Abstract:Abstract. The unrestricted T-system is a family of relations in the Grothendieck ring of the category of the finite-dimensional modules of the Yangian or the quantum affine algebra associated with a complex simple Lie algebra. The unrestricted T-system admits a reduction called the restricted T-system. In this paper we formulate the periodicity conjecture for the restricted T-systems, which is the counterpart of the known and partially proved periodicity conjecture for the restricted Y-systems. Then, we partia… Show more
“…We assume that charged particles, including (primary) electrons, protons, and heavier nuclei are accelerated to high energies before they are injected into the blob, where they subsequently lose energy through various radiative processes. Several mechanisms of particle acceleration have been discussed in application to AGN jets, e.g., Fermi type I (Dermer & Razzaque 2010;Inoue & Tanaka 2016), Fermi type II (Böttcher et al 1999;Schlickeiser & Dermer 2000;Katarzynski et al 2006), magnetic reconnection (Lovelace et al 1997;Giannios et al 2009;Nalewajko et al 2018;Christie et al 2019), shear acceleration (Rieger & Duffy 2004;Rieger et al 2007;Kimura et al 2017b). In all scenarios, the acceleration efficiency depends on local plasma conditions (for relativistic shocks in magnetized jets, see Sironi et al 2015a,b).…”
The IceCube collaboration reported a ∼ 3.5σ excess of 13 ± 5 neutrino events in the direction of the blazar TXS 0506+056 during a ∼6 month period in 2014-2015, as well as the (∼ 3σ) detection of a high-energy muon neutrino during an electromagnetic flare in 2017. We explore the possibility that the 2014-2015 neutrino excess and the 2017 multi-messenger flare are both explained in a common physical framework that relies on the emergence of a relativistic neutral beam in the blazar jet due to interactions of accelerated cosmic rays (CRs) with photons. We demonstrate that the neutral beam model provides an explanation for the 2014-2015 neutrino excess without violating X-ray and γ-ray constraints, and also yields results consistent with the detection of one high-energy neutrino during the 2017 flare. If both neutrino associations with TXS 05065+056 are real, our model requires that (i) the composition of accelerated CRs is light, with a ratio of helium nuclei to protons 5, (ii) a luminous external photon field (∼ 10 46 erg s −1 ) variable (on year-long timescales) is present, and (iii) the CR injection luminosity as well as the properties of the dissipation region (i.e., Lorentz factor, magnetic field, and size) vary on year-long timescales.
“…We assume that charged particles, including (primary) electrons, protons, and heavier nuclei are accelerated to high energies before they are injected into the blob, where they subsequently lose energy through various radiative processes. Several mechanisms of particle acceleration have been discussed in application to AGN jets, e.g., Fermi type I (Dermer & Razzaque 2010;Inoue & Tanaka 2016), Fermi type II (Böttcher et al 1999;Schlickeiser & Dermer 2000;Katarzynski et al 2006), magnetic reconnection (Lovelace et al 1997;Giannios et al 2009;Nalewajko et al 2018;Christie et al 2019), shear acceleration (Rieger & Duffy 2004;Rieger et al 2007;Kimura et al 2017b). In all scenarios, the acceleration efficiency depends on local plasma conditions (for relativistic shocks in magnetized jets, see Sironi et al 2015a,b).…”
The IceCube collaboration reported a ∼ 3.5σ excess of 13 ± 5 neutrino events in the direction of the blazar TXS 0506+056 during a ∼6 month period in 2014-2015, as well as the (∼ 3σ) detection of a high-energy muon neutrino during an electromagnetic flare in 2017. We explore the possibility that the 2014-2015 neutrino excess and the 2017 multi-messenger flare are both explained in a common physical framework that relies on the emergence of a relativistic neutral beam in the blazar jet due to interactions of accelerated cosmic rays (CRs) with photons. We demonstrate that the neutral beam model provides an explanation for the 2014-2015 neutrino excess without violating X-ray and γ-ray constraints, and also yields results consistent with the detection of one high-energy neutrino during the 2017 flare. If both neutrino associations with TXS 05065+056 are real, our model requires that (i) the composition of accelerated CRs is light, with a ratio of helium nuclei to protons 5, (ii) a luminous external photon field (∼ 10 46 erg s −1 ) variable (on year-long timescales) is present, and (iii) the CR injection luminosity as well as the properties of the dissipation region (i.e., Lorentz factor, magnetic field, and size) vary on year-long timescales.
“…The derived categories of finite-dimensional nonsemisimple algebras are never CY, but they are often fractionally CY. Some recent meetings [3,4,39,41] as well as recent results including [16,21,25,27,32,33,[35][36][37][38]42] suggest that the fractionally CY property becomes more and more important in representation theory, singularity theory, commutative and non-commutative algebraic geometry. The aim of this paper is to apply the fractionally CY property in the study of n-representation-finite algebras defined below.…”
In this paper, we study n-representation-finite algebras from the viewpoint of the fractionally Calabi-Yau property. We shall show that all n-representation-finite algebras are twisted fractionally Calabi-Yau. We also show that for any > 0, twisted (n( − 1)/ )-Calabi-Yau algebras of global dimension at most n are n-representation-finite. As an application, we give a construction of n-representation-finite algebras using the tensor product.
“…Carreño [7] investigated the impact properties of the laminated composite plates consisting of brittle 1.55 wt% C UHCS steel and soft 0.035 wt% C mild steel, indicating that the Charpy V-notched energy of 7-layered laminated composites was 160 kJ m À2 higher than that of the UHCS mono-layered specimens. Inoue [8] prepared the multilayered steel composites consisting of brittle SS420 and relative soft SS304 via hot-roll-bonding, cold rolling and the final heat treated. The results indicated that the fracture elongation enhanced with the decreasing thickness of monolayer and reached to 15% for the specimens with 40 mm-thick per layer.…”
A 3‐layered composite plate is innovatively fabricated via composite rolling of 1.6 wt% B stainless steel surrounded by two layers of boron‐free steels. The tensile properties of composite and non‐composite plates are comparatively tested and analyzed. Besides, the microstructure evolution of the investigated plates is characterized in detail. It is found that the composite specimens exhibit higher tensile elongation comparing with that of non‐composite specimens. Specifically, the engineering strain of the 1050 °C × 30 min solution‐treated specimens reaches to 12.5 ± 0.8% which is 2.5–3.0 times as high as that of non‐composite specimens. In addition, the as‐cast lamellar borides break into bar‐shaped structures in hot rolled plates, however, their morphology and distribution hardly change after solution treatment. Besides, the transition regions between the core and clad layers are formed and characterized by medium‐sized recrystallized grains and fine borides in the solution‐treated composite specimens. The enhancement mechanism of tensile elongation is mainly analyzed in term of the geometrical restriction of necking in the composite plate during tensile deformation. This paper provides a promising method to effectively enhance the tensile fracture elongation for these metallic materials with poor plasticity like high borated stainless steels.
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