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icon https://en.wikipedia.org/wiki/Angular_velocity_tensor

Angular velocity tensor

Because s {\displaystyle \mathbf {s} } is an arbitrary vector, from nondegeneracy of scalar product follows Ω r = ω × r {\displaystyle \Omega \mathbf {r}
icon http://arxiv.org/abs/astro-ph/0310480v1

Acceleration and Dissipation in Relativistic Winds

I argue that ideal MHD relativistic winds are always limited in practice to asymptotic 4-velocity $γ_\infty \approx σ_0^{1/3}$ and asymptotic magnetization $σ\sim σ_0^{2/3} \gg 1$, where $σ_0$ is...
icon https://www.bing.com/ck/a?!&&p=1991f4081ca8e0e8f83dd6447499b1ada260ecb353a44136ef1b9f579723457fJmltdHM9MTc3MjY2ODgwMA&ptn=3&ver=2&hsh=4&fclid=1a3e6994-ad23-63d6-031a-7e80ac32620f&u=a1aHR0cHM6Ly93d3cudHJhdmVsb2NpdHkuY29tL0hvdGVscz9tc29ja2lkPTFhM2U2OTk0YWQyMzYzZDYwMzFhN2U4MGFjMzI2MjBm&ntb=1

Cheap Hotels: Book Hotel Deals With Our Hotel Finder | Travelocit...

Use Travelocity's Hotel Finder to book your next hotel, backed by our Price Match Guarantee. Search hotel deals, read reviews and Wander Wisely!
icon http://arxiv.org/abs/1911.06454v1

Estimating adaptive cruise control model parameters from on-board...

Two new methods are presented for estimating car-following model parameters using data collected from the Adaptive Cruise Control (ACC) enabled vehicles. The vehicle is assumed to follow a constant ti...
icon http://arxiv.org/abs/2303.06803v2

Energy flux and high-order statistics of hydrodynamic turbulence

We use the Dyson-Wyld diagrammatic technique to analyze the infinite series for the correlation functions of the velocity in the hydrodynamic turbulence. We demonstrate the fundamental role played by ...
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General Discussion - Sufficient Velocity

Threads 5.2K Messages 91.6K Chimera (A Bloodstained Mantle) vs Argenta (The Brighter Side of Gray)
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Creative Forums - Sufficient Velocity

For all user generated art and music, as well discussions about art and music in the wider world.
icon http://arxiv.org/abs/1910.03626v2

In the Presence of a Wrecking Ball: Orbital Stability in the HR 5...

Discoveries of exoplanets using the radial velocity method are progressively reaching out to increasingly longer orbital periods as the duration of surveys continues to climb. The improving sensitivit...
icon http://arxiv.org/abs/2012.07779v1

Rate-dependent adhesion of viscoelastic contacts. Part I: contact...

In this work, we investigate dissipative effects involved during the detachment of a smooth spherical glass probe from a viscoelastic silicone substrate patterned with micro-asperities. As a baseline,...
icon http://arxiv.org/abs/astro-ph/0509112v4

Extrasolar planets and brown dwarfs around A-F type stars. II. A ...

We present here the detection of a planet orbiting around the F6V star HD 33564. The radial velocity measurements, obtained with the ELODIE echelle spectrograph at the Haute-Provence Observatory, show...
icon http://arxiv.org/abs/astro-ph/9601151v2

The Dipole Observed in the COBE DMR Four-Year Data

The largest anisotropy in the cosmic microwave background (CMB) is the $\approx 3$ mK dipole assumed to be due to our velocity with respect to the CMB. Using the four year data set from all six channe...
icon http://arxiv.org/abs/1812.10603v2

Self-consistent Force Scheme in the Discrete Boltzmann Equation

In the work of N. Martys et al. [Nicos S. Martys, Xiaowen Shan, Hudong Chen, Phys. Rev. E, Vol. 58, Num.5, 1998 ], a self-consistent force term to any order in the Boltzmann-BKG equation is derived by...
icon http://arxiv.org/abs/1201.1046v1

Why variable AGB stars with Long Secondary Periods aren't binarie...

Roughly 30% of variable AGB stars show a Long Secondary Period, or LSP. These LSPs have posed something of a problem in recent years and their cause remains a mystery. By combining VLT-derived velocit...
icon https://en.wikipedia.org/wiki/Velocity-addition_formula

Velocity-addition formula

which expressions for the primed velocities were obtained using the standard recipe by replacing v by –v and swapping primed and unprimed coordinates.
icon http://arxiv.org/abs/1701.03668v1

Imprints of Zero-Age Velocity Dispersions and Dynamical Heating o...

Observations of stars in the the solar vicinity show a clear tendency for old stars to have larger velocity dispersions. This relation is called the age-velocity dispersion relation (AVR) and it is be...
icon http://arxiv.org/abs/1509.02038v1

Dissociation energies of AgRG (RG = Ar, Kr, Xe) and AgO molecules...

The near ultraviolet photodissociation dynamics of silver atom rare gas dimers have been studied by velocity map imaging. AgRG (RG = Ar, Kr, Xe) species generated by laser ablation are excited in the ...
icon http://arxiv.org/abs/1401.5929v1

Crawling on directional surfaces

In this paper we study crawling locomotion based on directional frictional interactions, namely, frictional forces that are sensitive to the sign of the sliding velocity. Surface interactions of this ...
icon http://arxiv.org/abs/1710.01138v1

The TROY project: Searching for co-orbital bodies to known planet...

The detection of Earth-like planets, exocomets or Kuiper belts show that the different components found in the solar system should also be present in other planetary systems. Trojans are one of these ...
icon http://arxiv.org/abs/0801.1834v5

Non-dispersive wavepacket solutions of the Schrodinger equation

The free Schrodinger equation has constant velocity wavepacket solutions ψ_{\bf v} of the form ψ= f({\bf r} - {\bf v}t) e^{- i m c^2 t / 2}. These solutions are eigenvectors of a momentum operator {...
icon http://arxiv.org/abs/quant-ph/0401104v1

Poincare group operators with 4-vector position

We present a new set of massless Poincaré group operators Hermitian with respect to the $ 1 / r $ inner product space, which have quasi-plane wave energy-momentum eigenfunctions having velocity $ c $...