Nonlinear spectral blueshift in semiconductor optical amplifiers [PDF]
We demonstrate that spectral peak power of negatively chirped optical pulses can acquire a blueshift after amplification by a semiconductor optical amplifier. The central wavelength of a transform limited optical pulse translates over 20 nm towards a shorter wavelength after propagation in a single-mode fiber and semiconductor optical amplifier.
Anastasia Bednyakova +3 more
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CFTs blueshift tensor fluctuations universally [PDF]
Abstract The strong constraints of conformal symmetry cause any nearly-conformal sector to blueshift tensor fluctuations in cosmology. Hidden sectors with approximate conformal symmetry, which may be quite large, are a well-motivated extension of physics beyond the Standard Models of particle physics and cosmology.
Matthew Baumgart +2 more
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Anomalous blueshift of aperture resonance enabled by the loss of a thin film [PDF]
The substrate effects on aperture resonance have been widely studied because the resonance peak position is key for sensing, communications, and field enhancement applications. So far, the theoretical works have focused on the lossless infinite substrate
Jisoo Kyoung
doaj +2 more sources
Origin of the injection-dependent emission blueshift and linewidth broadening of III-nitride light-emitting diodes [PDF]
III-nitride light-emitting diodes (LEDs) exhibit an injection-dependent emission blueshift and linewidth broadening that is severely detrimental to their color purity.
Nick Pant +5 more
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Redshifts and blueshifts of OH vibrations [PDF]
AbstractAb initio calculations of potential energy, dipole moment, equilibrium OH distance, force constants, and anharmonic frequencies, and correlation between these quantities, are presented for a water molecule and an OH− ion in a uniform electric field of varying field strength.
Kersti Hermansson
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Existence of blueshifts in quasispherical Szekeres spacetimes [PDF]
In Lema\^ tre -- Tolman (L--T) models, light rays emitted \textit{radially} at the Big Bang (BB) at such radial coordinates $r$ where the bang-time function $t_B(r)$ has $\dril {t_B} r \neq 0$ reach every observer with \textit{infinite blueshift}, $z = -1$. Consequently, there exist rays, emitted soon after the BB, that will reach later observers with
Andrzej Krasiński
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Gravitational redshift/blueshift of light emitted by geodesic test particles, frame-dragging and pericentre-shift effects, in the Kerr–Newman–de Sitter and Kerr–Newman black hole geometries [PDF]
We investigate the redshift and blueshift of light emitted by timelike geodesic particles in orbits around a Kerr–Newman–(anti) de Sitter (KN(a)dS) black hole.
G. V. Kraniotis
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Heat flux induced blueshift of dominant phonon wavelength and its impact on thermal conductivity [PDF]
The concept of dominant phonon wavelength is investigated in systems submitted to a heat flux at low temperatures. Using spectral energy distributions, a treatment of two-dimensional and three-dimensional structures is conducted in parallel.
Aymeric Ramiere +2 more
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Gravitational blueshift from a collapsing object
We discuss a counterintuitive phenomenon of classical general relativity, in which a significant fraction of the radiation emitted by a collapsing object and detected by a distant observer may be blueshifted rather than redshifted.
Lingyao Kong +2 more
doaj +4 more sources
GRB 011211: An alternative interpretation of the optical and X-ray spectra in terms of blueshifts [PDF]
The redshifts of the gamma ray burst (GRB) GRB 011211 has been determined as 2.14 from several absorption lines seen in the spectrum of its optical afterglow.
D. Basu
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