Kernel density estimation of three-parameter Weibull distribution with neural network and genetic algorithm
• The initial estimations were obtained by the RRM and GM(1,1). • The proposed way to deal with the estimation problem was an optimization problem. • Neural network was adopted as approximate model based on the samples. • GA was selected for optimization method based on the neural network model....
Ausführliche Beschreibung
Autor*in: |
Yang, Fan [verfasserIn] |
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E-Artikel |
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Sprache: |
Englisch |
Erschienen: |
2014 |
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Systematik: |
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Umfang: |
12 |
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Übergeordnetes Werk: |
Enthalten in: Geodesic synchrotron radiation in black hole spacetimes: Analytical investigation - Moreira, Zeus S. ELSEVIER, 2021, New York, NY |
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Übergeordnetes Werk: |
volume:247 ; year:2014 ; day:15 ; month:11 ; pages:803-814 ; extent:12 |
Links: |
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DOI / URN: |
10.1016/j.amc.2014.09.065 |
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Katalog-ID: |
ELV017227054 |
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10.1016/j.amc.2014.09.065 doi GBVA2014002000005.pica (DE-627)ELV017227054 (ELSEVIER)S0096-3003(14)01290-9 DE-627 ger DE-627 rakwb eng 510 510 DE-600 530 VZ UA 1000 VZ rvk (DE-625)rvk/145215: 33.40 bkl 33.50 bkl 39.22 bkl Yang, Fan verfasserin aut Kernel density estimation of three-parameter Weibull distribution with neural network and genetic algorithm 2014 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier • The initial estimations were obtained by the RRM and GM(1,1). • The proposed way to deal with the estimation problem was an optimization problem. • Neural network was adopted as approximate model based on the samples. • GA was selected for optimization method based on the neural network model. Optimization algorithm Elsevier Genetic algorithm Elsevier Grey model Elsevier Weibull distribution Elsevier Maximum likelihood method Elsevier Neural network model Elsevier Yue, Zhufeng oth Enthalten in Elsevier Moreira, Zeus S. ELSEVIER Geodesic synchrotron radiation in black hole spacetimes: Analytical investigation 2021 New York, NY (DE-627)ELV006733727 volume:247 year:2014 day:15 month:11 pages:803-814 extent:12 https://doi.org/10.1016/j.amc.2014.09.065 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHY SSG-OPC-AST UA 1000 Referateblätter und Zeitschriften Physik Referateblätter und Zeitschriften (DE-625)rvk/145215: (DE-576)329175343 33.40 Kernphysik VZ 33.50 Physik der Elementarteilchen und Felder: Allgemeines VZ 39.22 Astrophysik VZ AR 247 2014 15 1115 803-814 12 045F 510 |
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10.1016/j.amc.2014.09.065 doi GBVA2014002000005.pica (DE-627)ELV017227054 (ELSEVIER)S0096-3003(14)01290-9 DE-627 ger DE-627 rakwb eng 510 510 DE-600 530 VZ UA 1000 VZ rvk (DE-625)rvk/145215: 33.40 bkl 33.50 bkl 39.22 bkl Yang, Fan verfasserin aut Kernel density estimation of three-parameter Weibull distribution with neural network and genetic algorithm 2014 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier • The initial estimations were obtained by the RRM and GM(1,1). • The proposed way to deal with the estimation problem was an optimization problem. • Neural network was adopted as approximate model based on the samples. • GA was selected for optimization method based on the neural network model. Optimization algorithm Elsevier Genetic algorithm Elsevier Grey model Elsevier Weibull distribution Elsevier Maximum likelihood method Elsevier Neural network model Elsevier Yue, Zhufeng oth Enthalten in Elsevier Moreira, Zeus S. ELSEVIER Geodesic synchrotron radiation in black hole spacetimes: Analytical investigation 2021 New York, NY (DE-627)ELV006733727 volume:247 year:2014 day:15 month:11 pages:803-814 extent:12 https://doi.org/10.1016/j.amc.2014.09.065 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHY SSG-OPC-AST UA 1000 Referateblätter und Zeitschriften Physik Referateblätter und Zeitschriften (DE-625)rvk/145215: (DE-576)329175343 33.40 Kernphysik VZ 33.50 Physik der Elementarteilchen und Felder: Allgemeines VZ 39.22 Astrophysik VZ AR 247 2014 15 1115 803-814 12 045F 510 |
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10.1016/j.amc.2014.09.065 doi GBVA2014002000005.pica (DE-627)ELV017227054 (ELSEVIER)S0096-3003(14)01290-9 DE-627 ger DE-627 rakwb eng 510 510 DE-600 530 VZ UA 1000 VZ rvk (DE-625)rvk/145215: 33.40 bkl 33.50 bkl 39.22 bkl Yang, Fan verfasserin aut Kernel density estimation of three-parameter Weibull distribution with neural network and genetic algorithm 2014 12 nicht spezifiziert zzz rdacontent nicht spezifiziert z rdamedia nicht spezifiziert zu rdacarrier • The initial estimations were obtained by the RRM and GM(1,1). • The proposed way to deal with the estimation problem was an optimization problem. • Neural network was adopted as approximate model based on the samples. • GA was selected for optimization method based on the neural network model. Optimization algorithm Elsevier Genetic algorithm Elsevier Grey model Elsevier Weibull distribution Elsevier Maximum likelihood method Elsevier Neural network model Elsevier Yue, Zhufeng oth Enthalten in Elsevier Moreira, Zeus S. ELSEVIER Geodesic synchrotron radiation in black hole spacetimes: Analytical investigation 2021 New York, NY (DE-627)ELV006733727 volume:247 year:2014 day:15 month:11 pages:803-814 extent:12 https://doi.org/10.1016/j.amc.2014.09.065 Volltext GBV_USEFLAG_U GBV_ELV SYSFLAG_U SSG-OLC-PHY SSG-OPC-AST UA 1000 Referateblätter und Zeitschriften Physik Referateblätter und Zeitschriften (DE-625)rvk/145215: (DE-576)329175343 33.40 Kernphysik VZ 33.50 Physik der Elementarteilchen und Felder: Allgemeines VZ 39.22 Astrophysik VZ AR 247 2014 15 1115 803-814 12 045F 510 |
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• The initial estimations were obtained by the RRM and GM(1,1). • The proposed way to deal with the estimation problem was an optimization problem. • Neural network was adopted as approximate model based on the samples. • GA was selected for optimization method based on the neural network model. |
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• The initial estimations were obtained by the RRM and GM(1,1). • The proposed way to deal with the estimation problem was an optimization problem. • Neural network was adopted as approximate model based on the samples. • GA was selected for optimization method based on the neural network model. |
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• The initial estimations were obtained by the RRM and GM(1,1). • The proposed way to deal with the estimation problem was an optimization problem. • Neural network was adopted as approximate model based on the samples. • GA was selected for optimization method based on the neural network model. |
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title_short |
Kernel density estimation of three-parameter Weibull distribution with neural network and genetic algorithm |
url |
https://doi.org/10.1016/j.amc.2014.09.065 |
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Yue, Zhufeng |
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10.1016/j.amc.2014.09.065 |
up_date |
2024-07-06T21:27:44.243Z |
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