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Affiner la rechercheAbad, Enrique. Energy Level Alignment and Electron Transport Through Metal/Organic Contacts
Titre de série : Abad, Enrique Titre : Energy Level Alignment and Electron Transport Through Metal/Organic Contacts : From Interfaces to Molecular Electronics Type de document : texte imprimé Editeur : london:springer Année de publication : 2013 Collection : springer theses Présentation : 198p Format : 16*24cm ISBN/ISSN/EAN : 978-3-642-30906-9 Prix : 119,99 € Langues : Anglais (eng) Mots-clés : Energy Electron Organic Contacts Abad, Enrique. Energy Level Alignment and Electron Transport Through Metal/Organic Contacts : From Interfaces to Molecular Electronics [texte imprimé] . - [S.l.] : london:springer, 2013 . - : 198p ; 16*24cm. - (springer theses) .
ISBN : 978-3-642-30906-9 : 119,99 €
Langues : Anglais (eng)
Mots-clés : Energy Electron Organic Contacts Exemplaires
Code-barres Cote Support Localisation Section Disponibilité BC2014/4173-6 547.2 ABA Ouvrage Bibliothèque de la Faculté des Sciences Exactes et Informatique Physique Disponible BC2014/4173-7 547.2 ABA Ouvrage Bibliothèque de la Faculté des Sciences Exactes et Informatique Physique Disponible BC2014/4173-5 547.2 ABA Ouvrage Bibliothèque de la Faculté des Sciences Exactes et Informatique Physique Disponible BC2014/4173-4 547.2 ABA Ouvrage Bibliothèque de la Faculté des Sciences Exactes et Informatique Physique Exclu du prêt BC2014/4173-1 BC.05-07-060 Ouvrage Bibliothèque Universitaire Centrale Physique Exclu du prêt BC2014/4173-3 BC.05-07-060 Ouvrage Bibliothèque Universitaire Centrale Physique Disponible BC2014/4173-2 BC.05-07-060 Ouvrage Bibliothèque Universitaire Centrale Physique Disponible Advanced Statistical Methods for Astrophysical Probes of Cosmology / March, Marisa Cristina
Titre : Advanced Statistical Methods for Astrophysical Probes of Cosmology Type de document : texte imprimé Auteurs : March, Marisa Cristina Editeur : london:springer Année de publication : 2013 Collection : springer theses Importance : 177 p Présentation : couv. ill. Format : 24 cm ISBN/ISSN/EAN : 978-3-642-35059-7 Langues : Anglais (eng) Mots-clés : Statistical Methods Astrophysical Probes of Cosmology Résumé : This thesis explores advanced Bayesian statistical methods for extracting key information for cosmological model selection, parameter inference and forecasting from astrophysical observations. Bayesian model selection provides a measure of how good models in a set are relative to each other - but what if the best model is missing and not included in the set? Bayesian Doubt is an approach which addresses this problem and seeks to deliver an absolute rather than a relative measure of how good a model is. Supernovae type Ia were the first astrophysical observations to indicate the late time acceleration of the Universe - this work presents a detailed Bayesian Hierarchical Model to infer the cosmological parameters (in particular dark energy) from observations of these supernovae type Ia. Note de contenu : Index, Advanced Statistical Methods for Astrophysical Probes of Cosmology [texte imprimé] / March, Marisa Cristina . - [S.l.] : london:springer, 2013 . - 177 p : couv. ill. ; 24 cm. - (springer theses) .
