[ [ [ "https://dx.doi.org/10.1007/BF01700692" ], { "headers": { "accept": "application/x-bibtex" } }, "@article{G_del_1931,\n\tdoi = {10.1007/bf01700692},\n\turl = {https://doi.org/10.1007%2Fbf01700692},\n\tyear = 1931,\n\tmonth = {dec},\n\tpublisher = {Springer Nature},\n\tvolume = {38-38},\n\tnumber = {1},\n\tpages = {173--198},\n\tauthor = {Kurt G\u00f6del},\n\ttitle = {\u00dcber formal unentscheidbare S\u00e4tze der Principia Mathematica und verwandter Systeme I},\n\tjournal = {Monatshefte f\u00fcr Mathematik und Physik}\n}", 200, null ], [ [ "https://dx.doi.org/10.1007/BF01700692" ], { "headers": { "accept": "application/x-bibtex" } }, "@article{G_del_1931,\n\tdoi = {10.1007/bf01700692},\n\turl = {https://doi.org/10.1007%2Fbf01700692},\n\tyear = 1931,\n\tmonth = {dec},\n\tpublisher = {Springer Nature},\n\tvolume = {38-38},\n\tnumber = {1},\n\tpages = {173--198},\n\tauthor = {Kurt G\u00f6del},\n\ttitle = {\u00dcber formal unentscheidbare S\u00e4tze der Principia Mathematica und verwandter Systeme I},\n\tjournal = {Monatshefte f\u00fcr Mathematik und Physik}\n}", 200, null ], [ [ "https://dx.doi.org/10.1007/s00422-012-0514-6" ], { "headers": { "accept": "application/x-bibtex" } }, "@article{Loeb_2012,\n\tdoi = {10.1007/s00422-012-0514-6},\n\turl = {https://doi.org/10.1007%2Fs00422-012-0514-6},\n\tyear = 2012,\n\tmonth = {aug},\n\tpublisher = {Springer Nature},\n\tvolume = {106},\n\tnumber = {11-12},\n\tpages = {757--765},\n\tauthor = {Gerald E. Loeb},\n\ttitle = {Optimal isn't good enough},\n\tjournal = {Biological Cybernetics}\n}", 200, null ], [ [ "https://dx.doi.org/10.1007/s00422-012-0514-6" ], { "headers": { "accept": "application/x-bibtex" } }, "@article{Loeb_2012,\n\tdoi = {10.1007/s00422-012-0514-6},\n\turl = {https://doi.org/10.1007%2Fs00422-012-0514-6},\n\tyear = 2012,\n\tmonth = {aug},\n\tpublisher = {Springer Nature},\n\tvolume = {106},\n\tnumber = {11-12},\n\tpages = {757--765},\n\tauthor = {Gerald E. Loeb},\n\ttitle = {Optimal isn't good enough},\n\tjournal = {Biological Cybernetics}\n}", 200, null ], [ [ "https://dx.doi.org/10.1007/s00422-012-0514-6" ], { "headers": { "accept": "application/x-bibtex" } }, "@article{Loeb_2012,\n\tdoi = {10.1007/s00422-012-0514-6},\n\turl = {https://doi.org/10.1007%2Fs00422-012-0514-6},\n\tyear = 2012,\n\tmonth = {aug},\n\tpublisher = {Springer Nature},\n\tvolume = {106},\n\tnumber = {11-12},\n\tpages = {757--765},\n\tauthor = {Gerald E. Loeb},\n\ttitle = {Optimal isn't good enough},\n\tjournal = {Biological Cybernetics}\n}", 200, null ], [ [ "https://dx.doi.org/10.1007/s00422-012-0514-6" ], { "headers": { "accept": "application/x-bibtex" } }, "@article{Loeb_2012,\n\tdoi = {10.1007/s00422-012-0514-6},\n\turl = {https://doi.org/10.1007%2Fs00422-012-0514-6},\n\tyear = 2012,\n\tmonth = {aug},\n\tpublisher = {Springer Nature},\n\tvolume = {106},\n\tnumber = {11-12},\n\tpages = {757--765},\n\tauthor = {Gerald E. Loeb},\n\ttitle = {Optimal isn't good enough},\n\tjournal = {Biological Cybernetics}\n}", 200, null ], [ [ "https://dx.doi.org/10.1086/307221" ], { "headers": { "accept": "application/x-bibtex" } }, "@article{Perlmutter_1999,\n\tdoi = {10.1086/307221},\n\turl = {https://doi.org/10.1086%2F307221},\n\tyear = 1999,\n\tmonth = {jun},\n\tpublisher = {{IOP} Publishing},\n\tvolume = {517},\n\tnumber = {2},\n\tpages = {565--586},\n\tauthor = {S. Perlmutter and G. Aldering and G. Goldhaber and R. A. Knop and P. Nugent and P. G. Castro and S. Deustua and S. Fabbro and A. Goobar and D. E. Groom and I. M. Hook and A. G. Kim and M. Y. Kim and J. C. Lee and N. J. Nunes and R. Pain and C. R. Pennypacker and R. Quimby and C. Lidman and R. S. Ellis and M. Irwin and R. G. McMahon and P. Ruiz-Lapuente and N. Walton and B. Schaefer and B. J. Boyle and A. V. Filippenko and T. Matheson and A. S. Fruchter and N. Panagia and H. J. M. Newberg and W. J. Couch and The Supernova Cosmology Project},\n\ttitle = {Measurements of $\\{upOmega}$ and $\\{upLambda}$ from 42 High-Redshift Supernovae},\n\tjournal = {The Astrophysical Journal}\n}", 200, null ], [ [ "https://dx.doi.org/10.1086/307221" ], { "headers": { "accept": "application/x-bibtex" } }, "@article{Perlmutter_1999,\n\tdoi = {10.1086/307221},\n\turl = {https://doi.org/10.1086%2F307221},\n\tyear = 1999,\n\tmonth = {jun},\n\tpublisher = {{IOP} Publishing},\n\tvolume = {517},\n\tnumber = {2},\n\tpages = {565--586},\n\tauthor = {S. Perlmutter and G. Aldering and G. Goldhaber and R. A. Knop and P. Nugent and P. G. Castro and S. Deustua and S. Fabbro and A. Goobar and D. E. Groom and I. M. Hook and A. G. Kim and M. Y. Kim and J. C. Lee and N. J. Nunes and R. Pain and C. R. Pennypacker and R. Quimby and C. Lidman and R. S. Ellis and M. Irwin and R. G. McMahon and P. Ruiz-Lapuente and N. Walton and B. Schaefer and B. J. Boyle and A. V. Filippenko and T. Matheson and A. S. Fruchter and N. Panagia and H. J. M. Newberg and W. J. Couch and The Supernova Cosmology Project},\n\ttitle = {Measurements of $\\{upOmega}$ and $\\{upLambda}$ from 42 High-Redshift Supernovae},\n\tjournal = {The Astrophysical Journal}\n}", 200, null ], [ [ "https://dx.doi.org/10.1103/INVALIDDOI.89.084044" ], { "headers": { "accept": "application/x-bibtex" } }, "\n\n\nError: DOI Not Found\n\n\n\n\n \n\n\n\n\n\n\n
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DOI Not Found

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10.1103/INVALIDDOI.89.084044

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\n\n\n", 404, "404 Client Error: for url: https://dx.doi.org/10.1103/INVALIDDOI.89.084044" ], [ [ "https://dx.doi.org/10.1186/s12984-017-0305-3" ], { "headers": { "accept": "application/x-bibtex" } }, "@article{Valero_Cuevas_2017,\n\tdoi = {10.1186/s12984-017-0305-3},\n\turl = {https://doi.org/10.1186%2Fs12984-017-0305-3},\n\tyear = 2017,\n\tmonth = {oct},\n\tpublisher = {Springer Nature},\n\tvolume = {14},\n\tnumber = {1},\n\tauthor = {Francisco J. Valero-Cuevas and Marco Santello},\n\ttitle = {On neuromechanical approaches for the study of biological and robotic grasp and manipulation},\n\tjournal = {Journal of {NeuroEngineering} and Rehabilitation}\n}", 200, null ], [ [ "https://dx.doi.org/999999" ], { "headers": { "accept": "application/x-bibtex" } }, "\n\n\nError: DOI Not Found\n\n\n\n\n \n\n\n\n\n\n\n
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DOI Not Found

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10/999999

