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PERFECT FLUID

  • Perfect fluid
  • Fluid fully characterized by its density and isotropic pressure

    In physics, a perfect fluid or ideal fluid is a fluid that can be completely characterized by its rest frame mass density ρ m {\displaystyle \rho _{m}}

    Perfect fluid

    Perfect_fluid

  • Fluid
  • Liquid, gas, or other continuously deforming and flowing material

    compressibility are called perfect fluids. Matter Liquid Gas Supercritical fluid "Fluid | Definition, Models, Newtonian Fluids, Non-Newtonian Fluids, & Facts". Encyclopedia

    Fluid

    Fluid

  • Energy condition
  • Mathematics of general relativity

    context of perfect fluids. Finally, there are proposals for extension of the energy conditions to spacetimes containing non-perfect fluids, where the

    Energy condition

    Energy_condition

  • Fluid solution
  • Class of exact solutions to Einstein's field equations

    a fluid. In astrophysics, fluid solutions are often employed as stellar models, since a perfect gas can be thought of as a special case of a perfect fluid

    Fluid solution

    Fluid_solution

  • Wahlquist fluid
  • Perfect fluid solution in general relativity

    In general relativity, the Wahlquist fluid is an exact rotating perfect fluid solution to Einstein's equation with equation of state corresponding to constant

    Wahlquist fluid

    Wahlquist_fluid

  • Big Bang
  • Physical theory of the cosmos

    in all directions regardless of location. A perfect fluid has no viscosity; the pressure of a perfect fluid is proportional to its density. These ideas

    Big Bang

    Big Bang

    Big_Bang

  • Equation of state (cosmology)
  • Equation of state in cosmology

    In cosmology, the equation of state of a perfect fluid is characterized by a dimensionless number w {\displaystyle w} , equal to the ratio of its pressure

    Equation of state (cosmology)

    Equation of state (cosmology)

    Equation_of_state_(cosmology)

  • Friedmann equations
  • Equations in physical cosmology

    gravitation for the Friedmann–Lemaître–Robertson–Walker metric and a perfect fluid with a given mass density ρ and pressure p. The equations for negative

    Friedmann equations

    Friedmann equations

    Friedmann_equations

  • Static spherically symmetric perfect fluid
  • Class of exact solutions to the Einstein field equations

    spherically symmetric perfect fluid (ssspf) solution is a spacetime equipped with suitable tensor fields which models a static round ball of a fluid with isotropic

    Static spherically symmetric perfect fluid

    Static_spherically_symmetric_perfect_fluid

  • Dust solution
  • Class of exact solutions to Einstein's field equations

    density of a perfect fluid that has positive mass density but vanishing pressure. Dust solutions are an important special case of fluid solutions in general

    Dust solution

    Dust_solution

  • Euler equations (fluid dynamics)
  • Set of quasilinear hyperbolic equations governing adiabatic and inviscid flow

    In fluid dynamics, the Euler equations are a set of partial differential equations governing adiabatic and inviscid flow. They are named after Leonhard

    Euler equations (fluid dynamics)

    Euler equations (fluid dynamics)

    Euler_equations_(fluid_dynamics)

  • Hydrostatic equilibrium
  • State of balance between external forces on a fluid and internal pressure gradient

    In fluid mechanics, hydrostatic equilibrium, also called hydrostatic balance and hydrostasy, is the condition of a fluid or plastic solid at rest, which

    Hydrostatic equilibrium

    Hydrostatic equilibrium

    Hydrostatic_equilibrium

  • History of fluid mechanics
  • fluid mechanics The history of fluid mechanics is a fundamental strand of the history of physics and engineering. The study of the movement of fluids

    History of fluid mechanics

    History of fluid mechanics

    History_of_fluid_mechanics

  • Fluid dynamics
  • Aspects of fluid mechanics involving fluid flow

    physical chemistry, and engineering, fluid dynamics is a subdiscipline of fluid mechanics that describes the flow of fluids – liquids and gases. It has several

