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Phase-dependent Hanbury-Brown and Twiss effect for the complete measurement of the complex coherence function.
Light Sci Appl
January 2025
Department of Physics, City University of Hong Kong, 83 Tat Chee Avenue, Kowloon, Hong Kong SAR, China.
Hanbury-Brown and Twiss (HBT) effect is the foundation for stellar intensity interferometry. However, it is a phase insensitive two-photon interference effect. Here we extend the HBT interferometer by mixing intensity-matched reference fields with the input fields before intensity correlation measurement.
View Article and Find Full Text PDFAbsorption spectra of PS in the ultraviolet and infrared region.
Spectrochim Acta A Mol Biomol Spectrosc
January 2025
Institute of Atomic and Molecular Physics, Jilin University, Changchun 130012 China. Electronic address:
The line list is essential for accurately modeling various astrophysical phenomena, such as stellar photospheres and atmospheres of extrasolar planets. This paper introduces a new line database for the PS molecule spanning from the ultraviolet to the infrared regions, covering wavenumbers up to 45000 cm and containing over ten million transitions between 150,458 states with total angular momentum J < 160. Accurate line intensities for rotational, vibrational and electronic transitions are generated by using the general purpose variational code DUO.
View Article and Find Full Text PDFThe GD-1 Stellar Stream Perturber as a Core-collapsed Self-interacting Dark Matter Halo.
Astrophys J Lett
January 2025
Carnegie Observatories, 813 Santa Barbara Street, Pasadena, CA 91101, USA;
The GD-1 stellar stream exhibits spur and gap structures that may result from a close encounter with a dense substructure. When interpreted as a dark matter subhalo, the perturber is denser than predicted in the standard cold dark matter (CDM) model. In self-interacting dark matter (SIDM), however, a halo could evolve into a phase of gravothermal collapse, resulting in a higher central density than its CDM counterpart.
View Article and Find Full Text PDFLanguorous cosmic beats could be generated by magnetic forces between orbiting stars.
View Article and Find Full Text PDFSun-like stars produce superflares roughly once per century.
Science
December 2024
Max-Planck-Institut für Sonnensystemforschung, Göttingen, Germany.
Stellar superflares are energetic outbursts of electromagnetic radiation that are similar to solar flares but release more energy, up to 10 erg on main-sequence stars. It is unknown whether the Sun can generate superflares and, if so, how often they might occur. We used photometry from the Kepler space observatory to investigate superflares on other stars with Sun-like fundamental parameters.
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