528 citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- Los Alamos National LaboratoryUS74 papers
- Universidad Nacional Autónoma de MéxicoMX74 papers
- University of Maryland, College ParkUS74 papers
- Universidad Autónoma de ChiapasMX73 papers
- Universidad Michoacana de San Nicolás de HidalgoMX73 papers
- Instituto Politécnico NacionalMX72 papers
- National Institute of Astrophysics, Optics and ElectronicsMX72 papers
- University of UtahUS72 papers
- Michigan State UniversityUS71 papers
- Michigan Technological UniversityUS71 papers
- University of Wisconsin–MadisonUS71 papers
- Benemérita Universidad Autónoma de PueblaMX70 papers
87 papers
Search for TeV emission from spider millisecond pulsars with HAWC
R. Alfaro, E. Anita-Rangel, M. Araya +90
Millisecond pulsars (MSPs) are observed to emit multi-wavelength radiation, from radio to GeV. Spider MSPs, which interact with their low-mass companion in close orbit (orbital per…
The first 10years of the HAWC Gamma-Ray Observatory: science results
Anna Lia Longinotti, HAWC Collaboration
The High-Altitude Water Cherenkov (HAWC) Observatory, located on the slopes of the Sierra Negra volcano in Mexico, began operations in March 2015. Over the past decade, HAWC has en…
Combined dark matter search towards dwarf spheroidal galaxies with Fermi-LAT, HAWC, H.E.S.S., MAGIC, and VERITAS
LAT Collaboration, S. Abdollahi, L. Baldini +586
Dwarf spheroidal galaxies (dSphs) are excellent targets for indirect dark matter (DM) searches using gamma-ray telescopes because they are thought to have high DM content and a low…
A curvilinear framework for vector light fields
Leonardo S. Gonzalez-Aceves, Gabriela Flores-Cova, Blas M. Rodríguez-Lara +4
Vector beams are often regarded as non-separable superpositions of spatial and polarization degrees of freedom that satisfy the wave equation. This interpretation ties their polari…
Absence of TeV halos around millisecond pulsars
A. U. Abeysekara, R. Alfaro, C. Alvarez +82
TeV halos are extended very-high-energy (VHE; 0.1-100 TeV) gamma-ray emission around middle-aged pulsars. So far they have only been found around isolated pulsars, but it has been…
Extended TeV Halos May Commonly Exist around Middle-Aged Pulsars
A. Albert, R. Alfaro, C. Alvarez +81
Extended gamma-ray emission around isolated pulsars at TeV energies, also known as TeV halos, have been found around a handful of middle-aged pulsars. The halos are significantly m…
Noisy Cyclic Quantum Random Walk
G. Juarez Rangel, B. M. Rodríguez-Lara
We explore static noise in a discrete quantum random walk over a homogeneous cyclic graph, focusing on spectral and dynamical properties. Using a three-parameter unitary coin, we c…
Decoding physics identity: A Spanish-language adaptation on an instrument and its correlation with STEM achievement
O. I. González-Peña, G. Morán-Soto, B. M. Rodríguez-Lara
The representation of Spanish-speaking students in STEM identity literature, particularly in physics identity, is conspicuously minimal. This study addresses this gap with a two-pr…
Orbital Angular Momentum Coherent State Beams
D. Aguirre-Olivas, G. Mellado-Villaseñor, B. Perez-Garcia +1
We explore a family of paraxial beams constructed by the linear superposition of Laguerre-Gaussian beams, representing an optical analogue to generalized Lie group coherent…
Ultra-High-Energy Gamma-Ray Bubble around Microquasar V4641 Sgr
R. Alfaro, C. Alvarez, J. C. Arteaga-Velázquez +89
Microquasars are laboratories for the study of jets of relativistic particles produced by accretion onto a spinning black hole. Microquasars are near enough to allow detailed imagi…
Majorana constellations for optical scalar beams and vector fields
F. Torres-Leal, E. García Herrera, M. P. Morales Rodríguez +2
We explore Majorana stellar representation on the Riemann sphere for optical scalar beams and vector fields, leveraging the spin and orbital angular momentum of light. For scalar b…
