CONGRuENTS (COsmic-ray, Neutrino, Gamma-ray and Radio Non-Thermal Spectra). II. Population-level correlations between galactic infrared, radio, and γ-ray emission
arXiv:2310.05693 · doi:10.1093/mnras/stae932
Abstract
Galaxies obey a number of empirical correlations between their radio, γ-ray, and infrared emission, but the physical origins of these correlations remain uncertain. Here we use the CONGRuENTS model for broadband non-thermal emission from star-forming galaxies, which self-consistently calculates energy-dependent transport and non-thermal emission from cosmic ray hadrons and leptons, to predict radio and γ-ray emission for a synthetic galaxy population with properties drawn from a large deep-field survey. We show that our synthetic galaxies reproduce observed relations such as the FIR-radio correlation, the FIR-γ correlation, and the distribution of radio spectral indices, and we use the model to explain the physical origins of these relations. Our results show that the FIR-radio correlation arises because the amount of cosmic ray electron power ultimately radiated as synchrotron emission varies only weakly with galaxy star formation rate as a result of the constraints imposed on gas properties by hydrostatic balance and turbulent dynamo action; the same physics dictates the extent of proton calorimetry in different galaxies, and thus sets the FIR-γ-ray correlation. We further show that galactic radio spectral indices result primarily from competition between thermal free-free emission and energy-dependent loss of cosmic ray electrons to bremsstrahlung and escape into galactic halos, with shaping of the spectrum by inverse Compton, synchrotron, and ionisation processes typically playing a sub-dominant role. In addition to explaining existing observations, we use our analysis to predict a heretofore unseen correlation between the curvature of galaxies' radio spectra and their pion-driven γ-ray emission, a prediction that will be testable with upcoming facilities.
arXiv comment17 pages, 14 figures
References in corpus (51)
- CANDELS: The Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey
- A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
- 3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since
- Radio Properties of Infrared Selected Galaxies in the IRAS 2 Jy Sample
- The lesser role of starbursts for star formation at z=2
- Estimating Star Formation Rates from Infrared and Radio Luminosities: The Origin of the Radio-Infrared Correlation
- Fermi-LAT Observations of the Diffuse Gamma-Ray Emission: Implications for Cosmic Rays and the Interstellar Medium
- Molecular Gas and Star Formation in Nearby Disk Galaxies
- PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions
- Structural Parameters of Galaxies in CANDELS
- GeV Observations of Star-forming Galaxies with \textit{Fermi} LAT
- Global cosmic-ray related luminosity and energy budget of the Milky Way
- The far-infrared/radio correlation as probed by Herschel
- Science with the Cherenkov Telescope Array
- The Physics of the FIR-Radio Correlation: I. Calorimetry, Conspiracy, and Implications
- Magnetic Fields in Starburst Galaxies and The Origin of the FIR-Radio Correlation
- VLA-COSMOS 3GHz Large Project: The infrared-radio correlation of star-forming galaxies and AGN to
- The far-infrared/radio correlation and radio spectral index of galaxies in the SFR-M* plane up to z 2
- On The GeV & TeV Detections of the Starburst Galaxies M82 & NGC 253
- A Universal Neutral Gas Profile for Nearby Disk Galaxies
- Cosmic ray feedback in the FIRE simulations: constraining cosmic ray propagation with GeV gamma ray emission
- Extended Schmidt Law: Role Of Existing Stars In Current Star Formation
- The Starburst Contribution to the Extra-Galactic Gamma-Ray Background
- The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to
- The infrared-radio correlation of star-forming galaxies is strongly M-dependent but nearly redshift-invariant since z4
- A new interpretation of the far-infrared - radio correlation and the expected breakdown at high redshift
- Old and young stellar populations in DustPedia galaxies and their role in dust heating
- No Evolution in the IR-Radio Relation for IR-Luminous Galaxies at z<2 in the COSMOS Field
- The VLA-COSMOS Perspective on the IR-Radio Relation. I. New Constraints on Selection Biases and the Non-Evolution of the IR/Radio Properties of Star Forming and AGN Galaxies at Intermediate and High Redshift
- The -ray Emission of Star-Forming Galaxies
- A physically motivated definition for the size of galaxies in an era of ultra-deep imaging
- The Physics of the FIR-Radio Correlation: II. Synchrotron Emission as a Star-Formation Tracer in High-Redshift Galaxies
- Deep multi-frequency radio imaging in the Lockman Hole using the GMRT and VLA: II. The spectral index of submillimetre galaxies
- Cosmic ray transport in starburst galaxies
- Radio synchrotron spectra of star-forming galaxies
- Calibration of ultraviolet, mid-infrared and radio star formation rate indicators
- The diffuse -ray background is dominated by star-forming galaxies
- Gamma Rays from Cosmic Rays in Supernova Remnants
- Cosmic rays and non-thermal emission in simulated galaxies: III. probing cosmic ray calorimetry with radio spectra and the FIR-radio correlation
- Cosmic rays and non-thermal emission in simulated galaxies. II. -ray maps, spectra and the far infrared--ray relation
- Star-Forming Galaxies Significantly Contribute to the Isotropic Gamma-Ray Background
- What drives the velocity dispersion of ionized gas in star-forming galaxies?
- The gamma-ray / infrared luminosity correlation of star-forming galaxies
- Cosmic rays across the star-forming galaxy sequence. I: Cosmic ray pressures and calorimetry
- Exploring the physics behind the non-thermal emission from star-forming galaxies detected in gamma rays
- Cosmic rays across the star-forming galaxy sequence. II: Stability limits and the onset of cosmic ray-driven outflows
- Gamma-ray emission from the Sagittarius Dwarf Spheroidal galaxy due to millisecond pulsars
- An updated estimate of the cosmic radio background and implications for ultra-high-energy photon propagation
- Millisecond Pulsars Modify the Radio-SFR Correlation in Quiescent Galaxies
- The Andromeda Gamma-Ray Excess: Background Systematics of the Millisecond Pulsars and Dark Matter Interpretations
- CONGRuENTS (COsmic-ray, Neutrino, Gamma-ray and Radio Non-Thermal Spectra). I. A predictive model for galactic non-thermal emission