initial fluctuations
(primordial fluctuations)
(early universe density variations leading to current universe)
The initial fluctuations (aka primordial fluctuations) are
density variations in the energy/matter of the early universe
that lead to the large scale structure of the universe today. According to
modern Big Bang theories such as Lambda-CDM model, these were random
quantum fluctuations that inflation expanded
into the substantial density variations in the subsequent universe.
Cosmology is interested in characteristics of the
initial fluctuations, such as whether they appear to vary
in the manner that theory predicts (initial fluctuation spectrum).
The CMB is an observable phenomena offering clues to it
(CMB anisotropies).
(cosmology,quantum mechanics,early universe)
Further reading:
https://en.wikipedia.org/wiki/Primordial_fluctuations
https://physics.aps.org/articles/v13/16
https://hipacc.ucsc.edu/IPC2013/slides/130626_PriyamvadaNatarajan_RemarksCosmology.pdf
https://www.slac.stanford.edu/econf/C070730/talks/Wechsler_080207.pdf
https://ned.ipac.caltech.edu/level5/March01/Coles/Coles2.html
Referenced by pages:
baryon acoustic oscillations (BAO)
CMB anisotropies
CMB polarization
initial fluctuation spectrum
Press-Schechter formalism
primordial black hole (PBH)
quantum fluctuations
Index