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Related papers: Pulse Pileup Rejection Methods Using a Two-Compone…

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We study a two-lane two-species exclusion process inspired by Lin et al. (C. Lin et al. J. Stat. Mech., 2011), that exhibits a non-equilibrium pulsing phase. Particles move on two parallel one-dimensional tracks, with one open and one…

Statistical Mechanics · Physics 2017-03-31 Sarah Klein , Cécile Appert-Rolland , Martin R. Evans

Well-known quantum machine learning techniques, namely quantum kernel assisted support vector machines (QSVMs) and quantum convolutional neural networks (QCNNs), are applied to the binary classification of pulsars. In this comparitive study…

Quantum Physics · Physics 2024-09-09 Donovan Slabbert , Matt Lourens , Francesco Petruccione

Anomaly detection is not an easy problem since distribution of anomalous samples is unknown a priori. We explore a novel method that gives a trade-off possibility between one-class and two-class approaches, and leads to a better performance…

Machine Learning · Statistics 2020-05-26 Maxim Borisyak , Artem Ryzhikov , Andrey Ustyuzhanin , Denis Derkach , Fedor Ratnikov , Olga Mineeva

Neutron stars or pulsars are very rapidly rotating compact stars with extremely high density. One of the unsolved long-standing problems of these enigmatic celestial bodies is the origin of pulsars' glitches, i.e., the sudden rapid…

High Energy Astrophysical Phenomena · Physics 2020-10-20 Giacomo Marmorini , Shigehiro Yasui , Muneto Nitta

In high-background or calibration measurements with cryogenic particle detectors, a significant share of the exposure is lost due to pile-up of recoil events. We propose a method for the separation of pile-up events with an LSTM neural…

Instrumentation and Detectors · Physics 2021-12-14 Felix Wagner

Estimating the number of components is a fundamental challenge in unsupervised learning, particularly when dealing with high-dimensional data with many components or severely imbalanced component sizes. This paper addresses this challenge…

Machine Learning · Statistics 2026-04-22 Huan Qing

Searches for new physics typically rely on proton-proton collisions, where isolated mass bumps are the primary signatures. However, when a new particle is nearly degenerate in mass with a known Standard Model resonance, it can be partially…

High Energy Physics - Phenomenology · Physics 2026-05-14 Yi Yang

A pulse-shape discrimination method based on artificial neural networks was applied to pulses simulated for different background, signal and signal-like interactions inside a germanium detector. The simulated pulses were used to investigate…

Instrumentation and Detectors · Physics 2015-09-02 A. Caldwell , F. Cossavella , B. Majorovits , D. Palioselitis , O. Volynets

The detection of nanoHertz gravitational waves through pulsar timing arrays hinges on identifying a common stochastic process affecting all pulsars in a correlated way across the sky. In the presence of other deterministic and stochastic…

High Energy Astrophysical Phenomena · Physics 2024-02-14 Patrick M. Meyers , Katerina Chatziioannou , Michele Vallisneri , Alvin J. K. Chua

In a fissile material, the inherent multiplicity of neutrons born through induced fissions leads to correlations in their detection statistics. The correlations between neutrons can be used to trace back some characteristics of the fissile…

Computation · Statistics 2022-11-17 Paul Lartaud , Philippe Humbert , Josselin Garnier

Consider a spiked random tensor obtained as a mixture of two components: noise in the form of a symmetric Gaussian $p$-tensor for $p\geq 3$ and signal in the form of a symmetric low-rank random tensor. The latter is defined as a linear…

Probability · Mathematics 2021-10-11 Wei-Kuo Chen , Madeline Handschy , Gilad Lerman

In order to investigate the importance of dissipation in the pulsar magnetosphere we decided to combine Force-Free with Aristotelian Electrodynamics. We obtain solutions that are ideal (non-dissipative) everywhere except in an equatorial…

High Energy Astrophysical Phenomena · Physics 2016-09-28 Ioannis Contopoulos

The Double Chooz experiment measures the neutrino mixing angle $\theta_{13}$ by detecting reactor $\bar{\nu}_e$ via inverse beta decay. The positron-neutron space and time coincidence allows for a sizable background rejection, nonetheless…