ISBN : 978-3-642-35059-7
Langues : Anglais (eng)
Mots-clés : Statistical Methods Astrophysical Probes of Cosmology Résumé : This thesis explores advanced Bayesian statistical methods for extracting key information for cosmological model selection, parameter inference and forecasting from astrophysical observations. Bayesian model selection provides a measure of how good models in a set are relative to each other - but what if the best model is missing and not included in the set? Bayesian Doubt is an approach which addresses this problem and seeks to deliver an absolute rather than a relative measure of how good a model is. Supernovae type Ia were the first astrophysical observations to indicate the late time acceleration of the Universe - this work presents a detailed Bayesian Hierarchical Model to infer the cosmological parameters (in particular dark energy) from observations of these supernovae type Ia. Note de contenu : Index, Exemplaires
Code-barres Cote Support Localisation Section Disponibilité BC2014/4107-7 523.1 MAR Ouvrage Bibliothèque de la Faculté des Sciences Exactes et Informatique Physique Disponible BC2014/4107-6 523.1 MAR Ouvrage Bibliothèque de la Faculté des Sciences Exactes et Informatique Physique Disponible BC2014/4107-5 523.1 MAR Ouvrage Bibliothèque de la Faculté des Sciences Exactes et Informatique Physique Disponible BC2014/4107-4 523.1 MAR Ouvrage Bibliothèque de la Faculté des Sciences Exactes et Informatique Physique Exclu du prêt BC2014/4107-2 BC.05-07-066 Ouvrage Bibliothèque Universitaire Centrale Physique Disponible BC2014/4107-1 BC.05-07-066 Ouvrage Bibliothèque Universitaire Centrale Physique Exclu du prêt BC2014/4107-3 BC.05-07-066 Ouvrage Bibliothèque Universitaire Centrale Physique Disponible Theory of Bilayer Graphene Spectroscopy / Marcin Mucha-KruczyÅ„ski
Titre : Theory of Bilayer Graphene Spectroscopy Type de document : texte imprimé Auteurs : Marcin Mucha-Kruczyński Editeur : london:springer Année de publication : 2014 Collection : springer theses Importance : 96 pages Présentation : ill Format : 15.49 x 23.5 cm ISBN/ISSN/EAN : 978-3-642-30935-9 Langues : Anglais moyen (ca.1100-1500) (enm) Mots-clés : Graphene Spectroscopy Résumé : This thesis presents the theory of three key elements of optical spectroscopy of the electronic excitations in bilayer graphene: angle-resolved photoemission spectroscopy (ARPES), visible range Raman spectroscopy, and far-infrared (FIR) magneto-spectroscopy. Bilayer graphene (BLG) is an atomic two-dimensional crystal consisting of two honeycomb monolayers of carbon, arranged according to Bernal stacking. The unperturbed BLG has a unique band structure, which features chiral states of electrons with a characteristic Berry...
Theory of Bilayer Graphene Spectroscopy [texte imprimé] / Marcin Mucha-Kruczyński . - [S.l.] : london:springer, 2014 . - 96 pages : ill ; 15.49 x 23.5 cm. - (springer theses) .
ISBN : 978-3-642-30935-9
Langues : Anglais moyen (ca.1100-1500) (enm)
Mots-clés : Graphene Spectroscopy Résumé : This thesis presents the theory of three key elements of optical spectroscopy of the electronic excitations in bilayer graphene: angle-resolved photoemission spectroscopy (ARPES), visible range Raman spectroscopy, and far-infrared (FIR) magneto-spectroscopy. Bilayer graphene (BLG) is an atomic two-dimensional crystal consisting of two honeycomb monolayers of carbon, arranged according to Bernal stacking. The unperturbed BLG has a unique band structure, which features chiral states of electrons with a characteristic Berry...
Exemplaires
Code-barres Cote Support Localisation Section Disponibilité BC2014/4466-1 BC.05-10-011 Ouvrage Bibliothèque Universitaire Centrale Physique Exclu du prêt BC2014/4466-2 BC.05-10-011 Ouvrage Bibliothèque Universitaire Centrale Physique Disponible BC2014/4466-3 BC.05-10-011 Ouvrage Bibliothèque Universitaire Centrale Physique Disponible The Black Hole-Neutron Star Binary Merger in Full General Relativity / Koutarou, Kyutoku
Titre : The Black Hole-Neutron Star Binary Merger in Full General Relativity : Dependence on Neutron Star Equations of State Type de document : texte imprimé Auteurs : Koutarou, Kyutoku Editeur : london:springer Année de publication : 2013 Collection : springer theses Importance : 194p Présentation : ill Format : 15.5 x 24 cm ISBN/ISSN/EAN : 978-4-431-54200-1 Note générale : index Langues : Français (fre) Résumé : This thesis presents a systematic study of the orbital evolution, gravitational wave radiation, and merger remnant of the black hole–neutron star binary merger in full general relativity for the first time. Numerical-relativity simulations are performed using an adaptive mesh refinement code, SimulAtor for Compact objects in Relativistic Astrophysics (SACRA), which adopts a wide variety of zero-temperature equations of state for the neutron star matter.
