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Self-interaction among the neutrinos in the early Universe has been proposed as a solution to the Hubble tension, a discrepancy between the measured values of the Hubble constant from CMB and low-redshift data. However, flavor-universal…

High Energy Physics - Phenomenology · Physics 2021-09-09 Anirban Das

Dark matter particles can be gravitationally trapped by celestial bodies, motivating searches for localized annihilation or decay. If neutrinos are among the decay products, then IceCube and other neutrino observatories could detect them.…

High Energy Physics - Phenomenology · Physics 2022-05-02 Matthew Saveliev , Jeffrey Hyde

We have imaged the disc of the young star HL Tau using the VLA at 1.3 cm, with 0.08" resolution (as small as the orbit of Jupiter). The disc is around half the stellar mass, assuming a canonical gas-mass conversion from the measured mass in…

Astrophysics · Physics 2009-11-13 J. S. Greaves , A. M. S. Richards , W. K. M. Rice , T. W. B. Muxlow

We study ultrahigh energy astrophysical neutrinos and the contribution of tau neutrinos from neutrino oscillations, relative to the contribution of the other flavors. We show the effect of tau neutrino regeneration and tau energy loss as…

High Energy Physics - Phenomenology · Physics 2009-11-11 J. Jones , I. Mocioiu , M. H. Reno , I Sarcevic

We propose the first experimental test of the inelastic boosted dark matter hypothesis, capitalizing on the new physics potential with the imminent data taking of the ProtoDUNE detectors. More specifically, we explore various experimental…

High Energy Physics - Phenomenology · Physics 2019-02-15 Animesh Chatterjee , Albert De Roeck , Doojin Kim , Zahra Gh. Moghaddam , Jong-Chul Park , Seodong Shin , Leigh H. Whitehead , Jaehoon Yu

We present a model of the circumstellar environment of the so-called ``Butterfly Star'' in Taurus (IRAS 04302+2247). The appearance of this young stellar object is dominated by a large circumstellar disk seen edge-on and the light…

Astrophysics · Physics 2008-11-26 Sebastian Wolf , Deborah L. Padgett , Karl R. Stapelfeldt

Astrophysical neutrinos are powerful tools to investigate the fundamental properties of particle physics through their flavor content. In this paper, we perform the first general new physics study on ultra high energy neutrino flavor…

High Energy Physics - Phenomenology · Physics 2015-10-21 Carlos A. Argüelles , Teppei Katori , Jordi Salvado

The potential for artificial intelligence (AI) to take over the work of physicists should be treated with glee. Here I evaluate one of the scientific discoveries in quantum photonics made by a leading AI in the field, in order to try and…

Quantum Physics · Physics 2023-03-13 Terry Rudolph

We present a high spatial resolution, 10-20 micron survey of 65 T Tauri binary stars in Taurus, Ophiuchus, and Corona Australis using the Keck 10 m telescopes. Designed to probe the inner ~1 AU region of the circumstellar disks around the…

Astrophysics · Physics 2007-05-23 C. McCabe , A. M. Ghez , L. Prato , G. Duchene , R. S. Fisher , C. Telesco

Celestial observations often exhibit inexplicable planetary dependencies when the timing of an observable is projected onto planetary heliocentric positions. This is possible only for incident, non-relativistic streams. Notably, the…

The chemical evolution of fluorine is still a matter of debate in Galactic archaeology, especially at low metallicities, where it is particularly challenging to obtain the corresponding chemical abundances from observations. We present here…

Astrophysics of Galaxies · Physics 2025-11-03 Valeria Grisoni , Federico Rizzuti , Gabriele Cescutti

The discovery of extremely zirconium- and lead-rich surfaces amongst a small subgroup of hot subdwarfs has provoked questions pertaining to chemical peculiarity in hot star atmospheres and about their evolutionary origin. With only three…

Solar and Stellar Astrophysics · Physics 2020-01-08 N. Naslim , C. S. Jeffery , V. M. Woolf

We report here our latest search for molecular outflows from young brown dwarfs and very low-mass stars in nearby star-forming regions. We have observed three sources in Taurus with the Submillimeter Array and the Combined Array for…

Solar and Stellar Astrophysics · Physics 2015-06-22 Ngoc Phan-Bao , Chin-Fei Lee , Paul T. P. Ho , Cuong Dang-Duc , Di Li

The quark matter may have great implications in astrophysical studies, which could appear in the early Universe, in compact stars, and/or as cosmic rays. After a general review of astrophysical quark matter, the density-dominated quark…

Astrophysics · Physics 2014-10-13 R. X. Xu

We present the results of a search for new members of the Taurus star-forming region using data from the Spitzer Space Telescope and the XMM-Newton Observatory. We have obtained optical and near-infrared spectra of 44 sources that exhibit…

Astrophysics of Galaxies · Physics 2014-11-20 K. L. Luhman , E. E. Mamajek , P. R. Allen , K. L. Cruz

The recent discovery of ``ultra-hot'' ($P < 1$ day) Neptunes has come as a surprise: some of these planets have managed to retain gaseous envelopes despite being close enough to their host stars to trigger strong photoevaporation and/or…

Quanz and coworkers have reported the discovery of the coolest known member of the Taurus star-forming complex (L2+/-0.5) and Barrado and coworkers have identified a possible protostellar binary brown dwarf in the same region. We have…

Astrophysics of Galaxies · Physics 2015-05-19 K. L. Luhman , E. E. Mamajek

There is a puzzling contradiction: direct observations favor a low-mass density universe, but the only model which fits universe structure over more than three orders of magnitude in distance scale has a mix of hot (neutrino) and cold dark…

High Energy Physics - Phenomenology · Physics 2007-05-23 David O. Caldwell

The importance and signatures of cosmic tau--(anti)neutrinos have been studied for upward-- and downward--going $\mu^-+\mu^+$ and hadronic shower event rates relevant for present and future underground water or ice detectors, utilizing the…

High Energy Physics - Phenomenology · Physics 2009-11-11 E. Reya , J. Roediger