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bibliography.bib
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@book{tsallis2009introduction,
title={Introduction to nonextensive statistical mechanics: approaching a complex world},
author={Tsallis, Constantino},
year={2009},
publisher={Springer Science \& Business Media}
}
@article{YAMANO2002486,
title = {Some properties of q-logarithm and q-exponential functions in Tsallis statistics},
journal = {Physica A: Statistical Mechanics and its Applications},
volume = {305},
number = {3},
pages = {486-496},
year = {2002},
issn = {0378-4371},
doi = {https://doi.org/10.1016/S0378-4371(01)00567-2},
url = {https://www.sciencedirect.com/science/article/pii/S0378437101005672},
author = {Takuya Yamano},
keywords = {Tsallis statistics},
abstract = {We present some formulae which q-logarithmic and q-exponential functions introduced in Tsallis statistics satisfy. Exact expression of the Mellin transform of q-exponential function is given. Moreover, the q-generalization of the digamma function is presented.}
}
@article{tsallis1988possible,
title={Possible generalization of Boltzmann-Gibbs statistics},
author={Tsallis, Constantino},
journal={Journal of statistical physics},
volume={52},
number={1},
pages={479--487},
year={1988},
publisher={Springer}
}
@article{Silva:1998iy,
title = "{A Maxwellian path to the q-nonextensive velocity distribution function}",
author = "Silva, R. and Plastino, A. R. and Lima, J. A. S.",
doi = "10.1016/S0375-9601(98)00710-5",
journal = "Phys. Lett. A",
volume = "249",
pages = "401--408",
year = "1998"
}
@article{Kusakabe:2018dzx,
author = "Kusakabe, Motohiko and Kajino, Toshitaka and Mathews, Grant J. and Luo, Yudong",
title = "{On the relative velocity distribution for general statistics and an application to big-bang nucleosynthesis under Tsallis statistics}",
eprint = "1806.01454",
archivePrefix = "arXiv",
primaryClass = "astro-ph.CO",
doi = "10.1103/PhysRevD.99.043505",
journal = "Phys. Rev. D",
volume = "99",
number = "4",
pages = "043505",
year = "2019"
}
@article{STOSIC20181069,
title = {Nonextensive triplets in cryptocurrency exchanges},
journal = {Physica A: Statistical Mechanics and its Applications},
volume = {505},
pages = {1069-1074},
year = {2018},
issn = {0378-4371},
doi = {https://doi.org/10.1016/j.physa.2018.04.066},
url = {https://www.sciencedirect.com/science/article/pii/S0378437118304965},
author = {Darko Stosic and Dusan Stosic and Teresa B. Ludermir and Tatijana Stosic},
keywords = {Non-extensive statistical mechanics, Cryptocurrency exchanges, Bitcoin,
-triplet},
abstract = {Cryptocurrencies represent a new type of financial assets that are traded in a decentralized and transparent way. Recently, cryptocurrencies with large market capitalization (mostly Bitcoin) have been studied theoretically, but a deeper understanding of their underlying mechanisms remains elusive. Here we explore the nonextensivity of price changes for 20 cryptocurrency exchanges from 2013 until 2017. We discover nonextensive triplets in the cryptocurrency market, where the three associated values for Bitcoin are remarkably close to those of the logistic map near the edge of chaos. The current findings strongly indicate that the cryptocurrency market represents a system whose physics is properly described by nonextensive statistical mechanics. Our results shed light on the complex and volatile nature of cryptocurrencies, and establish the first formal link with the nonextensive theory.}
}
@article{cyburt2016big,
title={Big Bang Nucleosynthesis: 2015},
author={Cyburt Richard, H and Fields Brian, D and Olive Keith, A and Yeh, Tsung-Han},
journal={Rev. Mod. Phys},
volume={88},
pages={015004},
year={2016}
}
@InProceedings{10.1007/978-94-010-3467-8_23,
author="Olbert, Stanislaw",
editor="Carovillano, Robert L.
and McClay, John F.
and Radoski, Henry R.",
title="Summary of Experimental Results from M.I.T. Detector on IMP-1",
booktitle="Physics of the Magnetosphere",
year="1968",
publisher="Springer Netherlands",
address="Dordrecht",
pages="641--659",
abstract="This paper is an extended version of the summary of experimental results reported by Dr. Pai and myself at the AGU meeting of April 1967, in Washington, D.C. The results pertain primarily to the M.I.T. data from IMP-1, launched in November 1963.( Figure 1, taken from Ness (1966), shows the first 30 orbits of IMP-1 projected into the ecliptic plane. Apogee is at about 30 earth radii, and the major axis of the first orbit points roughly toward the sun. The orbital period is about four days so that during each revolution the major axis of the orbit rotates by about 4{\textdegree} toward the dawn side of the earth. In a time span of about four months, the satellite explores a vast region that covers the noon, morning, dawn, and predawn portion of the magneto-sphere in the neighborhood of the ecliptic plane. Furthermore, and this is essential to the discussion, the large apogee makes it possible for the satellite not only to cross the sunward portion of the magnetosphere and the magnetosheath, but also to enter fairly deeply into the interplanetary domain where the presence of Earth's magnetic field is not felt.",
isbn="978-94-010-3467-8"
}
@book{iliadis2015nuclear,
title={Nuclear Physics of Stars},
author={Iliadis, C.},
isbn={9783527336487},
series={Physics Textbook},
url={https://books.google.co.in/books?id=iUCkBgAAQBAJ},
year={2015},
publisher={Wiley}
}
@article{Serpico_2004,
doi = {10.1088/1475-7516/2004/12/010},
url = {https://doi.org/10.1088%2F1475-7516%2F2004%2F12%2F010},
year = 2004,
month = {dec},
publisher = {{IOP} Publishing},
volume = {2004},
