Chemical properties of long gamma-ray bursts progenitors in cosmological simulations

In this work, we investigate the chemical dependence of the progenitors of long gamma-ray bursts. Using hydrodynamical cosmological simulations consistent with the concordance Λ-CDM model which include star formation, chemical enrichment and supernova feedback in a self-consistent way, and assuming...

Descripción completa

Guardado en:
Detalles Bibliográficos
Autor principal: Pellizza, L.J
Otros Autores: Artale, M.C, Tissera, P.B
Formato: Acta de conferencia Capítulo de libro
Lenguaje:Inglés
Publicado: Sissa Medialab Srl 2012
Acceso en línea:Registro en Scopus
Handle
Registro en la Biblioteca Digital
Aporte de:Registro referencial: Solicitar el recurso aquí
LEADER 05620caa a22006137a 4500
001 PAPER-23518
003 AR-BaUEN
005 20230518205513.0
008 190411s2012 xx ||||fo|||| 10| 0 eng|d
024 7 |2 scopus  |a 2-s2.0-85052404750 
040 |a Scopus  |b spa  |c AR-BaUEN  |d AR-BaUEN 
100 1 |a Pellizza, L.J. 
245 1 0 |a Chemical properties of long gamma-ray bursts progenitors in cosmological simulations 
260 |b Sissa Medialab Srl  |c 2012 
506 |2 openaire  |e Política editorial 
504 |a Artale, M.C., Pellizza, L.J., Tissera, P.B., Chemical abundances and spatial distribution of long gamma-ray bursts (2011) MNRAS, (415), p. 3417 
504 |a Band, D., Matteson, J., Ford, L., BATSE observations of gamma-ray burst spectra (1993) I - Spectral Diversity ApJ, (413), p. 281 
504 |a Chisari, N.E., Tissera, P.B., Pellizza, L.J., Host galaxies of long gamma-ray bursts in the Millennium Simulation (2011) MNRAS, (408), p. 647 
504 |a Daigné, F., Rossi, E.M., Mochkovitch, R., The redshift distribution of Swift gamma-ray bursts: Evidence for evolution (2006) MNRAS, 372, p. 1034 
504 |a Elliott, J., Greiner, J., Khochfar, S., Schady, P., Johnson, J.L., Rau, A., The long γ-ray burst rate and the correlation with host galaxy properties (2012) A&A, (539), p. 113 
504 |a Hopkins, A.M., Beacom, J.F., On the Normalization of the Cosmic Star Formation History (2006) ApJ, (651), p. 142 
504 |a Nuza, S.E., Tissera, P.B., Pellizza, L.J., The host galaxies of long-duration gamma-ray bursts in a cosmological hierarchical scenario (2007) MNRAS, 375, p. 665 
504 |a Pellizza, L., Nuza, S., Tissera, P., (2008) Proceedings of The First La Plata International School: “Compact Objects and Their Emission, p. 109. , G.E. Romero & I. Andruchow 
504 |a Porciani, C., Madau, P., On the Association of Gamma-Ray Bursts with Massive Stars: Implications for Number Counts and Lensing Statistics (2001) ApJ, (548), p. 522. , astro-ph/0008294 
504 |a Salvaterra, R., Chincarini, G., The Gamma Ray Burst Luminosity Function in the Light of the Swift 2-year Data (2007) ApJ, (656), p. 49. , astro-ph/0612278 
504 |a Scannapieco, C., Tissera, P.B., White, S., Springel, V., Feedback and metal enrichment in cosmological smoothed particle hydrodynamics simulations - I. A model for chemical enrichment (2005) MNRAS, 364, p. 552. , astro-ph/0505440v5 
504 |a Scannapieco, C., Tissera, P.B., White, S., Springel, V., Feedback and metal enrichment in cosmological SPH simulations - II. A multiphase model with supernova energy feedback (2006) MNRAS, 371, p. 1125 
504 |a Stern, B., Tikhomirova, Y., Kompaneets, D., An Off-Line Scan of the BATSE Daily Records and a Large Uniform Sample of Gamma-Ray Bursts (2001) ApJ, (563), p. 80. , astro-ph/0009447 
504 |a Vedrenne, G., Atteia, J., Gamma-Ray Bursts: The Brigthest Explosions in The Universe, , Springer Praxis Books, Jointly published with Praxis Publishing, UK 
520 3 |a In this work, we investigate the chemical dependence of the progenitors of long gamma-ray bursts. Using hydrodynamical cosmological simulations consistent with the concordance Λ-CDM model which include star formation, chemical enrichment and supernova feedback in a self-consistent way, and assuming that these bursts are produced by a subset of massive stars (possibly with distinct chemical properties), we compute the LGRB rate at different redshifts. Introducing prescriptions for their peak isotropic luminosity function and intrinsic spectrum, and using a Monte Carlo scheme to model their detectability by different high-energy observatories, we compute the distributions of the burst observables (peak flux, spectral peak energy) and compare them to actual data. Our preliminary results show that a possible chemical dependence for LGRBs progenitors cannot be ruled out, but it might be more complex than the usually assumed metallicity cut-off. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-ShareAlike Licence.  |l eng 
593 |a Instituto de Astronomía y Física del Espacio, Buenos Aires, Argentina 
593 |a Consejo Nacional de Investigaciones Cientícas y Técnicas, Argentina 
593 |a Max Planck Institute for Astrophysics, Germany 
690 1 0 |a CHEMICAL PROPERTIES 
690 1 0 |a STARS 
690 1 0 |a ENERGY OBSERVATORY 
690 1 0 |a GAMMA RAY BURSTS 
690 1 0 |a LUMINOSITY FUNCTIONS 
690 1 0 |a MASSIVE STARS 
690 1 0 |a METALLICITIES 
690 1 0 |a MONTE CARLO SCHEMES 
690 1 0 |a SPECTRAL PEAK ENERGIES 
690 1 0 |a STAR FORMATIONS 
690 1 0 |a GAMMA RAYS 
700 1 |a Artale, M.C. 
700 1 |a Tissera, P.B. 
711 2 |d 7 May 2012 through 11 May 2012  |g Código de la conferencia: 138611 
773 0 |d Sissa Medialab Srl, 2012  |g v. 2012-May  |p Proc. Sci.  |n Proceedings of Science  |x 18248039  |w (AR-BaUEN)CENRE-7670  |t 2012 Gamma-Ray Bursts Conference, GRB 2012 
856 4 1 |u https://www.scopus.com/inward/record.uri?eid=2-s2.0-85052404750&partnerID=40&md5=bf6d8a50f288e5f3be9f8bf2b6335411  |y Registro en Scopus 
856 4 0 |u https://hdl.handle.net/20.500.12110/paper_18248039_v2012-May_n_p_Pellizza  |y Handle 
856 4 0 |u https://bibliotecadigital.exactas.uba.ar/collection/paper/document/paper_18248039_v2012-May_n_p_Pellizza  |y Registro en la Biblioteca Digital 
961 |a paper_18248039_v2012-May_n_p_Pellizza  |b paper  |c PE 
962 |a info:eu-repo/semantics/conferenceObject  |a info:ar-repo/semantics/documento de conferencia  |b info:eu-repo/semantics/publishedVersion 
999 |c 84471