193,185 research outputs found

    Measuring the likelihood of models for network evolution

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    Many researchers have hypothesised models which explain the evolution of the topology of a target network. The framework described in this paper gives the likelihood that the target network arose from the hypothesised model. This allows rival hypothesised models to be compared for their ability to explain the target network. A null model (of random evolution) is proposed as a baseline for comparison. The framework also considers models made from linear combinations of model components. A method is given for the automatic optimisation of component weights. The framework is tested on simulated networks with known parameters and also on real data

    Measuring dark energy with the Eiso−EpE_{\rm iso}-E_{\rm p} correlation of gamma-ray bursts using model-independent methods

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    In this paper, we use two model-independent methods to standardize long gamma-ray bursts (GRBs) using the Eiso−EpE_{\rm iso}-E_{\rm p} correlation, where EisoE_{\rm iso} is the isotropic-equivalent gamma-ray energy and EpE_{\rm p} is the spectral peak energy. We update 42 long GRBs and try to make constraint on cosmological parameters. The full sample contains 151 long GRBs with redshifts from 0.0331 to 8.2. The first method is the simultaneous fitting method. The extrinsic scatter σext\sigma_{\rm ext} is taken into account and assigned to the parameter EisoE_{\rm iso}. The best-fitting values are a=49.15±0.26a=49.15\pm0.26, b=1.42±0.11b=1.42\pm0.11, σext=0.34±0.03\sigma_{\rm ext}=0.34\pm0.03 and Ωm=0.79\Omega_m=0.79 in the flat Λ\LambdaCDM model. The constraint on Ωm\Omega_m is 0.55<Ωm<10.55<\Omega_m<1 at the 1σ\sigma confidence level. If reduced χ2\chi^2 method is used, the best-fit results are a=48.96±0.18a=48.96\pm0.18, b=1.52±0.08b=1.52\pm0.08 and Ωm=0.50±0.12\Omega_m=0.50\pm0.12. The second method is using type Ia supernovae (SNe Ia) to calibrate the Eiso−EpE_{\rm iso}-E_{\rm p} correlation. We calibrate 90 high-redshift GRBs in the redshift range from 1.44 to 8.1. The cosmological constraints from these 90 GRBs are Ωm=0.23−0.04+0.06\Omega_m=0.23^{+0.06}_{-0.04} for flat Λ\LambdaCDM, and Ωm=0.18±0.11\Omega_m=0.18\pm0.11 and ΩΛ=0.46±0.51\Omega_{\Lambda}=0.46\pm0.51 for non-flat Λ\LambdaCDM. For the combination of GRB and SNe Ia sample, we obtain Ωm=0.271±0.019\Omega_m=0.271\pm0.019 and h=0.701±0.002h=0.701\pm0.002 for the flat Λ\LambdaCDM, and for the non-flat Λ\LambdaCDM, the results are Ωm=0.225±0.044\Omega_m=0.225\pm0.044, ΩΛ=0.640±0.082\Omega_{\Lambda}=0.640\pm0.082 and h=0.698±0.004h=0.698\pm0.004. These results from calibrated GRBs are consistent with that of SNe Ia. Meanwhile, the combined data can improve cosmological constraints significantly, comparing to SNe Ia alone. Our results show that the Eiso−EpE_{\rm iso}-E_{\rm p} correlation is promising to probe the high-redshift universe.Comment: 10 pages, 6 figures, 4 table, accepted by A&A. Table 4 contains calibrated distance moduli of GRB

    A high-reproducibility and high-accuracy method for automated topic classification

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    Much of human knowledge sits in large databases of unstructured text. Leveraging this knowledge requires algorithms that extract and record metadata on unstructured text documents. Assigning topics to documents will enable intelligent search, statistical characterization, and meaningful classification. Latent Dirichlet allocation (LDA) is the state-of-the-art in topic classification. Here, we perform a systematic theoretical and numerical analysis that demonstrates that current optimization techniques for LDA often yield results which are not accurate in inferring the most suitable model parameters. Adapting approaches for community detection in networks, we propose a new algorithm which displays high-reproducibility and high-accuracy, and also has high computational efficiency. We apply it to a large set of documents in the English Wikipedia and reveal its hierarchical structure. Our algorithm promises to make "big data" text analysis systems more reliable.Comment: 23 pages, 24 figure

    Early-warning signals of topological collapse in interbank networks

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    The financial crisis clearly illustrated the importance of characterizing the level of 'systemic' risk associated with an entire credit network, rather than with single institutions. However, the interplay between financial distress and topological changes is still poorly understood. Here we analyze the quarterly interbank exposures among Dutch banks over the period 1998-2008, ending with the crisis. After controlling for the link density, many topological properties display an abrupt change in 2008, providing a clear - but unpredictable - signature of the crisis. By contrast, if the heterogeneity of banks' connectivity is controlled for, the same properties show a gradual transition to the crisis, starting in 2005 and preceded by an even earlier period during which anomalous debt loops could have led to the underestimation of counter-party risk. These early-warning signals are undetectable if the network is reconstructed from partial bank-specific data, as routinely done. We discuss important implications for bank regulatory policies.Comment: 28 pages, 23 figures, 1 tabl

    Failure dynamics of the global risk network

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    Risks threatening modern societies form an intricately interconnected network that often underlies crisis situations. Yet, little is known about how risk materializations in distinct domains influence each other. Here we present an approach in which expert assessments of risks likelihoods and influence underlie a quantitative model of the global risk network dynamics. The modeled risks range from environmental to economic and technological and include difficult to quantify risks, such as geo-political or social. Using the maximum likelihood estimation, we find the optimal model parameters and demonstrate that the model including network effects significantly outperforms the others, uncovering full value of the expert collected data. We analyze the model dynamics and study its resilience and stability. Our findings include such risk properties as contagion potential, persistence, roles in cascades of failures and the identity of risks most detrimental to system stability. The model provides quantitative means for measuring the adverse effects of risk interdependence and the materialization of risks in the network
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