    Fluid dynamics

    Fluid dynamics

    Fluid_dynamics

  • Solutions of the Einstein field equations
  • Aspect of general relativity

    u_{a}} is the fluid's 4-velocity vector field, and p {\displaystyle p} is the pressure. Non-interacting dust ( a special case of perfect fluid ): T a b =

    Solutions of the Einstein field equations

    Solutions_of_the_Einstein_field_equations

  • Tolman–Oppenheimer–Volkoff equation
  • Equation explaining structure of a spherical body of isotropic material

    c^{2}} and it is negative. Let us assume a static, spherically symmetric perfect fluid. The metric components are similar to those for the Schwarzschild metric:

    Tolman–Oppenheimer–Volkoff equation

    Tolman–Oppenheimer–Volkoff_equation

  • Exact solutions in general relativity
  • Fluid solutions: T α β {\displaystyle T^{\alpha \beta }} must arise entirely from the stress–energy tensor of a fluid (often taken to be a perfect fluid);

    Exact solutions in general relativity

    Exact_solutions_in_general_relativity

  • Newman–Janis algorithm
  • Technique to find exact solutions to Einstein field equations

    proved the uniqueness of certain solutions. In particular, the only perfect fluid solution generated by NJA is the Kerr metric and the only Petrov type

    Newman–Janis algorithm

    Newman–Janis_algorithm

  • Sonic black hole
  • Acoustic analogue of a black hole in which sound plays the role of light

    from a black hole. Sonic black holes are possible because phonons in perfect fluids exhibit the same properties of motion as fields, such as gravity, in

    Sonic black hole

    Sonic_black_hole

  • Supplee's paradox
  • Paradox in relativistic physics

    immersed in a fluid subject to an ambient gravitational field. If a bullet has neutral buoyancy when it is at rest in a perfect fluid and then it is

    Supplee's paradox

    Supplee's_paradox

  • Einstein field equations
  • Field-equations in general relativity

    (1986). "Self-similar spatially homogeneous cosmologies: orthogonal perfect fluid and vacuum solutions". Class. Quantum Grav. 3 (6): 1105–1124. Bibcode:1986CQGra

    Einstein field equations

    Einstein_field_equations

  • Semen
  • Reproductive biofluid of male or hermaphroditic animals

    as seminal fluid, is a bodily fluid that contains spermatozoa from the male gonads of animals. In humans and placental mammals, seminal fluid is ejaculated

    Semen

    Semen

    Semen

  • Asymptotically flat spacetime
  • Lorentzian manifold where curvature vanishes at large distances

    star should be a perfect fluid or dust rather than a vacuum, and then argues that there exist no asymptotically flat rotating perfect fluid solutions in general

    Asymptotically flat spacetime

    Asymptotically_flat_spacetime

  • Raychaudhuri equation
  • Result in general relativity

    each blob of fluid being provided by the pressure of surrounding fluid) counteracts the Raychaudhuri scalar, which for a perfect fluid in four dimensions

    Raychaudhuri equation

    Raychaudhuri_equation

  • Van Stockum dust
  • Exact solution of the Einstein field equations

    cylindrically symmetric perfect fluid solution in which the fluid exhibits rigid rotation. That is, we demand that the world lines of the fluid particles form

    Van Stockum dust

    Van_Stockum_dust

  • Event horizon
  • Region in spacetime from which nothing can escape

    Universe as composed of non-interacting constituents, each one being a perfect fluid. If a particle is moving at a constant velocity in a non-expanding universe

    Event horizon

    Event horizon

    Event_horizon

  • Schwarzschild coordinates
  • Coordinate system in black hole physics

    Einstein field equation is static, but this is certainly not true for perfect fluids. The extension of the exterior region of the Schwarzschild vacuum solution

    Schwarzschild coordinates

    Schwarzschild_coordinates

  • Gödel metric
  • Solution of Einstein field equations

    Lambdavacuum solution and the second term is characteristic of a pressureless perfect fluid or dust solution. The cosmological constant is carefully chosen to partially

