scholarly journals Signals of axion like dark matter in time dependent polarization of light

2020 ◽  
Vol 803 ◽  
pp. 135288 ◽  
Author(s):  
So Chigusa ◽  
Takeo Moroi ◽  
Kazunori Nakayama
Keyword(s):  
Dark Matter ◽  
Time Dependent ◽  
Dependent Polarization ◽  
Polarization Of Light

Time-dependent polarization in Mössbauer experiments with synchrotron radiation (II)

1994 ◽  
Vol 92 (1) ◽  
pp. 1113-1121 ◽  
Author(s):  
U. Bergmann ◽  
D. P. Siddons ◽  
J. B. Hastings
Keyword(s):  
Synchrotron Radiation ◽  
Time Dependent ◽  
Dependent Polarization

Time-dependent polarization transfer from molecular rotation to nuclear spin

2006 ◽  
Vol 74 (4) ◽  
Author(s):  
Luis Rubio-Lago ◽  
Dimitris Sofikitis ◽  
Antonis Koubenakis ◽  
T. Peter Rakitzis
Keyword(s):  
Nuclear Spin ◽  
Polarization Transfer ◽  
Molecular Rotation ◽  
Time Dependent ◽  
Dependent Polarization

scholarly journals Shaping Femtosecond Pulses with Targeted Time-Dependent Polarization

2005 ◽  
Vol 33 (5) ◽  
pp. 322-328
Author(s):  
Takayuki SUZUKI ◽  
Shinichirou MINEMOTO ◽  
Hirofumi SAKAI
Keyword(s):  
Time Dependent ◽  
Femtosecond Pulses ◽  
Dependent Polarization

scholarly journals Effective optical smoothing scheme to suppress laser plasma instabilities by time-dependent polarization rotation via pulse chirping

2021 ◽  
Vol 29 (2) ◽  
pp. 1304
Author(s):  
Zheqiang Zhong ◽  
Bin Li ◽  
Hao Xiong ◽  
Jiwei Li ◽  
Jie Qiu ◽  
...  
Keyword(s):  
Laser Plasma ◽  
Time Dependent ◽  
Plasma Instabilities ◽  
Polarization Rotation ◽  
Dependent Polarization

scholarly journals Geodesic motion of S2 and G2 as a test of the fermionic dark matter nature of our Galactic core

2020 ◽  
Vol 641 ◽  
pp. A34 ◽  
Author(s):  
E. A. Becerra-Vergara ◽  
C. R. Argüelles ◽  
A. Krut ◽  
J. A. Rueda ◽  
R. Ruffini
Keyword(s):  
Dark Matter ◽  
Radial Velocity ◽  
Drag Force ◽  
Gravitational Potential ◽  
Galactic Center ◽  
Critical Mass ◽  
Time Dependent ◽  
Fermion Mass ◽  
Massive Black Hole ◽  
Sgr A

The motion of S-stars around the Galactic center implies that the central gravitational potential is dominated by a compact source, Sagittarius A* (Sgr A*), which has a mass of about 4 × 106 M⊙ and is traditionally assumed to be a massive black hole (BH). The explanation of the multiyear accurate astrometric data of the S2 star around Sgr A*, including the relativistic redshift that has recently been verified, is particularly important for this hypothesis and for any alternative model. Another relevant object is G2, whose most recent observational data challenge the scenario of a massive BH: its post-pericenter radial velocity is lower than expected from a Keplerian orbit around the putative massive BH. This scenario has traditionally been reconciled by introducing a drag force on G2 by an accretion flow. As an alternative to the central BH scenario, we here demonstrate that the observed motion of both S2 and G2 is explained in terms of the dense core – diluted halo fermionic dark matter (DM) profile, obtained from the fully relativistic Ruffini-Argüelles-Rueda (RAR) model. It has previously been shown that for fermion masses 48−345 keV, the RAR-DM profile accurately fits the rotation curves of the Milky Way halo. We here show that the solely gravitational potential of such a DM profile for a fermion mass of 56 keV explains (1) all the available time-dependent data of the position (orbit) and line-of-sight radial velocity (redshift function z) of S2, (2) the combination of the special and general relativistic redshift measured for S2, (3) the currently available data on the orbit and z of G2, and (4) its post-pericenter passage deceleration without introducing a drag force. For both objects, we find that the RAR model fits the data better than the BH scenario: the mean of reduced chi-squares of the time-dependent orbit and z data are ⟨χ̄2⟩S2,RAR ≈ 3.1 and ⟨χ̄2⟩S2,BH ≈ 3.3 for S2 and ⟨χ̄2⟩G2,RAR ≈ 20 and ⟨χ̄2⟩G2,BH ≈ 41 for G2. The fit of the corresponding z data shows that while for S2 we find comparable fits, that is, χ̄2z,RAR ≈ 1.28 and χ̄2z,BH ≈ 1.04, for G2 the RAR model alone can produce an excellent fit of the data, that is, χ̄2z,RAR ≈ 1.0 and χ̄2z,BH ≈ 26. In addition, the critical mass for gravitational collapse of a degenerate 56 keV-fermion DM core into a BH is ∼ 108 M⊙. This result may provide the initial seed for the formation of the observed central supermassive BH in active galaxies, such as M 87.

scholarly journals Generation of Time-Dependent Polarization Pulses by Combinations of High-Intensity Femtosecond Laser Pulses.

2000 ◽  
Vol 28 (8) ◽  
pp. 506-510 ◽  
Author(s):  
Masayuki KAKEHATA ◽  
Roka UEDA ◽  
Hideyuki TAKADA ◽  
Kenji TORIZUKA ◽  
Minoru OBARA
Keyword(s):  
Femtosecond Laser ◽  
High Intensity ◽  
Laser Pulses ◽  
Femtosecond Laser Pulses ◽  
Time Dependent ◽  
Dependent Polarization
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