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The 4.9 GHz Micro-Arcsecond Scintillation-Induced Variability (MASIV) Survey detected a drop in Interstellar Scintillation (ISS) for sources at redshifts z > 2, indicating an apparent increase in angular diameter or a decrease in flux…

宇宙学与河外天体物理 · 物理学 2011-09-09 J. Y Koay , J. -P. Macquart , B. J. Rickett , H. E. Bignall , J. E. J. Lovell , C. Reynolds , D. L. Jauncey , T. Pursimo , L. Kedziora-Chudczer , R. Ojha

We have investigated the spatial distribution of quasars and its relationship with redshift by using the two-point correlation function, the variance of cell counts and the conditional density as a function of redshift. By comparing our…

天体物理学 · 物理学 2007-05-23 P. Andreani , S. Cristiani , F. La Franca

The high-k ($7 \lesssim k_{\bot} \rho_i \lesssim 11$) wavenumber spectrum of density fluctuations has been measured for the first time in MAST [B. Lloyd et al, Nucl. Fusion 43, 1665 (2003)]. This was accomplished with the first…

等离子体物理 · 物理学 2015-02-11 J. C. Hillesheim , N. A. Crocker , W. A. Peebles , H. Meyer , A. Meakins , A. R. Field , D. Dunai , M. Carr , N. Hawkes , the MAST Team

The viscosity of dark matter in cosmological models may cause an accelerated expansion and when this effect is sufficiently large, it can explain the dark energy. In this work, attributing the origin of viscosity to self-interaction of dark…

宇宙学与河外天体物理 · 物理学 2019-02-27 Abhishek Atreya , Jitesh R. Bhatt , Arvind Kumar Mishra

A common belief about big-bang cosmology is that the cosmological redshift cannot be properly viewed as a Doppler shift (that is, as evidence for a recession velocity), but must be viewed in terms of the stretching of space. We argue that,…

科普物理 · 物理学 2010-11-02 Emory F. Bunn , David W. Hogg

Single-detector 3D dynamic light scattering (3D-DLS) emerges as a reliable technique to determine the drift velocity of out-of-equilibrium colloidal particles. In particular, our investigation reveals the appearance of oscillations of a…

软凝聚态物质 · 物理学 2024-10-08 José López-Molina , Arturo Moncho-Jordá , María Tirado-Miranda

A strongly self-interacting component of asymmetric dark matter (DM) particles can form compact dark stars (DSs). These objects have a broad spectrum of masses and radii, with distinct evolution histories from both neutron stars and black…

高能物理 - 唯象学 · 物理学 2026-03-25 Boris Betancourt Kamenetskaia , Qianhang Ding , Chris Kouvaris

The exploration of the redshift drift, a direct measurement of cosmological expansion, is expected to take several decades of observation with stable, sensitive instruments. We introduced a new method to probe cosmology which bypasses the…

宇宙学与河外天体物理 · 物理学 2023-08-16 Chengyi Wang , Krzysztof Bolejko , Geraint F. Lewis

We forecast the detectability of the Doppler magnification dipole with a joint analysis of galaxy spectroscopic redshifts and size measurements. The Doppler magnification arises from an apparent size variation caused by galaxies' peculiar…

宇宙学与河外天体物理 · 物理学 2026-04-01 Isabelle Ye , Philip Bull , Caroline Guandalin , Chris Clarkson , Ainulnabilah Nasirudin

A fundamental prediction of relativistic cosmologies is that, due to the expansion of space, observations of the distant cosmos should be time dilated and appear to run slower than events in the local universe. Whilst observations of…

宇宙学与河外天体物理 · 物理学 2023-06-08 Geraint F. Lewis , Brendon J. Brewer

Nonlinear waves emitted from a moving source are studied. A meandering spiral in a reaction-diffusion medium provides an example, where waves originate from a source exhibiting a back-and-forth movement in radial direction. The periodic…

统计力学 · 物理学 2007-05-23 Lutz Brusch , Alessandro Torcini , Markus Baer

Spatial maps of the high-pass frequency filtered time-averaged root-mean-squared (RMS) Doppler velocities tend to show substantial decrements within regions of strong field and curiously, randomly distributed patches of enhancement in the…

太阳与恒星天体物理 · 物理学 2015-05-13 Shravan M. Hanasoge

The oscillating pressure of the ultralight scalar dark matter (DM) can induce the oscillation of the local gravitational potential. Similar to the time-dependent frequency shift for the pulse signals of pulsars, the oscillation of the local…

宇宙学与河外天体物理 · 物理学 2023-11-29 Ke Wang , Yin Zhong

We have identified 469 MgII doublet systems having W_r >= 0.02 {\AA} in 252 Keck/HIRES and UVES/VLT quasar spectra over the redshift range 0.1 < z < 2.6. Using the largest sample yet of 188 weak MgII systems (0.02 {\AA} <= W_r < 0.3 {\AA}),…

宇宙学与河外天体物理 · 物理学 2015-06-15 Jessica L. Evans , Christopher W. Churchill , Michael T. Murphy , Nikole M. Nielsen , Elizabeth S. Klimek

We derive the scatter in the relationship between redshift and radio-to-submm spectral index, alpha^{350}_{1.4}, using the observed spectral energy distributions of 17 low redshift star forming galaxies. A mean galaxy model is derived,…

天体物理学 · 物理学 2009-10-31 C. L. Carilli , M. S. Yun

We find that the Fe III$\lambda\lambda$2039-2113 spectral feature in quasars appears systematically redshifted by amounts accountable under the hypothesis of gravitational redshift induced by the central supermassive black hole. Our…

星系天体物理 · 物理学 2018-08-08 E. Mediavilla , J. JimÉnez-Vicente , C. Fian , J. A. MuÑoz , E. Falco , V. Motta , E. Guerras

As the Universe expands, the redshift of distant sources changes with time. Here we discuss gravitational lensing phenomena that are consequence of the redshift drift between lensed source, gravitational lens, and observer. When the source…

宇宙学与河外天体物理 · 物理学 2022-06-01 Giovanni Covone , Mauro Sereno

We show that, in multimode Raman lasers, cascaded light scattering (CLS) not only extends the optical frequency range, but could also modulate the laser dynamics. The origin of this phenomenon is based on the fact that many Raman lasing…

The distribution of SDSS quasars is described. The dependence of observational number of quasars within distances to an observer less than r on distance r is found to be the power law with correlation dimension value equal 2,71 in redshift…

宇宙学与河外天体物理 · 物理学 2015-03-17 I. K. Rozgacheva , A. A. Agapov

Previous studies have shown that the normalization and scatter of the galaxy 'main sequence' (MS), the relation between star formation rate (SFR) and stellar mass ($M_*$), evolves over cosmic time. However, such studies often rely on…