Testing the Molecular Cloud Paradigm for Ultra-High-Energy Gamma Ray Emission from the Direction of SNR G106.3+2.7
R. Alfaro, C. Alvarez, J. C. Arteaga-Velázquez +87
Supernova remnants (SNRs) are believed to be capable of accelerating cosmic rays (CRs) to PeV energies. SNR G106.3+2.7 is a prime PeVatron candidate. It is formed by a head region,…
Analysis of the Emission and Morphology of the Pulsar Wind Nebula Candidate HAWC J2031+415
R. Alfaro, C. Alvarez, J. C. Arteaga-Velázquez +78
The first TeV gamma-ray source with no lower energy counterparts, TeV J2032+4130, was discovered by HEGRA. It appears in the third HAWC catalog as 3HWC J2031+415 and it is a bright…
Spatial light mode analogues of generalized quantum coherent states
M. P. Morales Rodríguez, E. García Herrera, O. Magaña Loaiza +3
We use the spatial degree of freedom of light modes to construct optical analogues of generalized quantum coherent states for Hermite- and Laguerre-Gauss modes. Our optical analogu…
A supersymmetry journey from the Jaynes-Cummings to the anisotropic Rabi model
A. Kafuri, F. H. Maldonado-Villamizar, A. Moroz +1
We revisit the Jaynes-Cummings and anti-Jaynes-Cummings model through the lens of Lie theory, aiming to highlight the efficacy of an operator-based approach for diagonalization. We…
Harmonic motion modes in parabolic GRIN fibers
A. Collado Hernández, F. Marroquín, B. M. Rodríguez-Lara
We report electromagnetic field modes solving the inhomogeneous Maxwell equations for parabolic gradient index fibers in the low refractive index contrast approximation. The first…
Galactic Gamma-Ray Diffuse Emission at TeV energies with HAWC Data
R. Alfaro, C. Alvarez, J. C. Arteaga-Velazquez +77
The Galactic gamma-ray diffuse emission (GDE) is emitted by cosmic rays (CRs), ultra-relativistic protons and electrons, interacting with gas and electromagnetic radiation fields i…
Coherent states of the Laguerre-Gauss modes
M. P. Morales Rodríguez, O. S. Magaña-Loaiza, B. Perez-Garcia +3
Large quantum photonic systems hold promise for surpassing classical computational limits, yet their state preparation remains a challenge. We propose an alternative approach to st…
HAWC Study of Very-High-Energy -ray Spectrum of HAWC J1844-034
HAWC Collaboration, A. Albert, C. Alvarez +74
Recently, the region surrounding eHWC J1842-035 has been studied extensively by gamma-ray observatories due to its extended emission reaching up to a few hundred TeV and potential…
Optical coupling control of isolated mechanical resonators
F. E. Onah, B. R. Jaramillo-Ávila, F. H. Maldonado-Villamizar +1
We present a Hamiltonian model describing two pairs of mechanical and optical modes under standard optomechanical interaction. The vibrational modes are mechanically isolated from…
Continuous-time quantum harmonic oscillator state engineering
E. García Herrera, F. Torres-Leal, B. M. Rodríguez-Lara
The center of mass motion of trapped ions and neutral atoms is suitable for approximation by a time-dependent driven quantum harmonic oscillator whose frequency and driving strengt…
The High-Altitude Water Cherenkov (HAWC) Observatory in México: The Primary Detector
A. U. Abeysekara, A. Albert, R. Alfaro +140
The High-Altitude Water Cherenkov (HAWC) observatory is a second-generation continuously operated, wide field-of-view, TeV gamma-ray observatory. The HAWC observatory and its analy…
Detailed Analysis of the TeV γ-Ray Sources 3HWC J1928+178, 3HWC J1930+188, and the New Source HAWC J1932+192
A. Albert, R. Alfaro, C. Alvarez +91
The latest High Altitude Water Cherenkov (HAWC) point-like source catalog up to 56 TeV reported the detection of two sources in the region of the Galactic plane at galactic longitu…
Searching for TeV Dark Matter in Irregular dwarf galaxies with HAWC Observatory
R. Alfaro, C. Alvarez, J. C. Arteaga-Velázquez +69
We present the results of dark matter (DM) searches in a sample of 31 dwarf irregular (dIrr) galaxies within the field of view of the HAWC Observatory. dIrr galaxies are DM dominat…