Stellar energy loss from the reactionγγ→e+e−νν¯

1976 ◽  
Vol 14 (2) ◽  
pp. 335-339 ◽  
Author(s):  
A. Soni ◽  
J. A. M. Vermaseren
Keyword(s):  
Energy Loss ◽  
Stellar Energy

Hidden Higgs boson models and stellar energy loss

1989 ◽  
Vol 217 (3) ◽  
pp. 238-242 ◽  
Author(s):  
Darwin Chang ◽  
Wai-Yee Keung
Keyword(s):  
Higgs Boson ◽  
Energy Loss ◽  
Stellar Energy

Light Pseudoscalar Particle and Stellar Energy Loss

1982 ◽  
Vol 48 (22) ◽  
pp. 1522-1525 ◽  
Author(s):  
M. Fukugita ◽  
S. Watamura ◽  
M. Yoshimura
Keyword(s):  
Energy Loss ◽  
Pseudoscalar Particle ◽  
Stellar Energy

Stellar energy loss throughe+e−→νν¯inE6

1989 ◽  
Vol 40 (8) ◽  
pp. 2712-2715 ◽  
Author(s):  
S. Alam ◽  
J. D. Anand ◽  
S. N. Biswas ◽  
Ashok Goyal
Keyword(s):  
Energy Loss ◽  
Stellar Energy

scholarly journals Neutrino energy-loss rate in 331β model

2021 ◽  
Vol 36 (26) ◽  
Author(s):  
D. T. Binh ◽  
L. T. Hue ◽  
V. H. Binh ◽  
H. N. Long
Keyword(s):  
Dipole Moment ◽  
Energy Loss ◽  
Loss Rate ◽  
Mass Range ◽  
Neutrino Energy ◽  
Correction Formula ◽  
Energy Loss Rate ◽  
Stellar Energy ◽  
Neutrino Pair ◽  
Text Correction

We evaluate the stellar energy-loss rates [Formula: see text] due to the production of neutrino pair in 3-3-1 models. The energy loss rate [Formula: see text] is evaluated for different values of [Formula: see text] in which [Formula: see text] is a parameter used to define the charge operator in the 331 models. We show that the contribution of dipole moment to the energy loss rate is small compared to the contribution of new natural gauge boson [Formula: see text]. The correction [Formula: see text] compared with that of Standard Model is evaluated and do not exceed 14% and is highest with [Formula: see text]. Of all the evaluated models, model with [Formula: see text] give a relative large [Formula: see text] correction for the mass of [Formula: see text][Formula: see text] GeV. This mass range is within the searching range for [Formula: see text] boson at LHC.

scholarly journals Constraints on hidden gravitons from fifth-force experiments and stellar energy loss

2017 ◽  
Vol 2017 (9) ◽  
Author(s):  
J. A. R. Cembranos ◽  
A. L. Maroto ◽  
H. Villarrubia-Rojo
Keyword(s):  
Energy Loss ◽  
Fifth Force ◽  
Stellar Energy

ENERGY LOSS FROM THE SUN AND RED GIANTS: BOUNDS ON SHORT-RANGE BARYONIC AND LEPTONIC FORCES

1989 ◽  
Vol 04 (04) ◽  
pp. 311-323 ◽  
Author(s):  
J. A. GRIFOLS ◽  
E. MASSÓ ◽  
S. PERIS
Keyword(s):  
Energy Loss ◽  
Short Range ◽  
Red Giants ◽  
The Sun ◽  
Evolutionary Models ◽  
Astronomical Data ◽  
Astronomical Observations ◽  
Stellar Energy

Laboratory, geophysical and astronomical data can place severe limits on forces weaker than gravity whose ranges typically go from ~ 1 cm up to astronomical distances. Forces strictly microscopic, however, lie beyond reach of Cavendish-type and geophysical experiments as well as astronomical observations. By computing the stellar energy loss caused by new hypothetical forces coupled to baryon and/or lepton charges and by demanding that this energy drain does not upset current stellar evolutionary models, we put restrictions on forces with a range larger than or ~ 1 Å.

Sign in / Sign up

Export Citation Format

Share Document