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\n\n\n", 404, "404 Client Error: for url: https://dx.doi.org/999999" ], [ [ "https://export.arxiv.org/api/query?id_list=1312.2021" ], {}, "\n\n \n ArXiv Query: search_query=&id_list=1312.2021&start=0&max_results=10\n http://arxiv.org/api/eXBvi61X4ShcFWF7lwJgRo7KSFk\n 2019-01-04T00:00:00-05:00\n 1\n 0\n 10\n \n http://arxiv.org/abs/1312.2021v1\n 2013-12-06T21:33:40Z\n 2013-12-06T21:33:40Z\n Living with the Wrong Sign\n We describe a UV complete asymptotically fragile Lorentz-invariant theory\nexhibiting superluminal signal propagation. Its low energy effective action\ncontains \"wrong\" sign higher dimensional operators. Nevertheless, the theory\ngives rise to an S-matrix, which is defined at all energies. As expected for a\nnon-local theory, the corresponding scattering amplitudes are not exponentially\nbounded on the physical sheet, but otherwise are healthy. We study some of the\nphysical consequences of this S-matrix.\n\n \n Patrick Cooper\n \n \n Sergei Dubovsky\n \n \n Ali Mohsen\n \n 10.1103/INVALIDDOI.89.084044\n \n Phys. Rev. D 89, 084044 (2014)\n \n \n \n \n \n \n\n", 200, null ], [ [ "https://export.arxiv.org/api/query?id_list=1710.08557" ], {}, "\n\n \n ArXiv Query: search_query=&id_list=1710.08557&start=0&max_results=10\n http://arxiv.org/api/bNB5RPNlUYbELau5YJ4IzaIq1x8\n 2019-01-04T00:00:00-05:00\n 1\n 0\n 10\n \n http://arxiv.org/abs/1710.08557v1\n 2017-10-24T00:21:32Z\n 2017-10-24T00:21:32Z\n On Neuromechanical Approaches for the Study of Biological Grasp and\n Manipulation\n Biological and robotic grasp and manipulation are undeniably similar at the\nlevel of mechanical task performance. However, their underlying fundamental\nbiological vs. engineering mechanisms are, by definition, dramatically\ndifferent and can even be antithetical. Even our approach to each is\ndiametrically opposite: inductive science for the study of biological systems\nvs. engineering synthesis for the design and construction of robotic systems.\nThe past 20 years have seen several conceptual advances in both fields and the\nquest to unify them. Chief among them is the reluctant recognition that their\nunderlying fundamental mechanisms may actually share limited common ground,\nwhile exhibiting many fundamental differences. This recognition is particularly\nliberating because it allows us to resolve and move beyond multiple paradoxes\nand contradictions that arose from the initial reasonable assumption of a large\ncommon ground. Here, we begin by introducing the perspective of neuromechanics,\nwhich emphasizes that real-world behavior emerges from the intimate\ninteractions among the physical structure of the system, the mechanical\nrequirements of a task, the feasible neural control actions to produce it, and\nthe ability of the neuromuscular system to adapt through interactions with the\nenvironment. This allows us to articulate a succinct overview of a few salient\nconceptual paradoxes and contradictions regarding under-determined vs.\nover-determined mechanics, under- vs. over-actuated control, prescribed vs.\nemergent function, learning vs. implementation vs. adaptation, prescriptive vs.\ndescriptive synergies, and optimal vs. habitual performance. We conclude by\npresenting open questions and suggesting directions for future research. We\nhope this frank assessment of the state-of-the-art will encourage and guide\nthese communities to continue to interact and make progress in these important\nareas.