ZEU-THAT

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2018-11-07
13:22
[PUBDB-2018-04279] Report/Journal Article
; ; ; et al
Binary neutron star merger remnants as sources of cosmic-ray
[DESY-18-097; arXiv:1806.01624]
We investigate non-thermal electron and nuclei energy losses within the binary neutron star merger remnant produced by the event GW170817. The lack of a cooling feature within the detected synchrotron emission from the source is used to constrain the magnetic field at the mG level, assuming that this emission is electron synchrotron in origin, and that the accelerated spectrum in the electrons follows the form $dN/dE_e \propto E_e^{-2}$. [...]
Restricted: NS-NS_Mergers_v2(2) - Download fulltextPDF Download fulltextPDF (PDFA); 1-s2.0-S092765051830166X-main - Download fulltextPDF Download fulltextPDF (PDFA); External link: Download fulltextFulltext
ddc:540
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2018-11-05
13:36
OpenAccess [PUBDB-2018-04143] Report/Journal Article
; ; ; et al
Inefficient Cosmic-Ray Diffusion around Vela X: Constraints from H.E.S.S. Observations of Very High-energy Electrons
[arXiv:1807.04182]
Vela X is a nearby pulsar wind nebula (PWN) powered by a ~104 year old pulsar. Modeling of the spectral energy distribution of the Vela X PWN has shown that accelerated electrons have largely escaped from the confinement, which is likely due to the disruption of the initially confined PWN by the supernova remnant reverse shock [...]
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ddc:520
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2018-10-29
08:01
OpenAccess [PUBDB-2018-03978] Preprint/Report
; ;
Modeling of the spatially resolved non-thermal emission from the Vela Jr. supernova remnant
[DESY-18-039; arXiv:1807.10551]
 GO
Vela Jr. (RX J0852.0$-$4622) is one of just a few known supernova remnants (SNRs) with a resolved shell across the whole electromagnetic spectrum from radio to very-high-energy ($>100$ GeV; VHE) gamma-rays. [...]
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2018-09-04
17:33
OpenAccess [PUBDB-2018-03368] Preprint/Report
; ; ; et al
Data-driven model of the cosmic-ray flux and mass composition from 10 GeV to $10^{11}$ GeV
[arXiv:1711.11432]
We present a new parametrization of the cosmic-ray flux and its mass composition over an energy range from 10 GeV to $10^{11}$ GeV. Our approach is data-driven and relies on theoretical assumptions as little as possible. [...]
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ddc:530
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2018-09-04
14:43
OpenAccess [PUBDB-2018-03367] Preprint/Report
; ; ; et al
The hadronic interaction model SIBYLL 2.3c and Feynman scaling
[arXiv:1709.07227]
 GO
The Monte Carlo model Sibyll has been designed for efficient simulation of hadronic multiparticle production up to the highest energies as needed for interpreting cosmic ray measurements. For more than 15 years, version 2.1 of Sibyll has been one of the standard models for air shower simulation. [...]
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2018-09-04
14:26
[PUBDB-2018-03366] Master Thesis

Cosmogenic neutrinos as secondary messengers of Ultra-High Energy Cosmic Rays
x () = Masterarbeit, Humboldt-Universität zu Berlin, 2016

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2018-09-04
14:20
[PUBDB-2018-03365] Master Thesis

Implications of collision dynamics in Gamma-Ray Burst internal shocks on the production of multiple astrophysical messengers
x () = Masterarbeit, KIT Karlruhe, 2017

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2018-09-04
14:12
OpenAccess [PUBDB-2018-03364] Dissertation / PhD Thesis
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Implications of physics beyond the Standard Model in the quark and lepton sectors
Humboldt-Universität zu Berlin 154 pp. () [10.18452/19174] = Dissertation, Humboldt-Universität zu Berlin, 2018  GO
Das Standardmodell (SM) der Teilchenphysik hat sich in der Praxis als vielseitige Theorie bewährt, dennoch deuten nichtverschwindende Neutrinomassen, dunkle Materie und Baryonenasymmetrie auf Physik jenseits des SM (BSM) hin. Um also ein mit den Beobachtungen konsistentes Modell zu entwickeln, ist eine umfassendere Theorie nötig. [...]
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2018-09-04
14:01
OpenAccess [PUBDB-2018-03363] Journal Article/Contribution to a conference proceedings
; ; ; et al
The hadronic interaction model Sibyll – past, present and future
XIX International Symposium on Very High Energy Cosmic Ray Interactions, ISVHECRI 2016, MoscowMoscow, Russia, 22 Aug 2016 - 27 Aug 20162016-08-222016-08-27 The European physical journal / Web of Conferences 145, 08001 () [10.1051/epjconf/201714508001]  GO
Sibyll is one of the first microscopic interaction models that was specifically developed for interpreting cosmic ray data. It combines non-perturbative concepts of simulating hadronic particle production with predictions derived from perturbative QCD calculations, focusing on forward particle production of relevance in studying cosmic ray interactions [...]
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2018-09-04
13:54
OpenAccess [PUBDB-2018-03362] Journal Article/Report/Contribution to a conference proceedings
; ; ; et al
The hadronic interaction model Sibyll 2.3c and Feynman scaling
[arXiv:1709.07227]
35th International Cosmic Ray Conference, ICRC2017, BusanBusan, South Korea, 10 Jul 2017 - 20 Jul 20172017-07-102017-07-20 Proceedings of Science (ICRC2017), 301 () [10.22323/1.301.0301]  GO
The Monte Carlo model Sibyll has been designed for efficient simulation of hadronic multiparticle production up to the highest energies as needed for interpreting cosmic ray measurements. For more than 15 years, version 2.1 of Sibyll has been one of the standard models for air shower simulation. [...]
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ddc:530
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