ZEU-THAT

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2019-06-13
11:33
OpenAccess [PUBDB-2019-02473] Preprint/Report
et al
Non-thermal emission from the reverse shock of the youngest galactic Supernova remnant G1.9+0.3
[arXiv:1906.02725]
 GO
Context. The youngest Galactic supernova remnant G1.9+0.3 is an interesting target for next generation gamma-ray observatories. [...]
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ddc:520
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2019-05-20
16:18
OpenAccess [PUBDB-2019-02318] Report/Journal Article
et al
Constraining the Magnetic Field in the TeV Halo of Geminga with X-Ray Observations
[arXiv:1904.11438]
Recently, the High Altitude Water Cherenkov (HAWC) collaboration reported the discovery of a TeV halo around the Geminga pulsar. The TeV emission is believed to originate from the inverse Compton scattering of pulsar-injected electrons/positrons off cosmic microwave background photons. [...]
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2019-05-20
16:09
Embargoed OpenAccess [PUBDB-2019-02317] Report/Journal Article
et al
Secondary neutrino and gamma-ray fluxes from SimProp and CRPropa
[arXiv:1901.01244]
The interactions of ultra-high energy cosmic rays (UHECRs) with background photons in extragalactic space generate high-energy neutrinos and photons. Simulating UHECR propagation requires assumptions about physical quantities such as the spectrum of the extragalactic background light (EBL) and photodisintegration cross sections. [...]
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ddc:530
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2019-05-07
16:21
OpenAccess [PUBDB-2019-02175] Journal Article
et al
Leptohadronic Blazar Models Applied to the 2014–2015 Flare of TXS 0506+056
We investigate whether the emission of neutrinos observed in 2014–2015 from the direction of the blazar TXS 0506+056 can be accommodated with leptohadronic multiwavelength models of the source commonly adopted for the 2017 flare. While multiwavelength data during the neutrino flare are sparse, the large number of neutrino events (13 ± 5) challenges the missing activity in gamma-rays [...]
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2019-03-14
11:06
OpenAccess [PUBDB-2019-01535] Journal Article
et al
Relativistic Jet Simulations of the Weibel Instability in the Slab Model to Cylindrical Jets with Helical Magnetic Fields
Galaxies 7(1), 29 () [10.3390/galaxies7010029]  GO
The particle-in-cell (PIC) method was developed to investigate microscopic phenomena, and with the advances in computing power, newly developed codes have been used for several fields, such as astrophysical, magnetospheric, and solar plasmas. PIC applications have grown extensively, with large computing powers available on supercomputers such as Pleiades and Blue Waters in the US. [...]
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2019-01-10
14:38
[PUBDB-2019-00317] Conference Presentation

Cosmic ray diffusion in galactic turbulence
Cosmic Ray Transport and Energetic Radiations 2018, CRATER 2018, L'AquilaL'Aquila, Italy, 28 May 2018 - 1 Jun 20182018-05-282018-06-01

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2019-01-10
14:27
[PUBDB-2019-00312] Conference Presentation

Properties of MHD modes in compressible turbulence
Arcetri 2018 Workshop on Plasma Astrophysics, ArcetriArcetri, Italy, 22 Oct 2018 - 26 Oct 20182018-10-222018-10-26

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2019-01-10
14:17
[PUBDB-2019-00308] Conference Presentation

Hadronuclear interpretation of neutrino events from TXS 0506+056
TeV Particle Astrophysics conference, BerlinBerlin, Germany, 27 Aug 2018 - 31 Aug 20182018-08-272018-08-31

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2019-01-10
11:27
[PUBDB-2019-00274] Conference Presentation (Invited)

Identification of Magnetonsonic Modes in Galactic Turbulence with Synchrotron Polarization
1st TagKASI conference on Cosmic Dust and Magnetism, DaejeonDaejeon, South Korea, 30 Oct 2018 - 2 Nov 20182018-10-302018-11-02

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2019-01-10
11:24
[PUBDB-2019-00273] Conference Presentation (Invited)

3D Magnetic field detection with Ground stateAlignment (GSA)
1st TagKASI conference on Cosmic Dust and Magnetism, DaejeonDaejeon, South Korea, 30 Oct 2018 - 2 Nov 20182018-10-302018-11-02

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