arxiv.org/abs/physics/0008013v4
The group velocity for pulses in an optical medium can be negative at frequencies between those of a pair of laser-pumped spectral lines. The gain medium then can amplify the leading edge of a pulse resulting in a time advance of the pulse when it...
arxiv.org/abs/1708.09360v2
We study a 1D fluid mechanics model with nonlocal velocity. The equation can be viewed as a fractional porous medium flow, a 1D model of the quasi-geostrophic equation, and also a special case of Euler-Alignment system. For strictly positive smooth i...
arxiv.org/abs/1402.5233v1
Presented in this paper is an actuator concept, called a Parallel Force/Velocity Actuator (PFVA), that combines two fundamentally distinct actuators (one using low gear reduction or even direct drive, which we will call a Force Actuator (FA) and the...
www.bing.com/ck/a?!&&p=05f42334e4d7c5cfc1d567190d786abb4c7d6c0e977e6957fcf9034ff92bb75bJmltdHM9MTc3MjQ5NjAwMA&ptn=3&ver=2&hsh=4&fclid=1fadbb37-70e3-65e2-1179-ac25713e64a0&u=a1aHR0cHM6Ly93d3cucmVkZGl0LmNvbS9yL3ZlbG9jaXR5YmFua2luZy9jb21tZW50cy8xOWVrcmJ5L2JsYW5rX3ZlbG9jaXR5X2Jhbmtpbmdfc3ByZWFkc2hlZXQv&ntb=1
Blank Velocity Banking Spreadsheet So I'm very pleased my spreadsheet has been requested many times (that it's free probably helped somewhat). It's been a pain to have to ask for email addresses …
arxiv.org/abs/1306.6496v1
We study the systematic bias introduced when selecting the spectroscopic redshifts of brighter cluster galaxies to estimate the velocity dispersion of galaxy clusters from both simulated and observational galaxy catalogues. We select clusters with Ng...
arxiv.org/abs/1907.12509v2
Adopting the Standard Halo Model (SHM) of an isotropic Maxwellian velocity distribution for dark matter (DM) particles in the Galaxy, the most stringent current constraints on their spin-dependent scattering cross-section with nucleons come from the...
arxiv.org/abs/2203.06189v1
We prove the equivalence of two holographic computations of the butterfly velocity in higher-derivative theories with Lagrangian built from arbitrary contractions of curvature tensors. The butterfly velocity characterizes the speed at which local per...
github.com/julianshapiro/velocity
Accelerated JavaScript animation. (⭐ 17241)
arxiv.org/abs/2602.13512v1
The higher-order mean velocity profile in the convective atmospheric boundary layer (CBL) is derived using the method of matched asymptotic expansions. The universal expansion coefficients are obtained using field measurement data. The profile accoun...
arxiv.org/abs/2102.00636v2
Wireless communication systems are to use millimeter-wave (mmWave) spectra, which can enable extra radar functionalities. In this paper, we propose a multi-target velocity estimation technique using IEEE 802.11ad waveform in a vehicle-to-vehicle (V2V...
www.bing.com/ck/a?!&&p=75509ef28806ae294238379c36cc4292f7203c83f26bc2d8a2421807ce10fd47JmltdHM9MTc3MjQ5NjAwMA&ptn=3&ver=2&hsh=4&fclid=1fb85d1e-dfee-65ee-3048-4a0fdea464eb&u=a1aHR0cHM6Ly92ZWxvY2l0eWRhbmNlY2VudGVyLm9yZy8&ntb=1
Velocity is Seattle’s center dedicated to contemporary dance, and provides classes for adults, support to local artists, and international summer festivals.
arxiv.org/abs/1704.07569v2
We introduce a hybridizable discontinuous Galerkin method for the incompressible Navier--Stokes equations for which the approximate velocity field is pointwise divergence-free. The method builds on the method presented by Labeur and Wells [SIAM J. Sc...
arxiv.org/abs/2003.09732v1
We introduce the stellar sample of the WIYN Open Cluster Study radial-velocity survey for the rich open cluster NGC 7789 (1.6 Gyr, [Fe/H] = +0.02). This sample lies within an 18$'$ circular radius from the cluster center (10 pc in projection, or abou...
arxiv.org/abs/1405.6679v1
Observations of colliding galaxy clusters with high relative velocity probe the tail of the halo pairwise velocity distribution with the potential of providing a powerful test of cosmology. As an example it has been argued that the discovery of the B...
arxiv.org/abs/2012.07137v1
The space missions TESS and PLATO plan to double the number of 4000 exoplanets already discovered and will measure the size of thousands of exoplanets around the brightest stars in the sky, allowing ground-based radial velocity spectroscopy follow-up...
arxiv.org/abs/1202.0780v1
An extended XMM-Newton observation of the Seyfert 1 galaxy NGC 4051 in 2009 detected a photo-ionized outflow with a complex absorption line velocity structure and a broad correlation of velocity with ionization parameter, shown in Pounds et al (2011)...
arxiv.org/abs/2206.14902v1
Falling coffee filters are a common object of study in introductory physics laboratory classes. They are usually used to demonstrate the terminal velocity, and determine how the drag force depends on this velocity. However they can also be used to de...
arxiv.org/abs/astro-ph/9710332v1
We investigate the peculiar velocity field due to long cosmic strings in several cosmological models and analyse the influence of a nonscaling behaviour of the string network, which is expected in open cosmological models or models with a cosmologi...
arxiv.org/abs/1410.3597v1
In this paper we discuss the collisionless transport equations, continuity, momentum and energy conservation, derived from a kinetic exospheric model of the solar wind based on a kappa velocity distribution function of the electrons. The model is sta...
arxiv.org/abs/1304.2154v1
In the present paper, the proton velocity distribution function (VDF)in the solar wind is determined by solving numerically the kinetic evolution equation. We compare the results obtained when considering the effects of ex- ternal forces and Coulomb...