\n\n \n Francisco J Valero-Cuevas\n \n \n Marco Santello\n \n 10.1186/s12984-017-0305-3\n \n Journal of NeuroEngineering and Rehabilitation, 2017\n \n \n \n \n \n\n", 200, null ], [ [ "https://export.arxiv.org/api/query?id_list=1710.08557" ], {}, "\n\n \n ArXiv Query: search_query=&id_list=1710.08557&start=0&max_results=10\n http://arxiv.org/api/bNB5RPNlUYbELau5YJ4IzaIq1x8\n 2019-01-04T00:00:00-05:00\n 1\n 0\n 10\n \n http://arxiv.org/abs/1710.08557v1\n 2017-10-24T00:21:32Z\n 2017-10-24T00:21:32Z\n On Neuromechanical Approaches for the Study of Biological Grasp and\n Manipulation\n Biological and robotic grasp and manipulation are undeniably similar at the\nlevel of mechanical task performance. However, their underlying fundamental\nbiological vs. engineering mechanisms are, by definition, dramatically\ndifferent and can even be antithetical. Even our approach to each is\ndiametrically opposite: inductive science for the study of biological systems\nvs. engineering synthesis for the design and construction of robotic systems.\nThe past 20 years have seen several conceptual advances in both fields and the\nquest to unify them. Chief among them is the reluctant recognition that their\nunderlying fundamental mechanisms may actually share limited common ground,\nwhile exhibiting many fundamental differences. This recognition is particularly\nliberating because it allows us to resolve and move beyond multiple paradoxes\nand contradictions that arose from the initial reasonable assumption of a large\ncommon ground. Here, we begin by introducing the perspective of neuromechanics,\nwhich emphasizes that real-world behavior emerges from the intimate\ninteractions among the physical structure of the system, the mechanical\nrequirements of a task, the feasible neural control actions to produce it, and\nthe ability of the neuromuscular system to adapt through interactions with the\nenvironment. This allows us to articulate a succinct overview of a few salient\nconceptual paradoxes and contradictions regarding under-determined vs.\nover-determined mechanics, under- vs. over-actuated control, prescribed vs.\nemergent function, learning vs. implementation vs. adaptation, prescriptive vs.\ndescriptive synergies, and optimal vs. habitual performance. We conclude by\npresenting open questions and suggesting directions for future research. We\nhope this frank assessment of the state-of-the-art will encourage and guide\nthese communities to continue to interact and make progress in these important\nareas.\n\n \n Francisco J Valero-Cuevas\n \n \n Marco Santello\n \n 10.1186/s12984-017-0305-3\n \n Journal of NeuroEngineering and Rehabilitation, 2017\n \n \n \n \n \n\n", 200, null ], [ [ "https://export.arxiv.org/api/query?id_list=INVALIDID" ], {}, "\n\n \n ArXiv Query: search_query=&id_list=INVALIDID\n http://arxiv.org/api//TMQrv7hMz9PNtlUyGrhFtefYFQ\n 2019-01-04T00:00:00-05:00\n 1\n 0\n 1\n \n http://arxiv.org/api/errors#incorrect_id_format_for_INVALIDID\n Error\n incorrect id format for INVALIDID\n 2019-01-04T00:00:00-05:00\n \n \n arXiv api core\n \n \n\n", 400, "400 Client Error: Bad Request for url: https://export.arxiv.org/api/query?id_list=INVALIDID" ], [ [ "https://export.arxiv.org/api/query?id_list=astro-ph/9812133" ], {}, "\n\n \n ArXiv Query: search_query=&id_list=astro-ph/9812133&start=0&max_results=10\n http://arxiv.org/api/SfKekabpSjI/htnxCLpK3q9AsUs\n 2019-01-04T00:00:00-05:00\n 1\n 0\n 10\n \n http://arxiv.org/abs/astro-ph/9812133v1\n 