scholarly journals What we can learn from the spectral index of the tensor mode

2016 ◽  
Vol 755 ◽  
pp. 70-75 ◽  
Author(s):  
Kazunori Kohri ◽  
Chia-Min Lin ◽  
Tomohiro Matsuda
Keyword(s):  
Spectral Index ◽  
Tensor Mode

scholarly journals INFLATION WITH HIGH DERIVATIVE COUPLINGS

2007 ◽  
Vol 22 (25n28) ◽  
pp. 1987-1994 ◽  
Author(s):  
BIN CHEN ◽  
MIAO LI ◽  
TOWER WANG ◽  
YI WANG
Keyword(s):  
Power Spectrum ◽  
Spectral Index ◽  
High Derivative ◽  
Ricci Scalar ◽  
Tensor Mode ◽  
Consistency Relation ◽  
Mode Spectrum

We study a class of generalized inflation models in which the inflaton is coupled to the Ricci scalar by a general f(φ, R) term. The scalar power spectrum, the spectral index, the running of the spectral index, the tensor mode spectrum and a new consistency relation of the model are calculated.

Analysis of the spectral index method for vector modes of rib waveguides

1990 ◽  
Vol 137 (1) ◽  
pp. 21 ◽  
Author(s):  
M.S. Stern ◽  
P.C. Kendall ◽  
P.W.A. McLlroy
Keyword(s):  
Spectral Index ◽  
Index Method ◽  
Rib Waveguides

Spectral index method for rib waveguide analysis

1989 ◽  
Vol 25 (2) ◽  
pp. 107 ◽  
Author(s):  
P.C. Kendall ◽  
P.W.A. Mcllroy ◽  
M.S. Stern
Keyword(s):  
Spectral Index ◽  
Index Method ◽  
Rib Waveguide

scholarly journals Spectral index-flux relation for investigating the origins of steep decay in γ-ray bursts

2021 ◽  
Vol 12 (1) ◽  
Author(s):  
Samuele Ronchini ◽  
Gor Oganesyan ◽  
Marica Branchesi ◽  
Stefano Ascenzi ◽  
Maria Grazia Bernardini ◽  
...  
Keyword(s):  
Spectral Index ◽  
Proton Synchrotron ◽  
Relativistic Jets ◽  
Time Resolved ◽  
X Ray ◽  
Compact Binary ◽  
Internal Dissipation ◽  
Adiabatic Cooling ◽  
Alternative Scenarios ◽  
Steep Decay

Abstractγ-ray bursts (GRBs) are short-lived transients releasing a large amount of energy (1051 − 1053 erg) in the keV-MeV energy range. GRBs are thought to originate from internal dissipation of the energy carried by ultra-relativistic jets launched by the remnant of a massive star’s death or a compact binary coalescence. While thousands of GRBs have been observed over the last thirty years, we still have an incomplete understanding of where and how the radiation is generated in the jet. Here we show a relation between the spectral index and the flux found by investigating the X-ray tails of bright GRB pulses via time-resolved spectral analysis. This relation is incompatible with the long standing scenario which invokes the delayed arrival of photons from high-latitude parts of the jet. While the alternative scenarios cannot be firmly excluded, the adiabatic cooling of the emitting particles is the most plausible explanation for the discovered relation, suggesting a proton-synchrotron origin of the GRB emission.

A novel spectral index for estimation of relative chlorophyll content of sugar beet

2021 ◽  
Vol 184 ◽  
pp. 106088
Author(s):  
Jing Zhang ◽  
Haiqing Tian ◽  
Di Wang ◽  
Haijun Li ◽  
Abdul Mounem Mouazen
Keyword(s):  
Sugar Beet ◽  
Chlorophyll Content ◽  
Spectral Index ◽  
Relative Chlorophyll Content

Bipolar outflow of gas in the spiral galaxy NGC 3079

1986 ◽  
Vol 64 (4) ◽  
pp. 531-535 ◽  
Author(s):  
Nebojsa Duric ◽  
E. R. Seaquist
Keyword(s):  
Spectral Index ◽  
Spiral Galaxy ◽  
Central Region ◽  
Qualitative Description ◽  
Radio Continuum ◽  
Large Array ◽  
Very Large Array ◽  
Bipolar Outflow ◽  
The Galaxy

Very large array, radio-continuum observations of the edge-on spiral galaxy NGC 3079 are presented. The observations reveal that the nucleus has windlike properties and that the central region of the galaxy exhibits an unusual figure-eight morphology that shows evidence of severe depolarization and a flattening spectral index away from the nucleus. A qualitative description of a model is presented to account for the observed radio properties. It is shown that a wind-driven shock propagating away from the nucleus and focused by the ambient disk gas can give rise to the observed morphology.

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