    Gödel metric

    Gödel_metric

  • Test particle
  • distribution of momentum and stress (e.g. pressure, viscous stresses in a perfect fluid). In the case of test particles in a vacuum solution or electrovacuum

    Test particle

    Test_particle

  • Phantom dark energy
  • Hypothetical form of dark energy

    Robert R. Caldwell in 1999. In cosmology, the equation of state of a perfect fluid is given by p = w ρ , {\displaystyle p=w\rho ,} where p is the pressure

    Phantom dark energy

    Phantom_dark_energy

  • Particle horizon
  • Distance measurement used in cosmology

    approximated as composed by non-interacting constituents, each one being a perfect fluid with density ρ i {\displaystyle \rho _{i}} , partial pressure p i {\displaystyle

    Particle horizon

    Particle_horizon

  • Buchdahl's theorem
  • Theorem in general relativity

    matter confined to an areal radius R {\displaystyle R} that behaves as a perfect fluid with a density that does not increase outwards. Assume, in addition

    Buchdahl's theorem

    Buchdahl's theorem

    Buchdahl's_theorem

  • Quark
  • Elementary particle, fundamental constituent of matter

    have yielded evidence for liquid-like quark matter exhibiting "nearly perfect" fluid motion. The quark–gluon plasma would be characterized by a great increase

    Quark

    Quark

    Quark

  • Gravastar
  • Hypothesized alternative to a black hole

    energy", and in this region p = −ρ . Surrounding it is a thin shell of perfect fluid where p = ρ . On the exterior is true vacuum, where p = ρ = 0 . The

    Gravastar

    Gravastar

    Gravastar

  • Perfection
  • State of completeness, flawlessness, or supreme excellence

    completely, radiation falling upon it. A perfect fluid would be one that is incompressible and non-viscous. A perfect gas would be one whose molecules did

    Perfection

    Perfection

    Perfection

  • Naked singularity
  • Hypothetical phenomenon

    (1998-10-09). "Final fate of the spherically symmetric collapse of a perfect fluid". Physical Review D. 58 (10) 104015. arXiv:gr-qc/9807038. Bibcode:1998PhRvD

    Naked singularity

    Naked_singularity

  • Toroidal planet
  • Planet in the shape of a toroidal or doughnut shape

    authors list (link) Nambo, E. C., Sarbach, O. (2020). "Static spherical perfect fluid stars with finite radius in general relativity: a review". Revista Mexicana

    Toroidal planet

    Toroidal planet

    Toroidal_planet

  • Kerr metric
  • Exact solution for the Einstein field equations

    fluid interior, and indeed to more general static spherically symmetric perfect fluid solutions. However, the problem of finding a rotating perfect-fluid

    Kerr metric

    Kerr metric

    Kerr_metric

  • Rest frame
  • Frame of reference in which a specified particle is at rest

    list (link) See p. 139-140 for discussion of the stress-energy tensor for a perfect fluid such as an ideal gas. Co-moving frame Mass-energy equivalence

    Rest frame

    Rest_frame

  • Robert Finn (mathematician)
  • American mathematician (1922–2022)

    PMC 1063753. PMID 16589247. Finn, R. (October 1954). "On the Flow of a Perfect Fluid through a Polygonal Nozzle. I". Proc Natl Acad Sci U S A. 40 (10): 983–985

    Robert Finn (mathematician)

    Robert_Finn_(mathematician)

  • Expansion of the universe
  • Increase in distance between parts of the universe

    a^{-1}} as its peculiar momentum decays. In general, we can consider a perfect fluid with pressure p = w ρ {\displaystyle p=w\rho } , where ρ {\displaystyle

    Expansion of the universe

    Expansion of the universe

    Expansion_of_the_universe

  • Fluid replacement
  • Medical practice of replenishing bodily fluid

    Fluid replacement or fluid resuscitation is the medical practice of replenishing bodily fluid lost through sweating, bleeding, fluid shifts or other pathologic

    Fluid replacement

    Fluid replacement

    Fluid_replacement

  • Hawking radiation
  • Hypothetical astrophysical effect

    light in a gravitational black hole and the flow of an approximately perfect fluid is analogous to gravity. (See analog models of gravity.) Observations