1998-12-08T03:27:34Z\n 1998-12-08T03:27:34Z\n Measurements of Omega and Lambda from 42 High-Redshift Supernovae\n We report measurements of the mass density, Omega_M, and\ncosmological-constant energy density, Omega_Lambda, of the universe based on\nthe analysis of 42 Type Ia supernovae discovered by the Supernova Cosmology\nProject. The magnitude-redshift data for these SNe, at redshifts between 0.18\nand 0.83, are fit jointly with a set of SNe from the Calan/Tololo Supernova\nSurvey, at redshifts below 0.1, to yield values for the cosmological\nparameters. All SN peak magnitudes are standardized using a SN Ia lightcurve\nwidth-luminosity relation. The measurement yields a joint probability\ndistribution of the cosmological parameters that is approximated by the\nrelation 0.8 Omega_M - 0.6 Omega_Lambda ~= -0.2 +/- 0.1 in the region of\ninterest (Omega_M <~ 1.5). For a flat (Omega_M + Omega_Lambda = 1) cosmology we\nfind Omega_M = 0.28{+0.09,-0.08} (1 sigma statistical) {+0.05,-0.04}\n(identified systematics). The data are strongly inconsistent with a Lambda = 0\nflat cosmology, the simplest inflationary universe model. An open, Lambda = 0\ncosmology also does not fit the data well: the data indicate that the\ncosmological constant is non-zero and positive, with a confidence of P(Lambda >\n0) = 99%, including the identified systematic uncertainties. The best-fit age\nof the universe relative to the Hubble time is t_0 = 14.9{+1.4,-1.1} (0.63/h)\nGyr for a flat cosmology. The size of our sample allows us to perform a variety\nof statistical tests to check for possible systematic errors and biases. We\nfind no significant differences in either the host reddening distribution or\nMalmquist bias between the low-redshift Calan/Tololo sample and our\nhigh-redshift sample. The conclusions are robust whether or not a\nwidth-luminosity relation is used to standardize the SN peak magnitudes.\n\n \n S. Perlmutter\n The Supernova Cosmology Project\n \n \n G. Aldering\n The Supernova Cosmology Project\n \n \n G. Goldhaber\n The Supernova Cosmology Project\n \n \n R. A. Knop\n The Supernova Cosmology Project\n \n \n P. Nugent\n The Supernova Cosmology Project\n \n \n P. G. Castro\n The Supernova Cosmology Project\n \n \n S. Deustua\n The Supernova Cosmology Project\n \n \n S. Fabbro\n The Supernova Cosmology Project\n \n \n A. Goobar\n The Supernova Cosmology Project\n \n \n D. E. Groom\n The Supernova Cosmology Project\n \n \n I. M. Hook\n The Supernova Cosmology Project\n \n \n A. G. Kim\n The Supernova Cosmology Project\n \n \n M. Y. Kim\n The Supernova Cosmology Project\n \n \n J. C. Lee\n The Supernova Cosmology Project\n \n \n N. J. Nunes\n The Supernova Cosmology Project\n \n \n R. Pain\n The Supernova Cosmology Project\n \n \n C. R. Pennypacker\n The Supernova Cosmology Project\n \n \n R. Quimby\n The Supernova Cosmology Project\n \n \n C. Lidman\n The Supernova Cosmology Project\n \n \n R. S. Ellis\n The Supernova Cosmology Project\n \n \n M. Irwin\n The Supernova Cosmology Project\n \n \n R. G. McMahon\n The Supernova Cosmology Project\n \n \n P. Ruiz-Lapuente\n The Supernova Cosmology Project\n \n \n N. Walton\n The Supernova Cosmology Project\n \n \n B. Schaefer\n The Supernova Cosmology Project\n \n \n B. J. Boyle\n The Supernova Cosmology Project\n \n \n A. V. Filippenko\n