
@book{hartle2003gravity,
title={Gravity: An Introduction to Einstein's General Relativity},
author={Hartle, J.B.},
isbn={9780805386622},
lccn={2002151118},
url={https://books.google.it/books?id=ZHgpAQAAMAAJ},
year={2003},
publisher={Addison-Wesley}
}
@book{held2013applied,
title={Applied Statistical Inference: Likelihood and Bayes},
author={Held, L. and Bove, D.S.},
isbn={9783642378881},
url={https://books.google.it/books?id=\_VH8sgEACAAJ},
year={2013},
publisher={Springer}
}
@book{hobson2006general,
title={General Relativity: An Introduction for Physicists},
author={Hobson, M.P. and Efstathiou, G.P. and Lasenby, A.N.},
isbn={9781139447546},
url={https://books.google.it/books?id=xma1QuTJphYC},
year={2006},
publisher={Cambridge University Press}
}
@misc{sarin2020evolution,
title={The evolution of binary neutron star post-merger remnants: a review},
author={Nikhil Sarin and Paul D. Lasky},
year={2020},
eprint={2012.08172},
archivePrefix={arXiv},
primaryClass={astro-ph.HE}
}
@book{maggiore2008gravitational,
title={Gravitational Waves: Volume 1: Theory and Experiments},
author={Maggiore, M.},
isbn={9780198570745},
lccn={2008270556},
series={Gravitational Waves},
url={https://books.google.it/books?id=AqVpQgAACAAJ},
year={2008},
publisher={OUP Oxford}
}
@book{maggiore2018gravitational,
title={Gravitational Waves: Volume 2: Astrophysics and Cosmology},
author={Maggiore, M.},
isbn={9780198570899},
lccn={2008270556},
series={Gravitational Waves},
url={https://books.google.it/books?id=3ZNODwAAQBAJ},
year={2018},
publisher={Oxford University Press}
}
@article{Abbott_2019,
title={GWTC-1: A Gravitational-Wave Transient Catalog of Compact Binary Mergers Observed by LIGO and Virgo during the First and Second Observing Runs},
volume={9},
ISSN={2160-3308},
url={http://dx.doi.org/10.1103/PhysRevX.9.031040},
DOI={10.1103/physrevx.9.031040},
number={3},
journal={Physical Review X},
publisher={American Physical Society (APS)},
author={Abbott, B. P. and Abbott, R. and Abbott, T. D. and Abraham, S. and Acernese, F. and Ackley, K. and Adams, C. and Adhikari, R. X. and Adya, V. B. and Affeldt, C. and et al.},
year={2019},
month={Sep}
}
@article{Baumgarte_2000,
title={On the Maximum Mass of Differentially Rotating Neutron Stars},
volume={528},
ISSN={0004-637X},
url={http://dx.doi.org/10.1086/312425},
DOI={10.1086/312425},
number={1},
journal={The Astrophysical Journal},
publisher={American Astronomical Society},
author={Baumgarte, Thomas W. and Shapiro, Stuart L. and Shibata, Masaru},
year={2000},
month={Jan},
pages={L29–L32}
}
@article{Abbott_2020a,
title={Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA},
volume={23},
ISSN={1433-8351},
url={http://dx.doi.org/10.1007/s41114-020-00026-9},
DOI={10.1007/s41114-020-00026-9},
number={1},
journal={Living Reviews in Relativity},
publisher={Springer Science and Business Media LLC},
author={Abbott, B. P. and Abbott, R. and Abbott, T. D. and Abraham, S. and Acernese, F. and Ackley, K. and Adams, C. and Adya, V. B. and Affeldt, C. and et al.},
year={2020},
month={Sep}
}
@ARTICLE{Ciolfi_2020,
AUTHOR={Ciolfi, Riccardo},
TITLE={Binary Neutron Star Mergers After GW170817},
JOURNAL={Frontiers in Astronomy and Space Sciences},
VOLUME={7},
PAGES={27},
YEAR={2020},
URL={https://www.frontiersin.org/article/10.3389/fspas.2020.00027},
DOI={10.3389/fspas.2020.00027},
ISSN={2296-987X},
ABSTRACT={The first combined detection of gravitational waves and electromagnetic signals from a binary neutron star (BNS) merger in August 2017 (an event named GW170817) represents a major landmark in the ongoing investigation of these extraordinary systems. In this short review, we discuss BNS mergers as events of utmost importance for astrophysics and fundamental physics and survey the main discoveries enabled by this first multimessenger observation, including compelling evidence that such mergers produce a copious amount of heavy r-process elements and can power short gamma-ray bursts. We further discuss some remaining key open questions regarding this event and BNS mergers in general, focusing on the current status and limitations of theoretical models and numerical simulations.}
