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(Referência obtida automaticamente do Web of Science, por meio da informação sobre o financiamento pela FAPESP e o número do processo correspondente, incluída na publicação pelos autores.)

Probing the distance-duality relation with high-z data

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Autor(es):
Holanda, R. F. L. [1, 2, 3] ; Busti, V. C. [4, 5] ; Lima, F. S. [3] ; Alcaniz, J. S. [6]
Número total de Autores: 4
Afiliação do(s) autor(es):
[1] Univ Fed Rio Grande do Norte, Dept Fis, BR-59072970 Natal, RN - Brazil
[2] Univ Estadual Paraiba, Dept Fis, BR-58429500 Campina Grande, PB - Brazil
[3] Univ Fed Campina Grande, Dept Fis, BR-58429900 Campina Grande, PB - Brazil
[4] Univ Penn, Dept Phys & Astron, Philadelphia, PA 19104 - USA
[5] Univ Sao Paulo, Inst Fis, Dept Fis Matemat, BR-05508090 Sao Paulo, SP - Brazil
[6] Observ Nacl, Dept Astron, BR-20921400 Rio De Janeiro, RJ - Brazil
Número total de Afiliações: 6
Tipo de documento: Artigo Científico
Fonte: Journal of Cosmology and Astroparticle Physics; n. 9 SEP 2017.
Citações Web of Science: 3
Resumo

Measurements of strong gravitational lensing jointly with type Ia supernovae (SNe Ia) observations have been used to test the validity of the cosmic distance duality relation (CDDR), D-L (z) = {[}(1 + z)(2) D-A (z)] = eta = 1, where D-L (z) and D-A (z) are the luminosity and the angular diameter distances to a given redshift z, respectively. However, several lensing systems lie in the interval 1 : 4 <= z <= 3 : 6 i. e., beyond the redshift range of current SNe Ia compilations (z approximate to 1 : 50), which prevents this kind of test to be fully explored. In this paper, we circumvent this problem by testing the CDDR considering observations of strong gravitational lensing along with SNe Ia and a subsample from the latest gamma-ray burst distance modulus data, whose redshift range is 0 : 033 <= z <= 9 : 3. We parameterize their luminosity distances with a second degree polynomial function and search for possible deviations from the CDDR validity by using four di ff erent eta(z) functions: eta(z) = 1 + eta(0) z, eta(z) = 1 + eta(0) z = (1 + z), eta (z) = (1 + z) eta(0) and eta (z) = 1 + eta(0) ln(1 + z). Unlike previous tests done at redshifts lower than 1 : 50, the likelihood for eta(0) depends strongly on the eta (z) function considered, but we fi nd no signi fi cant deviation from the CDDR validity (eta(0) = 0). However, our analyses also point to the fact that caution is needed when one fi ts data in higher redshifts to test the CDDR as well as a better understanding of the mass distribution of lenses also is required for more accurate results. (AU)

Processo FAPESP: 14/21098-1 - Cosmologia de precisão com o Dark Energy Survey
Beneficiário:Vinicius Consolini Busti
Linha de fomento: Bolsas no Brasil - Pós-Doutorado
Processo FAPESP: 16/17271-5 - Aglomerados de galáxias como sondas cosmológicas: calibração da relação massa-riqueza
Beneficiário:Vinicius Consolini Busti
Linha de fomento: Bolsas no Exterior - Estágio de Pesquisa - Pós-Doutorado