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Scalar-field dark matter models imply small oscillations of fundamental constants. These oscillations could result in observable variations of the magnetic field in a permanent magnet. We propose an experiment for detection of this type of…

High Energy Physics - Phenomenology · Physics 2024-11-18 I. M. Bloch , D. Budker , V. V. Flambaum , I. B. Samsonov , A. O. Sushkov , O. Tretiak

The most successful method used so far to search for extrasolar planets is the radial velocity technique, where periodical shifts on the measured emission from a star provide evidence for an orbiting planet. This method has been used on…

Instrumentation and Methods for Astrophysics · Physics 2013-08-15 Carlos Bacigalupo

We demonstrate that artificial bipolar structure can be detected using spectro-astrometry when the point spread function (PSF) of a point source suffers distortion in a relatively wide slit. Spectro-astrometry is a technique which allows us…

Astrophysics · Physics 2009-11-13 E. Brannigan , M. Takami , A. Chrysostomou , J. Bailey

Using quasar spectra from the SDSS survey, we constrain the possibility of photon-axion oscillations as a source of dimming of high redshift objects. Such a process has been suggested as an explanation of the apparent faintness of distant…

Astrophysics · Physics 2009-11-07 Edvard Mortsell , Ariel Goobar

We use the distribution, and particularly the skewness, of high redshift type Ia supernovae brightnesses relative to the low redshift sample to constrain the density of macroscopic compact objects (MCOs) in the universe. The data favors…

Astrophysics · Physics 2008-11-26 R. Benton Metcalf , Joseph Silk

We show that, by studying the arrival times of radio pulses from highly-magnetized transient beamed sources, it may be possible to detect light pseudo-scalar particles, such as axions and axion-like particles, whose existence could have…

High Energy Physics - Phenomenology · Physics 2015-06-04 Doron Chelouche , Eduardo I. Guendelman

Spectra in astroparticle physics are commonly approximated by simple power laws. The steeply falling nature of these power laws, however, makes the detection of additional components rather challenging. This holds true especially, if the…

High Energy Astrophysical Phenomena · Physics 2021-09-22 Tim Ruhe , Wolfgang Rhode

A new scalar particle with generic couplings to the standard-model particles is a possible source for the lepton anomalous magnetic moment and the violation of the weak equivalence principle. Here, one-loop contributions to the lepton…

High Energy Physics - Phenomenology · Physics 2025-09-12 Xitong Mei , Dongfeng Gao , Wei Zhao , Jin Wang , Mingsheng Zhan

We report on a search for dark matter axion conversion photons from the magnetosphere of the Galactic Center magnetar PSR J1745-2900 using spectra obtained from the Karl G. Jansky Very Large Array. No significant spectral features are…

Cosmology and Nongalactic Astrophysics · Physics 2020-09-23 Jeremy Darling

We present numerical calculations of the photon-light-pseudoscalar-boson conversion in the recently discovered binary pulsar system J0737-3039. Light pseudoscalar bosons (LPBs) oscillate into photons in the presence of strong magnetic…

Astrophysics · Physics 2009-11-13 Arnaud Dupays , Carlo Rizzo , Marco Roncadelli , Giovanni F. Bignami

Collective excitations in condensed matter systems, such as phonons and magnons, have recently been proposed as novel detection channels for light dark matter. We show that excitation of i) optical phonon polaritons in polar materials in an…

High Energy Physics - Phenomenology · Physics 2020-11-11 Andrea Mitridate , Tanner Trickle , Zhengkang Zhang , Kathryn M. Zurek

Ultralight dark matter induces time-dependent perturbations in the spacetime metric, enabling its gravitational direct detection. In this work, we propose using astrometry to detect dark matter. After reviewing the calculation of the metric…

High Energy Physics - Phenomenology · Physics 2025-08-06 Jeff A. Dror , Sarunas Verner

Experimental searches for axions or axion-like particles rely on semiclassical phenomena resulting from the postulated coupling of the axion to two photons. Sensitive probes of the extremely small coupling constant can be made by exploiting…

High Energy Physics - Experiment · Physics 2010-09-28 Aaron S. Chou

We present some bottom-up motivations of axions and other weakly interacting sub-eV particles (WISPs) coupling to photons. Typically, these light particles are strongly constrained by their production or interaction in astrophysical and…

High Energy Physics - Phenomenology · Physics 2009-10-13 Markus Ahlers

Background radiation fields pervade the Universe, and above a certain energy any $\gamma$-ray flux emitted by an extragalactic source should be attenuated due to $e^+e^-$ pair production. The opacity could be alleviated if photons…

High Energy Astrophysical Phenomena · Physics 2014-09-05 Manuel Meyer , Daniele Montanino , Jan Conrad

An alternative mechanism that dims high redshift supernovae without cosmic acceleration utilizes an oscillation of photons into a pseudo-scalar particle during transit. Since angular diameter distance measures are immune to the loss of…

Astrophysics · Physics 2011-05-12 Yong-Seon Song , Wayne Hu

Based on a sample of 355 quasars with significant optical polarization, we found that quasar polarization vectors are not randomly oriented over the sky as naturally expected. The probability that the observed distribution of polarization…

Astrophysics · Physics 2014-01-22 D. Hutsemekers , A. Payez , R. Cabanac , H. Lamy , D. Sluse , B. Borguet , J. -R. Cudell

If an ultralight scalar interacts with the electromagnetic fields of a compact rotating star, then a long-range scalar field is developed outside the star. The Coulomb-like profile of the scalar field to the leading order is equivalent to…

High Energy Physics - Phenomenology · Physics 2026-01-23 Tanmay Kumar Poddar , Amol Dighe

Axion-like particles are promising candidates to make up the dark matter of the universe, but it is challenging to design experiments that can detect them over their entire allowed mass range. Dark matter in general, and in particular…

High Energy Physics - Phenomenology · Physics 2018-04-30 Peter W. Graham , David E. Kaplan , Jeremy Mardon , Surjeet Rajendran , William A. Terrano , Lutz Trahms , Thomas Wilkason