}
@article{Abbott_2020b,
title={GW190425: Observation of a Compact Binary Coalescence with Total Mass $\sim3.4${M}$_\odot$},
volume={892},
ISSN={2041-8213},
url={http://dx.doi.org/10.3847/2041-8213/ab75f5},
DOI={10.3847/2041-8213/ab75f5},
number={1},
journal={The Astrophysical Journal},
publisher={American Astronomical Society},
author={Abbott, B. P. and Abbott, R. and Abbott, T. D. and Abraham, S. and Acernese, F. and Ackley, K. and Adams, C. and Adhikari, R. X. and Adya, V. B. and Affeldt, C. and et al.},
year={2020},
month={Mar},
pages={L3}
}
@article{Schutz_2011,
title={Networks of gravitational wave detectors and three figures of merit},
volume={28},
ISSN={1361-6382},
url={http://dx.doi.org/10.1088/0264-9381/28/12/125023},
DOI={10.1088/0264-9381/28/12/125023},
number={12},
journal={Classical and Quantum Gravity},
publisher={IOP Publishing},
author={Schutz, Bernard F},
year={2011},
month={May},
pages={125023}
}
@article{Sathyaprakash_2009,
title={Physics, Astrophysics and Cosmology with Gravitational Waves},
volume={12},
ISSN={1433-8351},
url={http://dx.doi.org/10.12942/lrr-2009-2},
DOI={10.12942/lrr-2009-2},
number={1},
journal={Living Reviews in Relativity},
publisher={Springer Science and Business Media LLC},
author={Sathyaprakash, B. S. and Schutz, Bernard F.},
year={2009},
month={Mar}
}
@Article{universe3030059,
AUTHOR = {Królak, Andrzej and Patil, Mandar},
TITLE = {The First Detection of Gravitational Waves},
JOURNAL = {Universe},
VOLUME = {3},
YEAR = {2017},
NUMBER = {3},
ARTICLE-NUMBER = {59},
URL = {https://www.mdpi.com/2218-1997/3/3/59},
ISSN = {2218-1997},
ABSTRACT = {This article deals with the first detection of gravitational waves by the advanced Laser Interferometer Gravitational Wave Observatory (LIGO) detectors on 14 September 2015, where the signal was generated by two stellar mass black holes with masses 36 M ⊙ and 29 M ⊙ that merged to form a 62 M ⊙ black hole, releasing 3 M ⊙ energy in gravitational waves, almost 1.3 billion years ago. We begin by providing a brief overview of gravitational waves, their sources and the gravitational wave detectors. We then describe in detail the first detection of gravitational waves from a binary black hole merger. We then comment on the electromagnetic follow up of the detection event with various telescopes. Finally, we conclude with the discussion on the tests of gravity and fundamental physics with the first gravitational wave detection event.},
DOI = {10.3390/universe3030059}
}
@article{Abbott_2017c,
title={Multi-messenger Observations of a Binary Neutron Star Merger},
volume={848},
ISSN={2041-8213},
url={http://dx.doi.org/10.3847/2041-8213/aa91c9},
DOI={10.3847/2041-8213/aa91c9},
number={2},
journal={The Astrophysical Journal},
publisher={American Astronomical Society},
author={Abbott, B. P. and Abbott, R. and Abbott, T. D. and Acernese, F. and Ackley, K. and Adams, C. and Adams, T. and Addesso, P. and Adhikari, R. X. and Adya, V. B. and et al.},
year={2017},
month={Oct},
pages={L12}
}
@mastersthesis{Puecher_2018,
author={Anna Puecher},
title={Characterization of the gravitational wave emission from binary neutron stars mergers},
school={Università degli Studi di Trento},
year={2018},
}
@phdthesis{Tringali_2017,
author={Maria Concetta Tringali},
title={Analysis methods for gravitational wave from binary neutron star coalescences: investigation on the post-merger phase},