    Hawking radiation

    Hawking_radiation

  • List of scientific debates
  • on whether the luminiferous aether was unstable when considered a perfect fluid. Debate between Lord Kelvin and George Stokes. 1895 Lübeck Debate between

    List of scientific debates

    List_of_scientific_debates

  • Shape of the universe
  • Local and global geometry of the universe

    universe based on the mathematics of fluid dynamics, that is, modeling the matter within the universe as a perfect fluid. Although stars and structures of

    Shape of the universe

    Shape of the universe

    Shape_of_the_universe

  • Lambda-CDM model
  • Mathematical model of the Big Bang

    each line can be synchronized; the behavior resembles an expanding perfect fluid, General relativity that relates the geometry of spacetime to the distribution

    Lambda-CDM model

    Lambda-CDM model

    Lambda-CDM_model

  • Parker theorem
  • conducting fluid. When different magnetic field regions come into contact, they cannot smoothly merge due to the perfect conductivity of the fluid. Instead

    Parker theorem

    Parker_theorem

  • Axial fan design
  • Fan that induces gas flow mostly parallel to the shaft

    doi:10.1680/isenp.1935.13442. Marble, Frank E. (1948). "The Flow of a Perfect Fluid Through an Axial Turbomachine with Prescribed Blade Loading". Journal

    Axial fan design

    Axial_fan_design

  • Automatic transmission fluid
  • Hydraulic fluid used in vehicles with automatic transmissions

    Automatic transmission fluid (ATF) is a hydraulic fluid that is essential for the proper functioning of vehicles equipped with automatic transmissions

    Automatic transmission fluid

    Automatic transmission fluid

    Automatic_transmission_fluid

  • Are You the One?
  • American reality television series

    You the One?, all cast members were sexually fluid, with no gender limitations on their potential perfect matches. This season received a GLAAD Media Award

    Are You the One?

    Are You the One?

    Are_You_the_One?

  • Richard C. Tolman
  • American physicist (1881–1948)

    Einstein field equations describing the static spherically symmetric perfect fluid. It was Tolman who spurred J. Robert Oppenheimer's interest in relativistic

    Richard C. Tolman

    Richard C. Tolman

    Richard_C._Tolman

  • Vacuum energy
  • Background energy existing in space

    gravity and its interactions. In 1934, Georges Lemaître used an unusual perfect-fluid equation of state to interpret the cosmological constant as due to vacuum

    Vacuum energy

    Vacuum_energy

  • Bernoulli's principle
  • Principle relating to fluid dynamics

    Bernoulli's principle is a concept in fluid dynamics that relates pressure, speed and height. For example, for a fluid flowing horizontally, Bernoulli's principle

    Bernoulli's principle

    Bernoulli's principle

    Bernoulli's_principle

  • Interior Schwarzschild metric
  • Static exact solution in general relativity

    Schwarzschild metric (also interior Schwarzschild solution or Schwarzschild fluid solution) is an exact solution for the gravitational field in the interior

    Interior Schwarzschild metric

    Interior_Schwarzschild_metric

  • Negative mass
  • Concept in physical models

    required deformation through the introduction of the energy–momentum of a perfect fluid. Although no particles are known to have negative mass, physicists (primarily

    Negative mass

    Negative_mass

  • Ehlers–Geren–Sachs theorem
  • Physics theory

    J. Hancock and Claes Uggla show a counterexample in the non-tilted perfect fluid case. Thus an almost isotropic cosmic microwave temperature does not

    Ehlers–Geren–Sachs theorem

    Ehlers–Geren–Sachs theorem

    Ehlers–Geren–Sachs_theorem

  • Stress–energy tensor
  • Tensor describing energy momentum density in spacetime

    {E}{c^{2}}},\,\mathbf {p} ,\,\mathbf {p} \,\mathbf {v} \right)\,.} For a perfect fluid, the stress–energy tensor takes on the form T α β = ( ρ + p c 2 ) u

    Stress–energy tensor

    Stress–energy tensor

    Stress–energy_tensor

  • PHENIX detector
  • form of matter has indeed been discovered, and that it behaves like a perfect fluid. PHENIX scientists are now working to study its properties. Study matter

    PHENIX detector

    PHENIX detector

    PHENIX_detector

  • Francesco Sbrana
  • Italian mathematician (1891–1958)

    rational mechanics and mathematical physics, including the theory of perfect fluids, elastic deformations, and the metodo simbolico introduced by Giovanni

    Francesco Sbrana

    Francesco_Sbrana

  • David Gregory Ebin
  • American mathematician (born 1942)

    diffeomorphisms and the solution of the classical Euler equations for a perfect fluid, Bulletin of the American Mathematical Society, vol. 75, 1969, pp. 962–967

    David Gregory Ebin

    David_Gregory_Ebin

  • Alcubierre drive
  • Hypothetical FTL transportation by warping space

    a series of papers analysing which matter models—dust, perfect fluids, charged dust and fluids with a cosmological constant—are compatible with the warp-drive

    Alcubierre drive

    Alcubierre drive

    Alcubierre_drive

  • Julia Velkovska
  • Bulgarian-American high energy particle physicist

    Velkovska showed that these collisions result in small droplets of almost perfect fluid, i.e. a cohesive liquid that flows at zero viscosity, that emerge in

    Julia Velkovska

    Julia_Velkovska

  • Weyl curvature hypothesis
  • Hypothesis in physics

    P. Tod (1999). "Isotropic Cosmological Singularities I. Polytropic Perfect Fluid Spacetimes". Annals of Physics. 276 (2): 257–293. arXiv:gr-qc/9903008

    Weyl curvature hypothesis

    Weyl_curvature_hypothesis

  • Matter collineation
  • Vector field

    energy-momentum tensor represents a perfect fluid, every Killing vector field preserves the energy density, pressure and the fluid flow vector field. When the

    Matter collineation

    Matter_collineation

  • Closed wing
  • Aircraft wing configuration with a non-planar, continuous surface wing

    (1935). Durand, William F. (ed.). Division E: General Aerodynamic Theory-Perfect Fluids. Aerodynamic Theory: a General Review of Progress Under a Grant of the

    Closed wing

    Closed_wing

  • Perfect conductor
  • Idealized model for real conducting materials

    In electrostatics, a perfect conductor is an idealized model for real conducting materials. The defining property of a perfect conductor is that static

    Perfect conductor

    Perfect_conductor

  • Are You the One? season 8
  • American reality television program

    sexually fluid, with no gender limitations on their potential perfect matches. Notes  Name  Unconfirmed perfect match  Name  Confirmed perfect match In

    Are You the One? season 8

    Are_You_the_One?_season_8

  • Gérard Iooss
  • French mathematician

    Iooss, P.Plotnikov, J.F.Toland .  Standing waves on an infinitely deep perfect fluid under gravity. Arch. Rat. Mech. Anal. 177, 3, 367-478. doi:10.1007/s00205-005-0381-6

    Gérard Iooss

    Gérard_Iooss

  • Wolfgang R. Wasow
  • American mathematician

    on a solid surface as a fluid flows over it. Above the boundary layer, the fluid behaves approximately like a perfect fluid. But within the boundary

    Wolfgang R. Wasow

    Wolfgang_R._Wasow

  • Tribology
  • Science of rubbing surfaces

    materials. What we try to achieve by means of these materials is a perfect fluid lubrication, or a lubrication such that it is possible to avoid direct

    Tribology

    Tribology

  • Spacetime symmetries
  • Type of symmetry in physics

    energy–momentum tensor represents a perfect fluid, every Killing vector field preserves the energy density, pressure and the fluid flow vector field. When the

    Spacetime symmetries

    Spacetime_symmetries

  • Lavrentyev Institute of Hydrodynamics
  • Research institute based in Akademgorodok of Novosibirsk, Russia

    substantiation of approximate models of the theory of wave motions of a perfect fluid; the development of methods for group analysis of differential equations

    Lavrentyev Institute of Hydrodynamics

    Lavrentyev Institute of Hydrodynamics

    Lavrentyev_Institute_of_Hydrodynamics

  • Toroidal ring model
  • Model of subatomic particles

    mechanics today. In 1867 Lord Kelvin suggested that the vortex rings of a perfect fluid discovered by Hermann von Helmholtz represented "the only true atoms"

    Toroidal ring model

    Toroidal_ring_model

  • Vladimir Arnold
  • Russian mathematician (1937–2010)

    des fluides parfaits" ('On the differential geometry of infinite-dimensional Lie groups and its applications to the hydrodynamics of perfect fluids'),

    Vladimir Arnold

    Vladimir Arnold

    Vladimir_Arnold

  • Euler's equations (rigid body dynamics)
  • Quasilinear first-order ordinary differential equation

    des fluides parfaits" [On the differential geometry of infinite-dimensional Lie groups and its applications to the hydrodynamics of perfect fluids]. Annales

    Euler's equations (rigid body dynamics)

    Euler's_equations_(rigid_body_dynamics)

  • Sean Smith (bassist)
  • American modern jazz double bass player and composer

    Judith Schlesinger of AllMusic, writing in early 2000s, the "pitch-perfect, fluid, and elegant bassist" is one of the most employed musicians in the international

    Sean Smith (bassist)

    Sean Smith (bassist)

    Sean_Smith_(bassist)

  • Biofluid dynamics
  • Scientific discipline

    Biofluid dynamics or biological fluid dynamics is a specialization of fluid dynamics focused on biological fluids in humans and other animals. Alternatively

    Biofluid dynamics

    Biofluid_dynamics

  • George David Birkhoff
  • American mathematician (1884–1944)

    seem to mind) that his theory allows as sources only matter which is a perfect fluid in which the speed of sound must equal the speed of light. Birkhoff

    George David Birkhoff

    George David Birkhoff

    George_David_Birkhoff

  • Equation of state
  • Equation describing a state of matter under a given set of conditions

    (quark–gluon plasmas) and radiation fields. A related concept is the perfect fluid equation of state used in cosmology. Equations of state are applied

    Equation of state

    Equation of state

    Equation_of_state

  • Gaussian polar coordinates
  • Coordinate system

    theory of static spherically symmetric perfect fluids. Static spacetime Static spherically symmetric perfect fluids Schwarzschild coordinates Isotropic coordinates

    Gaussian polar coordinates

    Gaussian_polar_coordinates

  • Timeline of atomic and subatomic physics
  • the RHIC accelerator of Brookhaven National Laboratory generates a "perfect" fluid, perhaps the quark–gluon plasma. 2010 The Large Hadron Collider at CERN

    Timeline of atomic and subatomic physics

    Timeline_of_atomic_and_subatomic_physics

  • 1646 in science
  • Pascal's law, a law of hydrostatics is developed, stating that, in a perfect fluid, the pressure exerted on it anywhere is transmitted equally. Dr Thomas

    1646 in science

    1646_in_science

  • List of cosmological computation software
  • geometry and topology. CosmoGRaPH (Cosmological General Relativity And (Perfect fluid | Particle) Hydrodynamics) is a C++ code used to explore cosmological

    List of cosmological computation software

    List of cosmological computation software

    List_of_cosmological_computation_software

  • Cartan–Karlhede algorithm
  • solutions, at most three differentiations are required to compare any two perfect fluid solutions. Vanishing scalar invariant spacetime Computer algebra system

    Cartan–Karlhede algorithm

    Cartan–Karlhede_algorithm

  • Timeline of cosmological theories
  • the cosmological constant as due to a vacuum energy with an unusual perfect fluid equation of state. 1938 – Hans Bethe calculates the details of the two

    Timeline of cosmological theories

    Timeline of cosmological theories

    Timeline_of_cosmological_theories

  • Recoil (rheology)
  • in the fluid's recent past. However, the fluid cannot fully return to its original position due to energy losses stemming from less than perfect elasticity

    Recoil (rheology)

    Recoil_(rheology)

  • Parameterized post-Newtonian formalism
  • Approximation method for general relativity in physics

    is the coordinate velocity of the matter. Stress-energy tensor for a perfect fluid takes form T 00 = ρ ( 1 + Π + v 2 + 2 U ) {\displaystyle T^{00}=\rho

    Parameterized post-Newtonian formalism

    Parameterized_post-Newtonian_formalism

  • William Allen Zajc
  • American nuclear physicist

    discovered that this matter is in fact strongly interacting and nearly a perfect fluid. Since stepping down after nine years of dedicated service as spokesperson

    William Allen Zajc

    William Allen Zajc

    William_Allen_Zajc

  • Nordström's theory of gravitation
  • Predecessor to the theory of relativity

    special case when the only matter present is a cloud of dust (that is, a perfect fluid in which the pressure is assumed to be negligible). He argued that the

    Nordström's theory of gravitation

    Nordström's_theory_of_gravitation

  • Newton's identities
  • Relations between power sums and elementary symmetric functions

    the characteristic polynomial of the Einstein tensor in the case of a perfect fluid, and similar articles on other types of exact solutions in general relativity

    Newton's identities

    Newton's_identities

  • Euler–Arnold equation
  • Class of partial differential equations

    des fluides parfaits" ('On the differential geometry of infinite-dimensional Lie groups and its applications to the hydrodynamics of perfect fluids'),

    Euler–Arnold equation

    Euler–Arnold_equation

  • Xin Zhui
  • Well-preserved ancient body found in China

    and 162 carved wooden figurines representing servants and musicians. The fluid present in the coffin allowed Xin Zhui's body to remain in such well-preserved

    Xin Zhui

    Xin Zhui

    Xin_Zhui

  • Pleural effusion
  • Accumulation of excess fluid in the pleural cavity

    accumulation of excessive fluid in the pleural space, the potential space that surrounds each lung. Under normal conditions, pleural fluid is secreted by the

    Pleural effusion

    Pleural effusion

    Pleural_effusion

  • Truppenführung
  • German Army field manual

    defense-in-depth and reverse-slope defense. On the offense in 1918, they perfected fluid non-linear infiltration tactics supported by artillery (cf. Stormtrooper)

    Truppenführung

    Truppenführung

  • Electromagnetic mass
  • Physical concept

    who showed that the inertia of a body moving in an incompressible perfect fluid is increased.) So due to this self-induction effect, electrostatic energy

    Electromagnetic mass

    Electromagnetic mass

    Electromagnetic_mass

  • Relativistic Euler equations
  • Generalization of Euler equations

    μ {\displaystyle \nabla _{\mu }} is the covariant derivative. For a perfect fluid, T μ ν = ( e + p ) u μ u ν + p g μ ν . {\displaystyle T^{\mu \nu }\

    Relativistic Euler equations

    Relativistic_Euler_equations

  • Clapotis
  • Non-breaking standing wave pattern

    P. I.; Toland, J. F. (2005). "Standing Waves on an Infinitely Deep Perfect Fluid Under Gravity" (PDF). Archive for Rational Mechanics and Analysis. 177

    Clapotis

    Clapotis

    Clapotis

  • Carminati–McLenaghan invariants
  • tensor. In the case of vacuum solutions, electrovacuum solutions and perfect fluid solutions, the CM scalars comprise a complete set. Additional invariants

    Carminati–McLenaghan invariants

    Carminati–McLenaghan_invariants

  • Compressible flow
  • Branch of fluid mechanics

    flow (or gas dynamics) is the branch of fluid mechanics that deals with flows having significant changes in fluid density. While all flows are compressible

    Compressible flow

    Compressible_flow

  • Pressuron
  • Hypothetical gravitational particle

    T=g^{\mu \nu }T_{\mu \nu }} is its trace. If one considers a pressure-free perfect fluid (also known as a dust solution), the effective material Lagrangian becomes

    Pressuron

    Pressuron

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