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This paper introduces Quaternion Approximate Networks (QUAN), a novel deep learning framework that leverages quaternion algebra for rotation equivariant image classification and object detection. Unlike conventional quaternion neural…

计算机视觉与模式识别 · 计算机科学 2026-01-13 Bryce Grant , Peng Wang

The velocity distribution of cold dark matter within galaxies is expected to exhibit ultra-fine-grained substructure as a result of the many foldings of an initially smooth phase-space sheet under gravity. The innumerable folds of this…

高能物理 - 唯象学 · 物理学 2025-09-19 Ciaran A. J. O'Hare , Giovanni Pierobon

We investigate the prospect of an alternative laboratory-based search for the coupling of axions and axion-like particles to photons. Here, the collision of two laser beams resonantly produces axions, and a signal photon is detected after…

高能物理 - 唯象学 · 物理学 2020-05-18 K. A. Beyer , G. Marocco , R. Bingham , G. Gregori

We propose a framework in which the QCD axion has an exponentially large coupling to photons, relying on the "clockwork" mechanism. We discuss the impact of present and future axion experiments on the parameter space of the model. In…

高能物理 - 唯象学 · 物理学 2017-01-31 Marco Farina , Duccio Pappadopulo , Fabrizio Rompineve , Andrea Tesi

Direct detection of dark matter with directional sensitivity is a promising concept for improving the search for weakly interacting massive particles. With information on the direction of WIMP induced nuclear recoils one has access to the…

高能物理 - 唯象学 · 物理学 2015-10-15 Ciaran A. J. O'Hare

Axion-like particles are a broad class of dark matter candidates which are expected to behave as a coherent, classical field with a weak coupling to photons. Research into the detectability of these particles with laser interferometers has…

高能物理 - 唯象学 · 物理学 2019-08-07 Hongwan Liu , Brodi D. Elwood , Matthew Evans , Jesse Thaler

This thesis explores experimental and theoretical approaches to dark matter detection, from gas-based detectors to quantum sensors, tackling the challenge of identifying dark matter, which makes up 27% of the Universe's energy. It reviews…

天体物理仪器与方法 · 物理学 2025-12-05 David Díez-Ibáñez

If dark matter interactions with Standard Model particles are $CP$-violating, then dark matter annihilation/decay can produce photons with a net circular polarization. We consider the prospects for experimentally detecting evidence for such…

宇宙学与河外天体物理 · 物理学 2018-06-27 Andrey Elagin , Jason Kumar , Pearl Sandick , Fei Teng

The axion is an intriguing dark matter candidate emerging from the Peccei-Quinn solution to the strong CP problem. Current experimental searches for axion dark matter focus on the axion mass range below 40 $\mu$eV. However, if the…

天体物理仪器与方法 · 物理学 2019-08-15 Béla Majorovits , Javier Redondo

Object detection with 3D radar is essential for 360-degree automotive perception, but radar's long wavelengths produce sparse and irregular reflections that challenge traditional grid and sequence-based convolutional and transformer…

计算机视觉与模式识别 · 计算机科学 2025-11-20 Loveneet Saini , Hasan Tercan , Tobias Meisen

Adding an axion-like particle (ALP) to the Standard Model, with a field velocity in the early universe, simultaneously explains the observed baryon and dark matter densities. This requires one or more couplings between the ALP and photons,…

高能物理 - 唯象学 · 物理学 2021-02-24 Raymond T. Co , Lawrence J. Hall , Keisuke Harigaya

Astrophysics today faces a number of mysteries which defiant their resolutions in spite of drastic improvements in instrumental design, better technique being developed, and gradual improvements in theoretical and computation methods over…

高能物理 - 唯象学 · 物理学 2019-01-23 Victor V. Flambaum , Ariel R. Zhitnitsky

Signal estimates for direct axion dark matter searches have used the isothermal sphere halo model for the last several decades. While insightful, the isothermal model does not capture effects from a halo's infall history nor the influence…

星系天体物理 · 物理学 2017-08-30 Erik W. Lentz , Thomas R. Quinn , Leslie J Rosenberg , Michael J. Tremmel

The Horizon-10T collaboration \cite{Beisembaev:2016cyg,2017EPJWC.14514001B,Beznosko:2019cI,2019EPJWC.20806002B,Beisembaev:2019nzd} have reported observation of Multi-Modal Events (MME) containing multiple peaks suggesting their clustering…

高能物理 - 唯象学 · 物理学 2021-10-19 Ariel Zhitnitsky

The QCD axion is one of the most compelling candidates to explain the dark matter abundance of the universe. With its extremely small mass ($\ll 1\,\mathrm{eV}/c^2$), axion dark matter interacts as a classical field rather than a particle.…

We propose simple scenarios where the observed dark matter abundance arises from decays and scatterings of heavy quarks through freeze-in of an axion-like particle with mass in the $10 {\rm \, keV} - 1 {\rm \, MeV}$ range. These models can…

Axions are a well-motivated dark matter candidate, with a host of experiments around the world searching for direct evidence of their existence. The ORGAN Experiment is a type of axion detector known as an axion haloscope, which takes the…

高能物理 - 唯象学 · 物理学 2023-06-08 Ben T. McAllister , Aaron Quiskamp , Ciaran O'Hare , Paul Altin , Eugene Ivanov , Maxim Goryachev , Michael Tobar

Axion is one of the most popular candidates of the cosmological dark matter. Recent studies considering the misalignment production of axions suggest some benchmark axion mass ranges near $m_a \sim 20$ $\mu$eV. For such axion mass, the…

宇宙学与河外天体物理 · 物理学 2021-10-25 Man Ho Chan

NGC 3079 is a very active, disturbed galaxy which has been observed to have X-ray and radio ejections from it as well as an optical superbubble along its minor axis. Here we show that the brightest X-ray sources within about 40 arcmin are…

天体物理学 · 物理学 2007-05-23 H. Arp , E. M. Burbidge

The clustering of active galactic nuclei (AGN) sheds light on their typical large (Mpc-scale) environments, which can constrain the growth and evolution of supermassive black holes. Here we measure the clustering of luminous X-ray-selected…

星系天体物理 · 物理学 2020-03-11 M. C. Powell , C. M. Urry , N. Cappelluti , J. T. Johnson , S. M. LaMassa , T. T. Ananna , K. E. Kollmann
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