Comparison of predictions from alternative cosmologies with Cosmic Microwave Background data
- Autores
- Piccirilli, María Pía; León, Gabriel; Landau, Susana Judith
- Año de publicación
- 2014
- Idioma
- inglés
- Tipo de recurso
- documento de conferencia
- Estado
- versión publicada
- Descripción
- The emergence of the seeds of cosmic structure from a perfect isotropic and homogeneous Universe has not been clearly explained by the standard version of inflationary models. We consider alternative scenarios where the emergence of an anisotropic and inhomogeneous Universe from an initial isotropic and homogeneous state can be explained by the of introduction the “self-induced collapse hypothesis”, a scheme in which an internally induced collapse of the wave function of the inflaton field is the mechanism by which inhomogeneities and anisotropies arise at each particular length scale. Our aim is to test these models through statistical analysis comparing them with recent data of the Cosmic Microwave Background and galaxy surveys. This procedure will restrict the value of free parameters and test the viability of each scheme using the results of latest observational experiments.
Facultad de Ciencias Astronómicas y Geofísicas - Materia
-
Ciencias Astronómicas
alternative scenarios
inflaton field
statistical analysis - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- http://creativecommons.org/licenses/by-nc-sa/4.0/
- Repositorio
.jpg)
- Institución
- Universidad Nacional de La Plata
- OAI Identificador
- oai:sedici.unlp.edu.ar:10915/165270
Ver los metadatos del registro completo
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Comparison of predictions from alternative cosmologies with Cosmic Microwave Background dataPiccirilli, María PíaLeón, GabrielLandau, Susana JudithCiencias Astronómicasalternative scenariosinflaton fieldstatistical analysisThe emergence of the seeds of cosmic structure from a perfect isotropic and homogeneous Universe has not been clearly explained by the standard version of inflationary models. We consider alternative scenarios where the emergence of an anisotropic and inhomogeneous Universe from an initial isotropic and homogeneous state can be explained by the of introduction the “self-induced collapse hypothesis”, a scheme in which an internally induced collapse of the wave function of the inflaton field is the mechanism by which inhomogeneities and anisotropies arise at each particular length scale. Our aim is to test these models through statistical analysis comparing them with recent data of the Cosmic Microwave Background and galaxy surveys. This procedure will restrict the value of free parameters and test the viability of each scheme using the results of latest observational experiments.Facultad de Ciencias Astronómicas y Geofísicas2014-04info:eu-repo/semantics/conferenceObjectinfo:eu-repo/semantics/publishedVersionObjeto de conferenciahttp://purl.org/coar/resource_type/c_5794info:ar-repo/semantics/documentoDeConferenciaapplication/pdf215-218http://sedici.unlp.edu.ar/handle/10915/165270enginfo:eu-repo/semantics/altIdentifier/isbn/978-987-24948-2-7info:eu-repo/semantics/openAccesshttp://creativecommons.org/licenses/by-nc-sa/4.0/Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0)reponame:SEDICI (UNLP)instname:Universidad Nacional de La Platainstacron:UNLP2026-04-08T10:32:01Zoai:sedici.unlp.edu.ar:10915/165270Institucionalhttp://sedici.unlp.edu.ar/Universidad públicaNo correspondehttp://sedici.unlp.edu.ar/oai/snrdalira@sedici.unlp.edu.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:13292026-04-08 10:32:01.547SEDICI (UNLP) - Universidad Nacional de La Platafalse |
| dc.title.none.fl_str_mv |
Comparison of predictions from alternative cosmologies with Cosmic Microwave Background data |
| title |
Comparison of predictions from alternative cosmologies with Cosmic Microwave Background data |
| spellingShingle |
Comparison of predictions from alternative cosmologies with Cosmic Microwave Background data Piccirilli, María Pía Ciencias Astronómicas alternative scenarios inflaton field statistical analysis |
| title_short |
Comparison of predictions from alternative cosmologies with Cosmic Microwave Background data |
| title_full |
Comparison of predictions from alternative cosmologies with Cosmic Microwave Background data |
| title_fullStr |
Comparison of predictions from alternative cosmologies with Cosmic Microwave Background data |
| title_full_unstemmed |
Comparison of predictions from alternative cosmologies with Cosmic Microwave Background data |
| title_sort |
Comparison of predictions from alternative cosmologies with Cosmic Microwave Background data |
| dc.creator.none.fl_str_mv |
Piccirilli, María Pía León, Gabriel Landau, Susana Judith |
| author |
Piccirilli, María Pía |
| author_facet |
Piccirilli, María Pía León, Gabriel Landau, Susana Judith |
| author_role |
author |
| author2 |
León, Gabriel Landau, Susana Judith |
| author2_role |
author author |
| dc.subject.none.fl_str_mv |
Ciencias Astronómicas alternative scenarios inflaton field statistical analysis |
| topic |
Ciencias Astronómicas alternative scenarios inflaton field statistical analysis |
| dc.description.none.fl_txt_mv |
The emergence of the seeds of cosmic structure from a perfect isotropic and homogeneous Universe has not been clearly explained by the standard version of inflationary models. We consider alternative scenarios where the emergence of an anisotropic and inhomogeneous Universe from an initial isotropic and homogeneous state can be explained by the of introduction the “self-induced collapse hypothesis”, a scheme in which an internally induced collapse of the wave function of the inflaton field is the mechanism by which inhomogeneities and anisotropies arise at each particular length scale. Our aim is to test these models through statistical analysis comparing them with recent data of the Cosmic Microwave Background and galaxy surveys. This procedure will restrict the value of free parameters and test the viability of each scheme using the results of latest observational experiments. Facultad de Ciencias Astronómicas y Geofísicas |
| description |
The emergence of the seeds of cosmic structure from a perfect isotropic and homogeneous Universe has not been clearly explained by the standard version of inflationary models. We consider alternative scenarios where the emergence of an anisotropic and inhomogeneous Universe from an initial isotropic and homogeneous state can be explained by the of introduction the “self-induced collapse hypothesis”, a scheme in which an internally induced collapse of the wave function of the inflaton field is the mechanism by which inhomogeneities and anisotropies arise at each particular length scale. Our aim is to test these models through statistical analysis comparing them with recent data of the Cosmic Microwave Background and galaxy surveys. This procedure will restrict the value of free parameters and test the viability of each scheme using the results of latest observational experiments. |
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2014 |
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2014-04 |
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info:eu-repo/semantics/conferenceObject info:eu-repo/semantics/publishedVersion Objeto de conferencia http://purl.org/coar/resource_type/c_5794 info:ar-repo/semantics/documentoDeConferencia |
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http://sedici.unlp.edu.ar/handle/10915/165270 |
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eng |
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