school={Università degli Studi di Trento},
year={2017},
month={Jul},
howpublished = {\url{http://eprints-phd.biblio.unitn.it/2723/}}
}
@article{Akmal_1998,
title={Equation of state of nucleon matter and neutron star structure},
volume={58},
ISSN={1089-490X},
url={http://dx.doi.org/10.1103/PhysRevC.58.1804},
DOI={10.1103/physrevc.58.1804},
number={3},
journal={Physical Review C},
publisher={American Physical Society (APS)},
author={Akmal, A. and Pandharipande, V. R. and Ravenhall, D. G.},
year={1998},
month={Sep},
pages={1804–1828}
}
@article{Shen_2010,
title={Equation of state of dense matter from a density dependent relativistic mean field model},
volume={82},
ISSN={1089-490X},
url={http://dx.doi.org/10.1103/PhysRevC.82.015806},
DOI={10.1103/physrevc.82.015806},
number={1},
journal={Physical Review C},
publisher={American Physical Society (APS)},
author={Shen, G. and Horowitz, C. J. and Teige, S.},
year={2010},
month={Jul}
}
@misc{cWB_Manual,
title = {{cWB Manual}},
author = {cWB},
howpublished = {\url{https://gwburst.gitlab.io/documentation/latest/html/index.html}},
year = "2021",
note = {Accessed: 26 March 2021}
}
@misc{LIGO_Interferometer,
title = {{cWB Manual}},
author = {cWB},
howpublished = {\url{https://gwburst.gitlab.io/documentation/latest/html/index.html}},
year = "2021",
note = {Accessed: 26 March 2021}
}
@article{Han_2020,
doi = {10.3847/2041-8213/ab745a},
url = {https://doi.org/10.3847/2041-8213/ab745a},
year = 2020,
month = {feb},
publisher = {American Astronomical Society},
volume = {891},
number = {1},
pages = {L5},
author = {Ming-Zhe Han and Shao-Peng Tang and Yi-Ming Hu and Yin-Jie Li and Jin-Liang Jiang and Zhi-Ping Jin and Yi-Zhong Fan and Da-Ming Wei},
title = {Is {GW}190425 Consistent with Being a Neutron Star{\textendash}Black Hole Merger?},
journal = {The Astrophysical Journal},
abstract = {GW190425 is the second neutron star merger event detected by the Advanced LIGO/Virgo detectors. If interpreted as a double neutron star merger, the total gravitational mass is substantially larger than that of the binary systems identified in the Galaxy. In this work we analyze the gravitational-wave data within the neutron star–black hole merger scenario. For the black hole, we yield a mass of and an aligned spin of . As for the neutron star we find a mass of and the dimensionless tidal deformability of . These parameter ranges are for 90% credibility. The inferred masses of the neutron star and the black hole are not in tension with current observations and we suggest that GW190425 is a viable candidate of a neutron star–black hole merger event. Benefitting from the continual enhancement of the sensitivities of the advanced gravitational detectors and the increase of the number of the observatories, similar events are anticipated to be much more precisely measured in the future and the presence of black holes below the so-called mass gap will be unambiguously clarified. If confirmed, the mergers of neutron stars with (quickly rotating) low-mass black holes are likely important production sites of the heaviest r-process elements.}
}
@misc{ wiki_ligo,
author = "{LIGO Scientific Collaboration}",
title = "What is an Interferometer?",
howpublished = {\url{https://www.ligo.caltech.edu/page/what-is-interferometer}},
note = "[Online; accessed 29-March-2021]"
}
@misc{ curve_sens,
author = "{Brian O'Reilly, Marica Branchesi, Sadakazu Haino, Gianluca Gemme}",
title = "Noise curves used for Simulations in the update of the Observing Scenarios Paper",
howpublished = {\url{https://dcc.ligo.org/LIGO-T2000012/public}},
note = "[Online; accessed 30-March-2021]"
}
@misc{cWB,
title = {{coherent WaveBurst}},
author = {cWB},
howpublished = {\url{https://gwburst.gitlab.io/}},
year = "2021",
note = {Accessed: 01 April 2021}
}