The Supernova Cosmology Project\n \n \n T. Matheson\n The Supernova Cosmology Project\n \n \n A. S. Fruchter\n The Supernova Cosmology Project\n \n \n N. Panagia\n The Supernova Cosmology Project\n \n \n H. J. M. Newberg\n The Supernova Cosmology Project\n \n \n W. J. Couch\n The Supernova Cosmology Project\n \n 10.1086/307221\n \n 21 pages and 10 figures. Accepted for publication in the\n Astrophysical Journal. Individual color figures, supplementary tables, and\n preprint also available at http://www-supernova.lbl.gov/\n Astrophys.J.517:565-586,1999\n \n \n \n \n \n \n \n\n", 200, null ], [ [ "https://export.arxiv.org/api/query?id_list=astro-ph/9812133" ], {}, "\n\n \n ArXiv Query: search_query=&id_list=astro-ph/9812133&start=0&max_results=10\n http://arxiv.org/api/SfKekabpSjI/htnxCLpK3q9AsUs\n 2019-01-04T00:00:00-05:00\n 1\n 0\n 10\n \n http://arxiv.org/abs/astro-ph/9812133v1\n 1998-12-08T03:27:34Z\n 1998-12-08T03:27:34Z\n Measurements of Omega and Lambda from 42 High-Redshift Supernovae\n We report measurements of the mass density, Omega_M, and\ncosmological-constant energy density, Omega_Lambda, of the universe based on\nthe analysis of 42 Type Ia supernovae discovered by the Supernova Cosmology\nProject. The magnitude-redshift data for these SNe, at redshifts between 0.18\nand 0.83, are fit jointly with a set of SNe from the Calan/Tololo Supernova\nSurvey, at redshifts below 0.1, to yield values for the cosmological\nparameters. All SN peak magnitudes are standardized using a SN Ia lightcurve\nwidth-luminosity relation. The measurement yields a joint probability\ndistribution of the cosmological parameters that is approximated by the\nrelation 0.8 Omega_M - 0.6 Omega_Lambda ~= -0.2 +/- 0.1 in the region of\ninterest (Omega_M <~ 1.5). For a flat (Omega_M + Omega_Lambda = 1) cosmology we\nfind Omega_M = 0.28{+0.09,-0.08} (1 sigma statistical) {+0.05,-0.04}\n(identified systematics). The data are strongly inconsistent with a Lambda = 0\nflat cosmology, the simplest inflationary universe model. An open, Lambda = 0\ncosmology also does not fit the data well: the data indicate that the\ncosmological constant is non-zero and positive, with a confidence of P(Lambda >\n0) = 99%, including the identified systematic uncertainties. The best-fit age\nof the universe relative to the Hubble time is t_0 = 14.9{+1.4,-1.1} (0.63/h)\nGyr for a flat cosmology. The size of our sample allows us to perform a variety\nof statistical tests to check for possible systematic errors and biases. We\nfind no significant differences in either the host reddening distribution or\nMalmquist bias between the low-redshift Calan/Tololo sample and our\nhigh-redshift sample. The conclusions are robust whether or not a\nwidth-luminosity relation is used to standardize the SN peak magnitudes.\n\n \n S. Perlmutter\n The Supernova Cosmology Project\n \n \n G. Aldering\n The Supernova Cosmology Project\n \n \n G. Goldhaber\n The Supernova Cosmology Project\n \n \n R. A. Knop\n The Supernova Cosmology Project\n \n \n P. Nugent\n The Supernova Cosmology Project\n \n \n P. G. Castro\n The Supernova Cosmology Project\n \n \n S. Deustua\n The Supernova Cosmology Project\n \n \n S. Fabbro\n The Supernova Cosmology Project\n \n \n A. Goobar\n The Supernova Cosmology Project\n \n \n D. E. Groom\n The Supernova Cosmology Project\n \n \n I. M. Hook\n The Supernova Cosmology Project\n \n \n A. G. Kim\n The Supernova Cosmology Project\n \n \n M. Y. Kim\n The Supernova Cosmology Project\n \n \n J. C. Lee\n The Supernova Cosmology Project\n \n \n N. J. Nunes\n The Supernova Cosmology Project\n \n \n R. Pain\n The Supernova Cosmology Project\n \n \n C. R. Pennypacker\n The Supernova Cosmology Project\n \n \n R. Quimby\n The Supernova Cosmology Project\n \n \n C. Lidman\n The Supernova Cosmology Project\n \n \n R. S. Ellis\n The Supernova Cosmology Project\n \n \n M. Irwin\n The Supernova Cosmology Project\n \n \n R. G. McMahon\n The Supernova Cosmology Project\n \n \n P. Ruiz-Lapuente\n The Supernova Cosmology Project\n \n \n N. Walton\n The Supernova Cosmology Project\n \n \n B. Schaefer\n The Supernova Cosmology Project\n \n \n B. J. Boyle\n The Supernova Cosmology Project\n \n \n A. V. Filippenko\n The Supernova Cosmology Project\n \n \n T. Matheson\n The Supernova Cosmology Project\n \n \n A. S. Fruchter\n The Supernova Cosmology Project\n \n \n N. Panagia\n The Supernova Cosmology Project\n \n \n H. J. M. Newberg\n The Supernova Cosmology Project\n \n \n W. J. Couch\n The Supernova Cosmology Project\n \n 10.1086/307221\n \n 21 pages and 10 figures. Accepted for publication in the\n Astrophysical Journal. Individual color figures, supplementary tables, and\n preprint also available at http://www-supernova.lbl.gov/\n Astrophys.J.517:565-586,1999\n \n \n \n \n \n \n \n\n", 200, null ], [ [ "https://export.arxiv.org/api/query?id_list=math/0211159" ], {}, "\n\n \n ArXiv Query: search_query=&id_list=math/0211159&start=0&max_results=10\n http://arxiv.org/api/4nVRTcAL5Np4oaGFQnqVPG0+c5k\n 2019-01-04T00:00:00-05:00\n 1\n 0\n 10\n \n http://arxiv.org/abs/math/0211159v1\n 2002-11-11T16:11:49Z\n 2002-11-11T16:11:49Z\n The entropy formula for the Ricci flow and its geometric applications\n We present a monotonic expression for the Ricci flow, valid in all dimensions\nand without curvature assumptions. It is interpreted as an entropy for a\ncertain canonical ensemble. Several geometric applications are given. In\nparticular, (1) Ricci flow, considered on the space of riemannian metrics\nmodulo diffeomorphism and scaling, has no nontrivial periodic orbits (that is,\nother than fixed points); (2) In a region, where singularity is forming in\nfinite time, the injectivity radius is controlled by the curvature; (3) Ricci\nflow can not quickly turn an almost euclidean region into a very curved one, no\nmatter what happens far away. We also verify several assertions related to\nRichard Hamilton's program for the proof of Thurston geometrization conjecture\nfor closed three-manifolds, and give a sketch of an eclectic proof of this\nconjecture, making use of earlier results on collapsing with local lower\ncurvature bound.\n\n \n Grisha Perelman\n \n 39 pages\n \n \n \n \n \n \n\n", 200, null ], [ [ "https://export.arxiv.org/api/query?id_list=math/9501234" ], {}, "\n\n \n ArXiv Query: search_query=&id_list=math/9501234&start=0&max_results=10\n http://arxiv.org/api/7jH0+0cTfQ0YcTJCQMYE9FyHjoA\n 2019-01-04T00:00:00-05:00\n 1\n 0\n 10\n \n http://arxiv.org/abs/math/9501234v1\n 1995-01-23T00:00:00Z\n 1995-01-23T00:00:00Z\n Aztec diamonds, checkerboard graphs, and spanning trees\n This note derives the characteristic polynomial of a graph that represents\nnonjump moves in a generalized game of checkers. The number of spanning trees\nis also determined.