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researcher

D. Boyanovsky

173 papers hereh-index 415k citations246 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • sole author21
  • first author84
  • middle author18
  • last author22

Across the 145 of 173 papers where every author was matched, so the position is known.

fields
  • hep-ph110
  • astro-ph32
  • astro-ph.CO15
  • hep-th6
  • gr-qc4
  • quant-ph3
same name
  • D. Boyanovsky — 3 papers, h 6
  • D. Boyanovsky — 1 paper

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
19922025
most citedDissipation via Particle Production in Scalar Field Theories

374 citations · 6.3k across the 173 of their papers we have counts for

collaborators
Showing 2012Show all

4 papers · 1 filter

hep-ph2012★ 4 cited

Charged lepton mixing via heavy sterile neutrinos

Louis Lello, Daniel Boyanovsky

Pseudoscalar meson decay leads to an entangled state of charged leptons (μ,e) and massive neutrinos. Tracing out the neutrino degrees of freedom leads to a reduced density matrix…

hep-ph2012★ 25 cited

Searching for sterile neutrinos from π and K decays

Louis Lello, Daniel Boyanovsky

The production of heavy sterile neutrinos from π−,K− decay at rest yields charged leptons with negative helicity (positive for π+,K+). We obtain the branching ratio for thi…

astro-ph.CO2012★ 37 cited

Spontaneous symmetry breaking in inflationary cosmology: on the fate of Goldstone Bosons

Daniel Boyanovsky

We argue that in an inflationary cosmology a consequence of the lack of time translational invariance is that spontaneous breaking of a continuous symmetry and Goldstone's theorem…

hep-ph2012★ 52 cited

Condensates and quasiparticles in inflationary cosmology: mass generation and decay widths

Daniel Boyanovsky

During de Sitter inflation massless particles of minimally coupled scalar fields acquire a mass and a decay width thereby becoming \emph{quasiparticles}. For bare massless particle…

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