Gravitational waves provide us with quantitative information on the neutron star compactness and equation of state via the cutoff frequency in the spectra, if tidal disruption of the neutron star occurs before the binary merges. The cutoff frequency will be observed by next-generation laser interferometric ground-based gravitational wave detectors, such as Advanced LIGO, Advanced VIRGO, and KAGRA.
The author has also determined that the mass of remnant disks are sufficient for the remnant black hole accretion disk to become a progenitor of short-hard gamma ray bursts accompanied by tidal disruptions and suggests that overspinning black holes may not be formed after the merger of even an extremely spinning black hole and an irrotational neutron star.The Black Hole-Neutron Star Binary Merger in Full General Relativity : Dependence on Neutron Star Equations of State [texte imprimé] / Koutarou, Kyutoku . - [S.l.] : london:springer, 2013 . - 194p : ill ; 15.5 x 24 cm. - (springer theses) .
ISBN : 978-4-431-54200-1
index
Langues : Français (fre)
Résumé : This thesis presents a systematic study of the orbital evolution, gravitational wave radiation, and merger remnant of the black hole–neutron star binary merger in full general relativity for the first time. Numerical-relativity simulations are performed using an adaptive mesh refinement code, SimulAtor for Compact objects in Relativistic Astrophysics (SACRA), which adopts a wide variety of zero-temperature equations of state for the neutron star matter.
Gravitational waves provide us with quantitative information on the neutron star compactness and equation of state via the cutoff frequency in the spectra, if tidal disruption of the neutron star occurs before the binary merges. The cutoff frequency will be observed by next-generation laser interferometric ground-based gravitational wave detectors, such as Advanced LIGO, Advanced VIRGO, and KAGRA.
The author has also determined that the mass of remnant disks are sufficient for the remnant black hole accretion disk to become a progenitor of short-hard gamma ray bursts accompanied by tidal disruptions and suggests that overspinning black holes may not be formed after the merger of even an extremely spinning black hole and an irrotational neutron star.Exemplaires
Code-barres Cote Support Localisation Section Disponibilité BC2014/4461-1 BC.05-10-021 Ouvrage Bibliothèque Universitaire Centrale Physique Exclu du prêt BC2014/4461-2 BC.05-10-021 Ouvrage Bibliothèque Universitaire Centrale Physique Disponible BC2014/4461-3 BC.05-10-021 Ouvrage Bibliothèque Universitaire Centrale Physique Disponible Dirac Spectra in Dense QCD / Kanazawa, Takuya
Titre : Dirac Spectra in Dense QCD Type de document : texte imprimé Auteurs : Kanazawa, Takuya, Auteur Editeur : london:springer Année de publication : 2013 Collection : springer theses Importance : 136p Présentation : ill Format : 15.5 x 24 cm ISBN/ISSN/EAN : 978-4-431-54164-6 Langues : Français (fre) Résumé : This book reviews dense quark matter in QCD with gauge group SU(2) using low-energy effective theoretical methods, and connections of statistical properties of the Dirac operator spectrum at high baryon chemical potential and a class of random matrix theories. Dirac Spectra in Dense QCD [texte imprimé] / Kanazawa, Takuya, Auteur . - [S.l.] : london:springer, 2013 . - 136p : ill ; 15.5 x 24 cm. - (springer theses) .
ISBN : 978-4-431-54164-6
Langues : Français (fre)
Résumé : This book reviews dense quark matter in QCD with gauge group SU(2) using low-energy effective theoretical methods, and connections of statistical properties of the Dirac operator spectrum at high baryon chemical potential and a class of random matrix theories. Exemplaires
Code-barres Cote Support Localisation Section Disponibilité BC2014/4156-3 BC.05-09-018 Ouvrage Bibliothèque Universitaire Centrale Physique Disponible BC2014/4156-1 BC.05-09-018 Ouvrage Bibliothèque Universitaire Centrale Physique Disponible BC2014/4156-2 BC.05-09-018 Ouvrage Bibliothèque Universitaire Centrale Physique Disponible