2,104 research outputs found

    Application of the Gaussian mixture model in pulsar astronomy -- pulsar classification and candidates ranking for {\it Fermi} 2FGL catalog

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    Machine learning, algorithms to extract empirical knowledge from data, can be used to classify data, which is one of the most common tasks in observational astronomy. In this paper, we focus on Bayesian data classification algorithms using the Gaussian mixture model and show two applications in pulsar astronomy. After reviewing the Gaussian mixture model and the related Expectation-Maximization algorithm, we present a data classification method using the Neyman-Pearson test. To demonstrate the method, we apply the algorithm to two classification problems. Firstly, it is applied to the well known period-period derivative diagram, where we find that the pulsar distribution can be modeled with six Gaussian clusters, with two clusters for millisecond pulsars (recycled pulsars) and the rest for normal pulsars. From this distribution, we derive an empirical definition for millisecond pulsars as PΛ™10βˆ’17≀3.23(P100ms)βˆ’2.34\frac{\dot{P}}{10^{-17}} \leq3.23(\frac{P}{100 \textrm{ms}})^{-2.34}. The two millisecond pulsar clusters may have different evolutionary origins, since the companion stars to these pulsars in the two clusters show different chemical composition. Four clusters are found for normal pulsars. Possible implications for these clusters are also discussed. Our second example is to calculate the likelihood of unidentified \textit{Fermi} point sources being pulsars and rank them accordingly. In the ranked point source list, the top 5% sources contain 50% known pulsars, the top 50% contain 99% known pulsars, and no known active galaxy (the other major population) appears in the top 6%. Such a ranked list can be used to help the future follow-up observations for finding pulsars in unidentified \textit{Fermi} point sources.Comment: 9 pages, 4 figures, accepted by MNRA

    Convexity criteria and uniqueness of absolutely minimizing functions

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    We show that absolutely minimizing functions relative to a convex Hamiltonian H:Rnβ†’RH:\mathbb{R}^n \to \mathbb{R} are uniquely determined by their boundary values under minimal assumptions on H.H. Along the way, we extend the known equivalences between comparison with cones, convexity criteria, and absolutely minimizing properties, to this generality. These results perfect a long development in the uniqueness/existence theory of the archetypal problem of the calculus of variations in L∞.L^\infty.Comment: 34 page

    Des modèles biologiques à l'amélioration des plantes

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    Mechanical behavior of Zr-based bulk metallic glasses

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    Bulk metallic glasses have a very high corrosion resistance and mechanical strength. Bulk metallic glasses show elastic-perfectly plastic behavior with an extended region of elastic strain (β‰ˆ 2%). But at room temperature their macroscopic plasticity is weak even though a local plastic strain is observed in shear bands. A relaxation analysis allowed studying micro-mechanisms of plastic deformation and estimating the apparent activation volume (β‰ˆ 2000 ³).ВысокопрочныС стСкла Π½Π° основС ΠΌΠ΅Ρ‚Π°Π»Π»ΠΎΠ² ΠΈΠΌΠ΅ΡŽΡ‚ ΠΎΡ‡Π΅Π½ΡŒ высокиС характСристики ΠΊΠΎΡ€Ρ€ΠΎΠ·ΠΈΠΎΠ½Π½ΠΎΠΉ устойчивости ΠΈ мСханичСской проч­ности. Π˜Ρ… Π΄Π΅Ρ„ΠΎΡ€ΠΌΠΈΡ€ΠΎΠ²Π°Π½ΠΈΠ΅ являСтся Π°Π±ΡΠΎΠ»ΡŽΡ‚Π½ΠΎ упругопластичСским с протяТСнным участком упругости (β‰ˆ 2%). Однако ΠΏΡ€ΠΈ ΠΊΠΎΠΌΠ½Π°Ρ‚Π½ΠΎΠΉ Ρ‚Π΅ΠΌΠΏΠ΅Ρ€Π°Ρ‚ΡƒΡ€Π΅ ΠΈΡ… ΠΌΠ°ΠΊΡ€ΠΎΠΏΠ»Π°ΡΡ‚ΠΈΡ‡Π½ΠΎΡΡ‚ΡŒ проявляСтся слабо, нСсмотря Π½Π° Π½Π°Π»ΠΈΡ‡ΠΈΠ΅ Π»ΠΎΠΊΠ°Π»ΡŒΠ½Ρ‹Ρ… пластичСских Π΄Π΅Ρ„ΠΎΡ€ΠΌΠ°Ρ†ΠΈΠΉ Π² поло­сах скольТСния. Анализ рСлаксации напряТСний ΠΏΠΎΠ·Π²ΠΎΠ»ΠΈΠ» ΠΈΡΡΠ»Π΅Π΄ΠΎΠ²Π°Ρ‚ΡŒ ΠΌΠΈΠΊΡ€ΠΎΠΌΠ΅Ρ…Π°Π½ΠΈΠ·Β­ΠΌΡ‹ пластичСского дСформирования ΠΈ ΠΎΡ†Π΅Π½ΠΈΡ‚ΡŒ Π·Π½Π°Ρ‡Π΅Π½ΠΈΠ΅ объСма Π°ΠΊΡ‚ΠΈΠ²Π°Ρ†ΠΈΠΈ (β‰ˆ 2000 ³)

    Development of a pulsar-based timescale

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    Using observations of pulsars from the Parkes Pulsar Timing Array (PPTA) project we develop the first pulsar-based timescale that has a precision comparable to the uncertainties in international atomic timescales. Our ensemble of pulsars provides an Ensemble Pulsar Scale (EPS) analogous to the free atomic timescale Echelle Atomique Libre (EAL). The EPS can be used to detect fluctuations in atomic timescales and therefore can lead to a new realisation of Terrestrial Time, TT(PPTA11). We successfully follow features known to affect the frequency of the International Atomic Timescale (TAI) and we find marginally significant differences between TT(PPTA11) and TT(BIPM11). We discuss the various phenomena that lead to a correlated signal in the pulsar timing residuals and therefore limit the stability of the pulsar timescale.Comment: Accepted for publication in MNRA

    Understanding Paramagnetic Spin Correlations in the Spin-Liquid Pyrochlore Tb2Ti2O7

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    Recent elastic and inelastic neutron scattering studies of the highly frustrated pyrochlore antiferromagnet Tb2Ti2O7 have shown some very intriguing features that cannot be modeled by the local classical Ising model, naively expected to describe this system at low temperatures. Using the random phase approximation to take into account fluctuations between the ground state doublet and the first excited doublet, we successfully describe the elastic neutron scattering pattern and dispersion relations in Tb2Ti2O7, semi-quantitatively consistent with experimental observations.Comment: revtex4, 4 pages, 1 Color+ 2 BW figure
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