The cosmic evolution of the IMF under the Jeans conjecture with implications for massive galaxies

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dc.contributor.authorNarayanan, Desika
dc.contributor.authorDave, Romeel
dc.date.accessioned2017-07-24T07:55:09Z
dc.date.available2017-07-24T07:55:09Z
dc.date.issued2013
dc.description.abstractWe examine the cosmic evolution of a stellar initial mass function (IMF) in galaxies that varies with the Jeans mass in the interstellar medium, paying particular attention to the K-band stellar mass-to-light ratio (M/LK) of present-epoch massive galaxies. We calculate the typical Jeans mass using high-resolution hydrodynamic simulations coupled with a fully radiative model for the interstellar medium (ISM), which yields a parametrization of the IMF characteristic mass as a function of galaxy star formation rate (SFR).We then calculate the star formation histories of galaxies utilizing an equilibrium galaxy growth model coupled with constraints on the star formation histories set by abundance matching models. We find that at early times, energetic coupling between dust and gas drives warm conditions in the ISM, yielding bottom-light/topheavy IMFs associated with large ISM Jeans masses for massive star-forming galaxies. Owing to the remnants of massive stars that formed during the top-heavy phases at early times, the resultant M/LK(σ) in massive galaxies at the present epoch is increased relative to the nonvarying IMF case. At late times, lower cosmic ray fluxes allow for cooler ISM temperatures in massive galaxies, and hence newly formed clusters will exhibit bottom-heavy IMFs, further increasing M/LK(σ). Our central result is hence that a given massive galaxy may go through both top-heavy and bottom-heavy IMF phases during its lifetime, though the bulk of the stars form during a top-heavy phase. Qualitatively, the variations in M/LK(σ) with galaxy mass are in agreement with observations; however, our model may not be able to account for bottom-heavy mass functions as indicated by stellar absorption features.en_US
dc.description.accreditationDepartment of HE and Training approved list
dc.identifier.citationNarayanan, D. & Dave, R. (2013). The cosmic evolution of the IMF under the Jeans conjecture with implications for massive galaxies. Monthly Notices of the Royal Astronomical Society, 436: 2892–2906en_US
dc.identifier.issn0035-8711
dc.identifier.urihttp://hdl.handle.net/10566/3096
dc.language.isoenen_US
dc.publisherOxford University Pressen_US
dc.rightsPublisher retains copyright. Authors may archive the published version in their institutional repository.
dc.source.urihttp://dx.doi.org/10.1093/mnras/stt1548
dc.subjectStarsen_US
dc.subjectFormation – starsen_US
dc.subjectLuminosity functionen_US
dc.subjectMass function – galaxiesen_US
dc.subjectFormation – galaxiesen_US
dc.subjectHigh-redshift – galaxiesen_US
dc.subjectISM– galaxiesen_US
dc.subjectStarburst – cosmologyen_US
dc.subjectTheoryen_US
dc.titleThe cosmic evolution of the IMF under the Jeans conjecture with implications for massive galaxiesen_US
dc.typeArticleen_US

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