Search Results - "Beacom, John F"
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New Freezeout Mechanism for Strongly Interacting Dark Matter
Published in Physical review letters (25-09-2020)“…We present a new mechanism for thermally produced dark matter, based on a semi-annihilation-like process, χ + χ + SM → χ + SM , with intriguing consequences…”
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Precise relic WIMP abundance and its impact on searches for dark matter annihilation
Published in Physical review. D, Particles, fields, gravitation, and cosmology (03-07-2012)“…If dark matter (DM) is a weakly interacting massive particle (WIMP) that is a thermal relic of the early Universe, then its total self-annihilation cross…”
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Theoretically Palatable Flavor Combinations of Astrophysical Neutrinos
Published in Physical review letters (15-10-2015)“…The flavor composition of high-energy astrophysical neutrinos can reveal the physics governing their production, propagation, and interaction. The IceCube…”
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DUNE as the Next-Generation Solar Neutrino Experiment
Published in Physical review letters (27-09-2019)“…We show that the Deep Underground Neutrino Experiment (DUNE), with significant but feasible new efforts, has the potential to deliver world-leading results in…”
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High-energy Emission from Interacting Supernovae: New Constraints on Cosmic-Ray Acceleration in Dense Circumstellar Environments
Published in The Astrophysical journal (20-03-2019)“…Supernovae (SNe) with strong interactions with circumstellar material (CSM) are promising candidate sources of high-energy neutrinos and gamma-rays and have…”
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Echo Technique to Distinguish Flavors of Astrophysical Neutrinos
Published in Physical review letters (16-04-2019)“…The flavor composition of high-energy astrophysical neutrinos is a rich observable. However, present analyses cannot effectively distinguish particle showers…”
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On the Normalization of the Cosmic Star Formation History
Published in The Astrophysical journal (01-11-2006)“…Strong constraints on the cosmic star formation history (SFH) have recently been established using ultraviolet and far-infrared measurements, refining the…”
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Role of Line-of-sight Cosmic-ray Interactions in Forming the Spectra of Distant Blazars in TeV Gamma Rays and High-energy Neutrinos
Published in The Astrophysical journal (10-04-2011)“…Active galactic nuclei (AGNs) can produce both gamma rays and cosmic rays. The observed high-energy gamma-ray signals from distant blazars may be dominated by…”
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Stringent constraint on galactic positron production
Published in Physical review letters (18-08-2006)“…The intense 0.511 MeV gamma-ray line emission from the Galactic Center observed by INTEGRAL requires a large annihilation rate of nonrelativistic positrons. If…”
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Secondary photons and neutrinos from cosmic rays produced by distant blazars
Published in Physical review letters (09-04-2010)“…Secondary photons and neutrinos produced in the interactions of cosmic ray protons emitted by distant active galactic nuclei (AGN) with the photon background…”
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Measurement of the Core-collapse Progenitor Mass Distribution of the Small Magellanic Cloud
Published in The Astrophysical journal (20-01-2019)“…The physics of core-collapse (CC) supernovae (SNe) and how the explosions depend on progenitor properties are central questions in astronomy. For only a…”
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Evidence for a New Component of High-Energy Solar Gamma-Ray Production
Published in Physical review letters (28-09-2018)“…The observed multi-GeV γ-ray emission from the solar disk-sourced by hadronic cosmic rays interacting with gas and affected by complex magnetic fields-is not…”
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13
The Star Formation Rate in the Reionization Era as Indicated by Gamma-Ray Bursts
Published in The Astrophysical journal (10-11-2009)“…High-redshift gamma-ray bursts (GRBs) offer an extraordinary opportunity to study aspects of the early universe, including the cosmic star formation rate…”
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14
Small-scale Magnetic Fields Are Critical to Shaping Solar Gamma-Ray Emission
Published in The Astrophysical journal (01-02-2024)“…Abstract The Sun is a bright gamma-ray source due to hadronic cosmic-ray interactions with solar gas. While it is known that incoming cosmic rays must…”
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THE STAR-FORMING GALAXY CONTRIBUTION TO THE COSMIC MeV AND GeV GAMMA-RAY BACKGROUND
Published in The Astrophysical journal (01-05-2014)“…Star-forming galaxies could be major contributors to the cosmic GeV [gamma]-ray background, and they are expected to be MeV-dim because of the "pion bump"…”
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Upper bound on the dark matter total annihilation cross section
Published in Physical review letters (07-12-2007)“…We consider dark matter annihilation into standard model particles and show that the least detectable final states, namely, neutrinos, define an upper bound on…”
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A Survey About Nothing: Monitoring a Million Supergiants for Failed Supernovae
Published in The Astrophysical journal (10-09-2008)“…Extragalactic transient searches have historically been limited to looking for the appearance of new sources such as supernovae. It is now possible to carry…”
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An Unexpectedly Swift Rise in the Gamma-Ray Burst Rate
Published in The Astrophysical journal (01-02-2008)“…The association of long gamma-ray bursts with supernovae naturally suggests that the cosmic GRB rate should trace the star formation history. Finding otherwise…”
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Gamma-ray constraint on galactic positron production by MeV dark matter
Published in Physical review letters (06-05-2005)“…The Galactic positrons, as observed by their annihilation gamma-ray line at 0.511 MeV, are difficult to account for with astrophysical sources. It has been…”
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The Diffuse Supernova Neutrino Background
Published in Annual review of nuclear and particle science (23-11-2010)“…The diffuse supernova neutrino background (DSNB) is the weak glow of megaelectronvolt neutrinos and antineutrinos from distant core-collapse supernovae. The…”
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