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Promise of Future Searches for Cosmic Topology.
Akrami, Yashar; Anselmi, Stefano; Copi, Craig J; Eskilt, Johannes R; Jaffe, Andrew H; Kosowsky, Arthur; Petersen, Pip; Starkman, Glenn D; González-Quesada, Kevin; Güngör, Özenç; Mihaylov, Deyan P; Saha, Samanta; Tamosiunas, Andrius; Taylor, Quinn; Vardanyan, Valeri.
Afiliação
  • Akrami Y; CERCA/ISO, Department of Physics, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, Ohio 44106, USA.
  • Anselmi S; Instituto de Física Teórica (IFT) UAM-CSIC, C/ Nicolás Cabrera 13-15, Campus de Cantoblanco UAM, 28049 Madrid, Spain.
  • Copi CJ; Astrophysics Group and Imperial Centre for Inference and Cosmology, Department of Physics, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, United Kingdom.
  • Eskilt JR; Dipartimento di Fisica e Astronomia "G. Galilei," Università degli Studi di Padova, via Marzolo 8, I-35131 Padova, Italy.
  • Jaffe AH; INFN, Sezione di Padova, via Marzolo 8, I-35131 Padova, Italy.
  • Kosowsky A; LUTH, UMR 8102 CNRS, Observatoire de Paris, PSL Research University, Université Paris Diderot, 92190 Meudon, France.
  • Petersen P; CERCA/ISO, Department of Physics, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, Ohio 44106, USA.
  • Starkman GD; Astrophysics Group and Imperial Centre for Inference and Cosmology, Department of Physics, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, United Kingdom.
  • González-Quesada K; Institute of Theoretical Astrophysics, University of Oslo, P.O. Box 1029 Blindern, N-0315 Oslo, Norway.
  • Güngör Ö; Astrophysics Group and Imperial Centre for Inference and Cosmology, Department of Physics, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, United Kingdom.
  • Mihaylov DP; Department of Physics and Astronomy, University of Pittsburgh, Pittsburgh, Pennsylvania 15260, USA.
  • Saha S; CERCA/ISO, Department of Physics, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, Ohio 44106, USA.
  • Tamosiunas A; CERCA/ISO, Department of Physics, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, Ohio 44106, USA.
  • Taylor Q; Astrophysics Group and Imperial Centre for Inference and Cosmology, Department of Physics, Imperial College London, Blackett Laboratory, Prince Consort Road, London SW7 2AZ, United Kingdom.
  • Vardanyan V; CERCA/ISO, Department of Physics, Case Western Reserve University, 10900 Euclid Avenue, Cleveland, Ohio 44106, USA.
Phys Rev Lett ; 132(17): 171501, 2024 Apr 26.
Article em En | MEDLINE | ID: mdl-38728711
ABSTRACT
The shortest distance around the Universe through us is unlikely to be much larger than the horizon diameter if microwave background anomalies are due to cosmic topology. We show that observational constraints from the lack of matched temperature circles in the microwave background leave many possibilities for such topologies. We evaluate the detectability of microwave background multipole correlations for sample cases. Searches for topology signatures in observational data over the large space of possible topologies pose a formidable computational challenge.

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2024 Tipo de documento: Article País de afiliação: Estados Unidos

Texto completo: 1 Coleções: 01-internacional Base de dados: MEDLINE Idioma: En Revista: Phys Rev Lett Ano de publicação: 2024 Tipo de documento: Article País de afiliação: Estados Unidos
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