Instrumentation and Detectors · Physics 2014-10-08 Y. Abe , J. C. dos Anjos , J. C. Barriere , E. Baussan , I. Bekman , M. Bergevin , T. J. C. Bezerra , L. Bezrukov , E. Blucher , C. Buck , J. Busenitz , A. Cabrera , E. Caden , L. Camilleri , R. Carr , M. Cerrada , P. -J. Chang , E. Chauveau , P. Chimenti , A. P. Collin , E. Conover , J. M. Conrad , J. I. Crespo-Anadon , K. Crum , A. S. Cucoanes , E. Damon , J. V. Dawson , J. Dhooghe , D. Dietrich , Z. Djurcic , M. Dracos , M. Elnimr , A. Etenko , M. Fallot , F. von Feilitzsch , J. Felde , S. M. Fernandes , V. Fischer , D. Franco , M. Franke , H. Furuta , I. Gil-Botella , L. Giot , M. Goger-Neff , L. F. G. Gonzalez , L. Goodenough , M. C. Goodman , C. Grant , N. Haag , T. Hara , J. Haser , M. Hofmann , G. A. Horton-Smith , A. Hourlier , M. Ishitsuka , J. Jochum , C. Jollet , F. Kaether , L. N. Kalousis , Y. Kamyshkov , D. M. Kaplan , T. Kawasaki , E. Kemp , H. de Kerret , D. Kryn , M. Kuze , T. Lachenmaier , C. E. Lane , T. Lasserre , A. Letourneau , D. Lhuillier , H. P. Lima , M. Lindner , J. M. Lopez-Castano , J. M. LoSecco , B. Lubsandorzhiev , S. Lucht , J. Maeda , C. Mariani , J. Maricic , J. Martino , T. Matsubara , G. Mention , A. Meregaglia , T. Miletic , R. Milincic , A. Minotti , Y. Nagasaka , Y. Nikitenko , P. Novella , L. Oberauer , M. Obolensky , A. Onillon , A. Osborn , C. Palomares , I. M. Pepe , S. Perasso , P. Pfahler , A. Porta , G. Pronost , J. Reichenbacher , B. Reinhold , M. Rohling , R. Roncin , S. Roth , B. Rybolt , Y. Sakamoto , R. Santorelli , A. C. Schilithz , S. Schonert , S. Schoppmann , M. H. Shaevitz , R. Sharankova , S. Shimojima , D. Shrestha , V. Sibille , V. Sinev , M. Skorokhvatov , E. Smith , J. Spitz , A. Stahl , I. Stancu , L. F. F. Stokes , M. Strait , A. Stuken , F. Suekane , S. Sukhotin , T. Sumiyoshi , Y. Sun , R. Svoboda , K. Terao , A. Tonazzo , H. H. Trinh Thi , G. Valdiviesso , N. Vassilopoulos , C. Veyssiere , M. Vivier , S. Wagner , N. Walsh , H. Watanabe , C. Wiebusch , L. Winslow , M. Wurm , G. Yang , F. Yermia , V. Zimmer

Binary pulsars are a powerful tool for probing strong gravity that still outperforms direct gravitational wave observations in a number of directions due to the remarkable accuracy of the pulsar timing. They can constrain very precisely the…

General Relativity and Quantum Cosmology · Physics 2024-06-26 Petar Y. Yordanov , Kalin V. Staykov , Stoytcho S. Yazadjiev , Daniela D. Doneva

Modern pulsar surveys produce many millions of candidate pulsars, far more than can be individually inspected. Traditional methods for filtering these candidates, based upon the signal-to-noise ratio of the detection, cannot easily…

Solar and Stellar Astrophysics · Physics 2009-11-13 M. J. Keith , R. P. Eatough , A. G. Lyne , M. Kramer , A. Possenti , F. Camilo , R. N. Manchester

Finite mixture models are statistical models which appear in many problems in statistics and machine learning. In such models it is assumed that data are drawn from random probability measures, called mixture components, which are…

Machine Learning · Statistics 2022-04-05 Robert A. Vandermeulen , Clayton D. Scott

There is a broad class of astrophysical sources that produce detectable, transient, gravitational waves. Some searches for transient gravitational waves are tailored to known features of these sources. Other searches make few assumptions…

We introduce a new periodicity detection algorithm for binary time series of event onsets, the Gaussian Mixture Periodicity Detection Algorithm (GMPDA). The algorithm approaches the periodicity detection problem to infer the parameters of a…

Methodology · Statistics 2022-01-21 Ezekiel Barnett , Olga Kaiser , Jonathan Masci , Ernst Wit , Stephany Fulda

In the standard two-component crust-superfluid model of a neutron star, timing noise can arise when the two components are perturbed by stochastic torques. Here it is demonstrated how to analyse fluctuations in radio pulse times of arrival…

High Energy Astrophysical Phenomena · Physics 2024-03-26 Nicholas J. O'Neill , Patrick M. Meyers , Andrew Melatos

Because of the electromagnetic radiation produced during the merger, compact binary coalescences with neutron stars may result in multi-messenger observations. In order to follow up on the gravitational-wave signal with electromagnetic…

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