\n\n \n Donald E. Knuth\n \n J. Algebraic Combin. 6 (1997), no. 3, 253--257\n \n \n \n \n \n\n", 200, null ], [ [ "https://export.arxiv.org/api/query?id_list=math/9501234" ], {}, "\n\n \n ArXiv Query: search_query=&id_list=math/9501234&start=0&max_results=10\n http://arxiv.org/api/7jH0+0cTfQ0YcTJCQMYE9FyHjoA\n 2019-01-04T00:00:00-05:00\n 1\n 0\n 10\n \n http://arxiv.org/abs/math/9501234v1\n 1995-01-23T00:00:00Z\n 1995-01-23T00:00:00Z\n Aztec diamonds, checkerboard graphs, and spanning trees\n This note derives the characteristic polynomial of a graph that represents\nnonjump moves in a generalized game of checkers. The number of spanning trees\nis also determined.\n\n \n Donald E. Knuth\n \n J. Algebraic Combin. 6 (1997), no. 3, 253--257\n \n \n \n \n \n\n", 200, null ], [ [ "https://export.arxiv.org/api/query?id_list=math/9501234" ], {}, "\n\n \n ArXiv Query: search_query=&id_list=math/9501234&start=0&max_results=10\n http://arxiv.org/api/7jH0+0cTfQ0YcTJCQMYE9FyHjoA\n 2019-01-04T00:00:00-05:00\n 1\n 0\n 10\n \n http://arxiv.org/abs/math/9501234v1\n 1995-01-23T00:00:00Z\n 1995-01-23T00:00:00Z\n Aztec diamonds, checkerboard graphs, and spanning trees\n This note derives the characteristic polynomial of a graph that represents\nnonjump moves in a generalized game of checkers. The number of spanning trees\nis also determined.\n\n \n Donald E. Knuth\n \n J. Algebraic Combin. 6 (1997), no. 3, 253--257\n \n \n \n \n \n\n", 200, null ], [ [ "https://export.arxiv.org/api/query?id_list=math/9501234" ], {}, "\n\n \n ArXiv Query: search_query=&id_list=math/9501234&start=0&max_results=10\n http://arxiv.org/api/7jH0+0cTfQ0YcTJCQMYE9FyHjoA\n 2019-01-04T00:00:00-05:00\n 1\n 0\n 10\n \n http://arxiv.org/abs/math/9501234v1\n 1995-01-23T00:00:00Z\n 1995-01-23T00:00:00Z\n Aztec diamonds, checkerboard graphs, and spanning trees\n This note derives the characteristic polynomial of a graph that represents\nnonjump moves in a generalized game of checkers. The number of spanning trees\nis also determined.\n\n \n Donald E. Knuth\n \n J. Algebraic Combin. 6 (1997), no. 3, 253--257\n \n \n \n \n \n\n", 200, null ], [ [ "https://www.ottobib.com/isbn/978-0822324669/bibtex" ], { "headers": null }, "\n\n\n\n \n \n \n \n \n \n \n \n\n \n\n Bibliography and Works Cited Generator for MLA, APA, Wikipedia and Bibtex - OttoBib.com \n \n \n\n \n \n \n \n \n \n \n \n \n \n \n
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  3. I strive for accuracy of the citations but you should treat this tool as a starting point in your works cited, because you still need to look it over.
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  3. I strive for accuracy of the citations but you should treat this tool as a starting point in your works cited, because you still need to look it over.
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OttoBib

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Make a bibliography or works cited with just an ISBN. It's free, easy and FAST

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No Results for 9999999999999
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\n Enter ISBN of book(s) - separate with commas (,)\n

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