12,640 research outputs found

    Bijection between Conjugacy Classes and Irreducible Representations of Finite Inverse Semigroups

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    In this paper we show that the irreducible representations of a finite inverse semigroup SS over an algebraically closed field FF are in bijection with the conjugacy classes of SS if the characteristic of FF is zero or a prime number that does not divide the order of any maximal subgroup of SS

    Hard X-ray emission and 44^{44}Ti line features of Tycho Supernova Remnant

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    A deep hard X-ray survey of the INTEGRAL satellite first detected the non-thermal emission up to 90 keV in the Tycho supernova (SN) remnant. Its 3 -- 100 keV spectrum is fitted with a thermal bremsstrahlung of kT∼0.81±0.45kT\sim 0.81\pm 0.45 keV plus a power-law model of Γ∼3.01±0.16\Gamma \sim 3.01\pm 0.16. Based on the diffusive shock acceleration theory, this non-thermal emission, together with radio measurements, implies that Tycho remnant may not accelerate protons up to >>PeV but hundreds TeV. Only heavier nuclei may be accelerated to the cosmic ray spectral "knee". In addition, we search for soft gamma-ray lines at 67.9 and 78.4 keV coming from the decay of radioactive 44^{44}Ti in Tycho remnant by INTEGRAL. A bump feature in the 60-90 keV energy band, potentially associated with the 44^{44}Ti line emission, is found with a marginal significance level of ∼\sim 2.6 σ\sigma. The corresponding 3 σ\sigma upper limit on the 44^{44}Ti line flux amounts to 1.5 ×\times 10−5^{-5} ph cm−2^{-2} s−1^{-1}. Implications on the progenitor of Tycho SN, considered to be the prototype of type Ia SN, are discussed.Comment: 15 pages, 4 figures, accepted for publication in Ap
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