Prospects for directly detecting the first supernovae, and their impact on early star formation

dc.contributor.advisorBromm, Volkeren
dc.contributor.committeeMemberMilosavljevic, Milosen
dc.contributor.committeeMemberWheeler, J. Craigen
dc.contributor.committeeMemberFinkelstein, Stevenen
dc.contributor.committeeMemberYoshida, Naokien
dc.creatorHummel, Jacob Alexanderen
dc.creator.orcid0000-0001-8423-1225en
dc.date.accessioned2016-08-22T20:55:37Z
dc.date.available2016-08-22T20:55:37Z
dc.date.issued2016-05
dc.date.submittedMay 2016
dc.date.updated2016-08-22T20:55:37Z
dc.description.abstractThe formation of the first stars in the Universe marked a pivotal moment in cosmic history, initiating the transition from the simple initial conditions of the big bang to the complex structures we see today. Ionizing radiation produced by these so-called Population III stars began the process of reionization, and the supernovae marking their deaths initiated the process of chemical enrichment. We assess the prospects for direct detection of the first supernovae should they happen to end their lives as extremely energetic pair-instability supernovae, which should be within the detection limits of the upcoming James Webb Space Telescope. Using a combination of semi-analytic models and cosmological simulations to estimate their source density, we find that the primary obstacle to observing such events is their scarcity, not their faintness. The first supernovae and the compact remnants they leave behind also produce significant amounts of high-energy X-rays and cosmic rays able to travel through the predominantly neutral intergalactic medium and build up a cosmic background. To better understand how these violent explosions impact subsequent episodes of metal-free star formation, we employ ab-initio, cosmological hydrodynamics simulations to model the formation of stars in a minihalo at z = 20-30 under the influence of both an X-ray and cosmic ray background. The presence of an ionizing background---whether X-rays or cosmic rays---serves to expedite the collapse of gas to high densities by enhancing molecular hydrogen cooling, thus allowing stars to form at substantially earlier epochs in strongly irradiated minihalos. The mass of the stars thus formed however appears to be quite robust, maintaining a characteristic mass of order a few tens of solar masses even as the strength of the ionizing background varies by several orders of magnitude. Finally, we describe the novel software developed to enable this research. These tools for manipulating and analyzing simulation data have been released as the open-source GAdget DataFrame Library: gadfly.en
dc.description.departmentAstronomyen
dc.format.mimetypeapplication/pdfen
dc.identifierdoi:10.15781/T2QZ22H6Fen
dc.identifier.urihttp://hdl.handle.net/2152/39579en
dc.language.isoenen
dc.subjectFirst starsen
dc.subjectCosmologyen
dc.subjectStar formationen
dc.subjectSimulationsen
dc.titleProspects for directly detecting the first supernovae, and their impact on early star formationen
dc.typeThesisen
dc.type.materialtexten
thesis.degree.departmentAstronomyen
thesis.degree.disciplineAstronomyen
thesis.degree.grantorThe University of Texas at Austinen
thesis.degree.levelDoctoralen
thesis.degree.nameDoctor of Philosophyen

Access full-text files

Original bundle

Now showing 1 - 1 of 1
Loading...
Thumbnail Image
Name:
HUMMEL-DISSERTATION-2016.pdf
Size:
8.66 MB
Format:
Adobe Portable Document Format

License bundle

Now showing 1 - 1 of 1
No Thumbnail Available
Name:
LICENSE.txt
Size:
1.84 KB
Format:
Plain Text
Description: