|  Acceleration | 
In General > s.a. Fermi Acceleration;
  physics teaching; reference
  frame; rindler space [uniform acceleration].
  * Idea: The concept of
    acceleration as rate of change of velocity in time (as opposed to rate
    of change in space, for example), seems to be due to Galileo.
  * Accelerometers: 2014,
    Current accelerometers for submarines (used to pinpoint their position
    under water without having to surface to use the GPS) are accurate to
    within 1 km after traveling one day; An accelerometer being developed
    in the UK, based on the quantum interference of ultracold atoms, will
    be accurate to within 1 m; Further improvements are being planned.
  @ Maximal acceleration:
    Caianello LNC(81);
    Brandt FPL(89)
      [and 4-velocity fiber bundle over spacetime];
    Pati EPL(92) [for a quantum particle];
    Papini NCB(02);
    Feoli IJMPD(03) [different values];
    Papini qp/04 [and superconductors];
    Gallego Torromé gq/05 [Finsler models];
    Friedman a0912 [test];
    Rovelli & Vidotto PRL(13)-a1307 [from spin-foam quantum gravity];
    Brandt a1311 [and the quantum-to-classical transition];
    Gallego Torromé CQG(15)-a1404 [geometry and kinematics];
    > s.a. kerr spacetime; modified lorentz symmetry.
  @ Accelerated fields: Céleri & Kiosses a1712 [and the Unruh effect].
  > Theories with critical accelerations:
    see modifications of general relativity; MOND.
  > Online resources:
    see Wikipedia page.
Relativistic / Covariant
  * Idea:
    Acceleration is a well-defined concept; It can be measured with a box and
    a mass with springs, and does not need a specification of "with respect to
    what", contrary to the situation with velocity.
  $ Covariant definition: The 4-vector
    \(A^a:= u^b \nabla_b u^a\), perpendicular to the world-line, \(A^a u_a = 0\).
  * In general relativity: A
    world-line accelerates only if subject to non-gravitational forces; Objects
    in free fall follow geodesics \(A^a = 0\).
  @ Relativistic: Rindler & Mishra PLA(93) [relative acceleration in special relativity];
    Bini et al CQG(95)
      [transformation law in general relativity];
    Lyutikov a0903 [reversal of centrifugal acceleration];
    Llosa a1507
      [coordinate transformation laws and infinitesimal generators];
    Abramowicz a1608
      [covariant definitions and confusions].
  @ Constant / uniform acceleration: 
    Friedman & Scarr GRG(15)-a1602 [in an arbitrary curved spacetime];
    Pons & Ferran de Palol GRG(19)-a1811 [also constant proper jerk and  beyond].
  > Acceleration of the cosmological expansion:
    see cosmic acceleration; quantum
    field theory effects in curved spacetime.
Effects / Phenomenology
  @ Measurement, accelerometers: Dragan et al PRD(11)-a1007 [Unruh-DeWitt detector as quantum accelerometer];
    Dickerson et al PRL(13)
    + Bouter Phy(13) [use of atom interferometers];
    news pw(14)may [accelerometer under development].
  @ Effects on atoms:
    Marino et al PS(14)-a1404 [and interactions];
    Dahia & Felix de Araujo CQG(15)-a1412 [atomic clocks];
    Zhang FP(16)-a1612 [accelerated atom coupled  to electromagnetic vacuum fluctuations].
  @ Astrophysical effects: Chicone et al PLA(11) [particle acceleration by varying gravitational fields and cosmic jets];
    Chae et al ApJL(20)-a2010 [universal acceleration scale in elliptical galaxies].
  > Gravity-related phenomena:
    see astrophysics; matter near black holes
    [particle acceleration]; unruh effect [accelerated detectors].
  > Other particle-related phenomena: see
    acceleration radiation [accelerated charges]; anomalous
    acceleration [Pioneer effect]; quantum state evolution.
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  send feedback and suggestions to bombelli at olemiss.edu – modified 26 dec 2020