activity
20082026
most citedTesting the Hadronuclear Origin of PeV Neutrinos Observed with IceCube

372 citations · 2.1k across the 62 of their papers we have counts for

collaborators
Showing 2013Show all

6 papers · 1 filter

astro-ph.HE2013★ 5 cited

From 10 Kelvin to 10 TeraKelvin: Insights on the Interaction Between Cosmic Rays and Gas in Starbursts

Brian C. Lacki

Recent work has both illuminated and mystified our attempts to understand cosmic rays (CRs) in starburst galaxies. I discuss my new research exploring how CRs interact with the ISM…

astro-ph.CO2013★ 9 cited

Sturm und Drang: Supernova-Driven Turbulence, Magnetic Fields, and Cosmic Rays in the Chaotic Starburst Interstellar Medium

Brian C. Lacki

Frequent supernova explosions in compact starburst regions are a main shaper of these regions' interstellar media (ISM). In most starbursts, the supernova remnants blast open a hot…

astro-ph.HE2013★ 372 cited

Testing the Hadronuclear Origin of PeV Neutrinos Observed with IceCube

Kohta Murase, Markus Ahlers, Brian C. Lacki

We consider implications of the IceCube excess for hadronuclear (pp) scenarios of neutrino sources such as galaxy clusters/groups and star-forming galaxies. Since the observed neut…

astro-ph.CO2013★ 19 cited

The Ultimate Fate of Cosmic Rays from Galaxies and their Role in the Intergalactic Medium

Brian C. Lacki

The majority of cosmic rays (CRs) generated by star-forming galaxies escape them and enter the intergalactic medium (IGM). Galactic wind termination shocks might also accelerate CR…

astro-ph.HE2013★ 80 cited

The Fermi Bubbles as Starburst Wind Termination Shocks

Brian C. Lacki

The enhanced star formation in the inner 100 pc of the Galaxy launches a superwind at ~1600 km s for M82-like parameters. The ram pressure of the wind is very low compared t…

astro-ph.CO2013★ 85 cited

The Equipartition Magnetic Field Formula in Starburst Galaxies: Accounting for Pionic Secondaries and Strong Energy Losses

Brian C. Lacki, Rainer Beck

Equipartition arguments provide an easy way to find a characteristic scale for the magnetic field from radio emission, by assuming the energy densities in cosmic rays and magnetic…