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A search for solar axions and axion-like particles produced in the $p+d\rightarrow\rm{^3He}+A~(5.5\rm{ ~MeV})$ reaction was performed using the complete dataset of the Borexino detector (3995 days of measurement live-time). The following…

高能物理 - 实验 · 物理学 2025-10-23 Borexino Collaboration

We investigate the possibility of detecting 14.4 keV and 9.4 keV solar axions and axion-like particles that could be produced in the M1 nuclear transitions of $^{57}$Fe and $^{83}$Kr, respectively. To do so, we used data from soft X-ray…

高能物理 - 唯象学 · 物理学 2026-05-26 Tanmoy Kumar , Newton Nath

Light axion fields, if they exist, can be sourced by neutron stars due to their coupling to nuclear matter, and play a role in binary neutron star mergers. We report on a search for such axions by analysing the gravitational waves from the…

高能物理 - 唯象学 · 物理学 2021-10-20 Jun Zhang , Zhenwei Lyu , Junwu Huang , Matthew C. Johnson , Laura Sagunski , Mairi Sakellariadou , Huan Yang

Recent stellar evolution computations indicate that massive stars in the range ~ 20 - 30 Msun are located in the blue supergiant (BSG) region of the Hertzsprung-Russell diagram at two different stages of their life: immediately after the…

太阳与恒星天体物理 · 物理学 2015-06-22 C. Georgy , H. Saio , G. Meynet

We use a highly complete subset of the GAMA-II redshift sample to fully describe the stellar mass dependence of close-pairs and mergers between 10^8 Msun and 10^12 Msun. Using the analytic form of this fit we investigate the total stellar…

If axion-like particles (ALPs) exist, photons can convert to ALPs on passage through regions containing magnetic fields. The magnetised intracluster medium of large galaxy clusters provides a region that is highly efficient at ALP-photon…

高能天体物理现象 · 物理学 2018-06-27 Linhan Chen , Joseph P. Conlon

We explore the sensitivity of massive stars to neutrino magnetic moments. We find that the additional cooling due to the neutrino magnetic moments bring about qualitative changes to the structure and evolution of stars in the mass window 7…

天体物理学 · 物理学 2010-01-05 Alexander Heger , Alexander Friedland , Maurizio Giannotti , Vincenzo Cirigliano

The production of very-high-energy (VHE, $E_{\gamma} \gtrsim 100$ GeV) gamma rays resulting from the scattering of high-energy cosmic-ray protons off axion-like particles (ALPs) populating the dark matter halo of the Milky Way is…

高能物理 - 唯象学 · 物理学 2026-03-20 Victor P. Goncalves , Emmanuel Moulin , Igor Reis , Aion Viana

The CIBER collaboration released their first observational data of the Cosmic IR background (CIB) radiation, which has significant excesses at around the wavelength $\sim$ 1 $\mu$m compared to theoretically-inferred values. The amount of…

高能物理 - 唯象学 · 物理学 2017-10-04 Kazunori Kohri , Hideo Kodama

The post-helium burning evolution of stars from 7 to 11 solar masses is complicated by the lingering effects of degeneracy and off-center ignition. Here stars in this mass range are studied using a standard set of stellar physics. Two…

太阳与恒星天体物理 · 物理学 2015-09-09 S. E. Woosley , Alexander Heger

Axion-like particles (ALPs) can oscillate to photons and vice versa in electromagnetic fields. The photon-ALP oscillation provides an attractive solution to the apparent transparency of the Universe to TeV photons. The allowed parameter…

高能物理 - 唯象学 · 物理学 2019-06-26 Yun-Feng Liang , Cun Zhang , Zi-Qing Xia , Lei Feng , Qiang Yuan , Yi-Zhong Fan

The observed spatial distribution of $\gamma-$ray bursts indicates that they probably originate at cosmological distances. At this distance scale their variability timescale and flux above MeV imply an initial optical-depth to pair…

天体物理学 · 物理学 2010-01-06 Abraham Loeb

For searching beyond Standard Model physics, stars are laboratories which complement terrestrial experiments. Massless neutrinos in the Standard Model of particle physics cannot have a magnetic moment, but massive neutrinos have a finite…

太阳与恒星天体物理 · 物理学 2020-10-07 Kanji Mori , A. Baha Balantekin , Toshitaka Kajino , Michael A. Famiano

In non-hadronic axion models, which have a tree-level axion-electron interaction, the Sun produces a strong axion flux by bremsstrahlung, Compton scattering, and axio-recombination, the "BCA processes." Based on a new calculation of this…

Axions are a promising dark matter candidate that were motivated to solve the strong CP problem and that may also address the cosmological matter-antimatter asymmetry. Axion-photon conversion is possible in the presence of the strong…

宇宙学与河外天体物理 · 物理学 2020-08-26 Jeremy Darling

Kaluza-Klein (KK) axions appear in theories with extra dimensions as higher mass, significantly shorter lifetime, excitations of the Peccei-Quinn axion. When produced in the Sun, they would remain gravitationally trapped in the solar…

We argue that tracing star formation histories with ESA's space mission GAIA using main sequence turn-off (MSTO) point dating will mainly be effective in cases of mild interstellar extinction (E(B-V)<0.5). For higher reddenings the MSTO…

天体物理学 · 物理学 2007-05-23 A. Kucinskas , L. Lindegren , T. Tanabe , V. Vansevicius

The QCD axion and axion-like particles are compelling candidates for galactic dark matter. Theoretically, axions can convert into photons in the presence of a strong external magnetic field, which means it is possible to search for them…

Transformation of CMB photons into light pseudoscalar particles at post big bang nucleosynthesis epoch is considered. Using the present day value of a large scale magnetic field to estimate it at earlier cosmological epochs, the oscillation…

高能物理 - 唯象学 · 物理学 2014-09-16 Damian Ejlli , Alexander D. Dolgov