Hochschulschrift

Neutrino Flavor Conversions in High-Density Astrophysical andCosmological Environments

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Alternative title: Umwandlungen der Neutrinoflavors in astrophysikalischen undkosmologischen Umgebungen hoher Dichte

Location: Deutsche Nationalbibliothek Frankfurt am Main

Extent: Online-Ressource

Language: Englisch

Notes: Hamburg, Universität Hamburg, Diss., 2013 und Università degli Studi di Napoli "Federico II", Diss., 2013

Event: Veröffentlichung

(where): Hamburg

(who): Staats- und Universitätsbibliothek Hamburg

(when): 2014

Creator: Saviano, Ninetta

Contributor: Mirizzi, Alessandro

URN: urn:nbn:de:gbv:18-66932

Rights: Der Zugriff auf das Objekt ist unbeschränkt möglich.

Last update: 25.03.2025, 1:46 PM CET

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Object type

Hochschulschrift

Associated

Saviano, Ninetta
Mirizzi, Alessandro
Staats- und Universitätsbibliothek Hamburg

Time of origin

2014

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Neutrino flavor conversions in high-density astrophysical and cosmological environments

Cosmological and Astrophysical Tests of Constructive Gravity

Fast Neutrino Flavor Conversions in Core-Collapse Supernova Simulations

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Neutrino Flavor Conversions in High-Density Astrophysical andCosmological Environments

Object Details

Contributors, Places and Time

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Object type

Associated

Time of origin

Other Objects (12)

Neutrino flavor conversions in high-density astrophysical and cosmological environments

Cosmological and Astrophysical Tests of Constructive Gravity

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CONVERSIONS

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[Autres Conversions Illustres]

FLAVOR

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Astrophysical concepts

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11. Obstacles aux conversions

Neutrino flavor conversions in high-density astrophysical and cosmological environments

Cosmological and Astrophysical Tests of Constructive Gravity

Fast Neutrino Flavor Conversions in Core-Collapse Supernova Simulations

CONVERSIONS

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[Autres Conversions Illustres]

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11. Obstacles aux conversions

Neutrino flavor conversions in high-density astrophysical and cosmological environments

Cosmological and Astrophysical Tests of Constructive Gravity

Fast Neutrino Flavor Conversions in Core-Collapse Supernova Simulations

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[Autres Conversions Illustres]

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