number = {12},
pages = {010--010},
author = {P D Serpico and S Esposito and F Iocco and G Mangano and G Miele and O Pisanti},
title = {Nuclear reaction network for primordial nucleosynthesis: a detailed analysis of rates, uncertainties and light nuclei yields},
journal = {Journal of Cosmology and Astroparticle Physics}
}
@article{article,
author = {Bertulani, Carlos and Fuqua, J. and Hussein, M.},
year = {2012},
month = {05},
title = {Big Bang nucleosynthesis with a non-Maxwellian distribution},
volume = {767},
journal = {The Astrophysical Journal},
doi = {10.1088/0004-637X/767/1/67}
}
@article{Hou_2017,
doi = {10.3847/1538-4357/834/2/165},
url = {https://doi.org/10.3847%2F1538-4357%2F834%2F2%2F165},
year = 2017,
month = {jan},
publisher = {American Astronomical Society},
volume = {834},
number = {2},
pages = {165},
author = {S. Q. Hou and J. J. He and A. Parikh and D. Kahl and C. A. Bertulani and T. Kajino and G. J. Mathews and G. Zhao},
title = {{NON}-{EXTENSIVE} {STATISTICS} {TO} {THE} {COSMOLOGICAL} {LITHIUM} {PROBLEM}},
journal = {The Astrophysical Journal}
}
@misc{pypi,
author={tt-nakamura},
title={{BBN} 0.0.1 Python Package Index - PyPI},
url={https://pypi.org/project/BBN/#description},
urldate = {2021-03-27},
publisher={Python Software Foundation}
}
@article{smith1993experimental,
title={Experimental, computational, and observational analysis of primordial nucleosynthesis},
author={Smith, Michael S and Kawano, Lawrence H and Malaney, Robert A},
journal={The Astrophysical Journal Supplement Series},
volume={85},
pages={219--247},
year={1993}
}
@article{PITROU20181,
title = {Precision big bang nucleosynthesis with improved Helium-4 predictions},
journal = {Physics Reports},
volume = {754},
pages = {1-66},
year = {2018},
note = {Precision big bang nucleosynthesis with improved Helium-4 predictions},
issn = {0370-1573},
doi = {https://doi.org/10.1016/j.physrep.2018.04.005},
url = {https://www.sciencedirect.com/science/article/pii/S0370157318301054},
author = {Cyril Pitrou and Alain Coc and Jean-Philippe Uzan and Elisabeth Vangioni},
abstract = {Primordial nucleosynthesis is one of the three historical evidences for the big bang model, together with the expansion of the universe and the cosmic microwave background. There is a good global agreement between the computed primordial abundances of helium-4, deuterium, helium-3 and their values deduced from observations. Now that the number of neutrino families and the baryonic densities have been fixed by laboratory measurements or CMB observations, the model has no free parameter and its predictions are rigid. Since this is the earliest cosmic process for which we a priori know all the physics involved, departure from its predictions could provide hints or constraints on new physics or astrophysics in the early universe. Precision on primordial abundances deduced from observations has recently been drastically improved and reach the percent level for both deuterium and helium-4. Accordingly, the BBN predictions should reach the same level of precision. For most isotopes, the dominant sources of uncertainty come from those on the laboratory thermonuclear reactions. This article focuses on helium-4 whose predicted primordial abundance depends essentially on weak interactions which control the neutron–proton ratio. The rates of the various weak interaction processes depend on the experimentally measured neutron lifetime, but also includes numerous corrections that we thoroughly investigate here. They are the radiative, zero-temperature, corrections, finite nucleon mass corrections, finite temperature radiative corrections, weak-magnetism, and QED plasma effects, which are for the first time all included and calculated in a self consistent way, allowing to take into account the correlations between them, and verifying that all satisfy detailed balance. Finally, we include the incomplete neutrino decoupling and claim to reach a 10−4 accuracy on the helium-4 predicted mass fraction of 0.24709±0.00017 (when including the uncertainty on the neutron lifetime). In addition, we provide a Mathematica primordial nucleosynthesis code that incorporates, not only these corrections but also a full network of reactions, using the best available thermonuclear reaction rates, allowing the predictions of primordial abundances of helium-4, deuterium, helium-3 and lithium-7 but also of heavier isotopes up to the CNO region.}
}
@article{scikit-learn,
title={Scikit-learn: Machine Learning in {P}ython},
author={Pedregosa, F. and Varoquaux, G. and Gramfort, A. and Michel, V.
and Thirion, B. and Grisel, O. and Blondel, M. and Prettenhofer, P.
and Weiss, R. and Dubourg, V. and Vanderplas, J. and Passos, A. and
Cournapeau, D. and Brucher, M. and Perrot, M. and Duchesnay, E.},
journal={Journal of Machine Learning Research},
volume={12},
pages={2825--2830},
year={2011}
}
@article{Simplified_reaction_network,
author = {Cook, Kaitlin and Luong, D.H. and Carter, I. and Dasgupta, Mahananda and Hinde, D.J. and McNeil, S. and Rafferty, D. and Ramachandran, K. and Simenel, C. and Williams, Elizabeth},
year = {2015},
month = {04},
pages = {00002},
title = {Breakup following interactions with light targets: Investigating new methods to probe nuclear physics input to the cosmological lithium problem},
volume = {91},
journal = {EPJ Web of Conferences},
doi = {10.1051/epjconf/20159100002}
}
@article{asdfasdf,
author = {Tsallis, Constantino and Brigatti, Edgardo},
year = {2003},
month = {05},
pages = {},
title = {Nonextensive statistical mechanics: A brief introduction},
volume = {16},
journal = {Continuum Mechanics and Thermodynamics},
doi = {10.1007/s00161-004-0174-4}
}