Peer Revenue Smith, Jones, et al.

$TURB turbulence

Counts every occurrence of turbulence in arXiv titles and abstracts.
Price24.730.00% today
Hits14Wed 23 Sep · usual 13
Yield0.56%latest day
Dividends · 30d0.14per share

Price

Daily candles and credits traded. Today's candle is live.

Trade

Every player starts with 10,000 credits of play money.

Sign in to trade

Daily arXiv hits

settled still being announced 7-day average

Where it's used · 30 days

  1. Fluid Dynamics physics.flu-dyn 45%
  2. Plasma Physics physics.plasm-ph 12%
  3. Astrophysics of Galaxies astro-ph.GA 9%
  4. Solar and Stellar Astrophysics astro-ph.SR 6%
  5. Instrumentation and Methods for Astrophysics astro-ph.IM 5%
  6. High Energy Astrophysical Phenomena astro-ph.HE 4%
  7. Everything else 20%

Share of hits by each paper's main arXiv category, from 168 papers.

Latest papers

  1. Thermal behaviour of settling heavy inertial particles in turbulent natural convection physics.flu-dyn · 24 Sep · 1 hit

    …convection setup, where a uniform mean temperature gradient drives statistically homogeneous convective turbulence seeded with passive inertial particles. We quantify the effects of dynamic and thermal inertia on…

  2. Relative periodic orbits in spatially extended Kolmogorov turbulence: from global to localized recurrence physics.flu-dyn · 24 Sep · 2 hits

    Recurrent invariant solutions provide a dynamical framework for interpreting turbulence, but their computation becomes increasingly difficult in spatially extended flows, where close…

  3. AI-Accelerated Gyrokinetic Predictions of Turbulent Transport for Stellarator Design Optimization and Experimental Planning physics.plasm-ph · 23 Sep · 3 hits

    …positions in the plasma, and gradient scale lengths. In this paper, we demonstrate the use of the AI-based turbulence surrogate in the optimization of stellarator magnetic equilibrium and to speed up stellarator…

  4. Just a Phase? Weakening Vertical Shear Instability Explains Class II Disk Morphologies: Simulations with dust coagulation, sedimentation, thermal relaxation, and backreaction astro-ph.EP · 23 Sep · 2 hits

    The Vertical Shear Instability (VSI) is known to create turbulence and strong vertical mixing in protoplanetary disks if thermal relaxation is sufficiently fast. In…

  5. Dynamical and statistical properties of large scales in turbulence physics.flu-dyn · 23 Sep · 4 hits

    …concerning the properties of scales larger than the forcing scale in turbulent flows. In three-dimensional turbulence, when the power driving the flow is injected at a well-defined scale, the injection scale…

  6. Long time well-posedness and wave turbulence limit for a quadratic non-lienar Schr{\"o}dinger equation with well prepared random initial data math.AP · 23 Sep · 1 hit

    We prove a long time well-posedness result for a quadratic non-linear Schr{\"o}dinger equation with random…

  7. Anisotropy and energy distribution of leptons and photons in radiative relativistic Alfv\'{e}nic turbulence physics.plasm-ph · 23 Sep · 2 hits

    The anisotropic evolution of relativistic particles in magnetically dominated Alfv\'{e}nic turbulence is a fundamental process governing nonthermal emissions in high-energy astrophysical environments.…

  8. Transition from a weak-elastic to an elastic-activated regime in two-dimensional polymeric turbulence physics.flu-dyn · 23 Sep · 2 hits

    …the effects of dilute polymers on flow structure, statistical properties and energy transfer in 2D turbulence. As the Weissenberg number (Wi) increases, the flow undergoes a sharp but continuous crossover…

Dividends per share

7 days0.14
30 days0.14
Since IPO0.14
DayHitsPer share
Wed 23 Sep140.14

Recent trades

When (UTC)SideSharesCreditsPrice after
No trades yet. Be the first author.