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The ARCADE 2 balloon bolometer along with a number of other instruments have detected what appears to be a radio synchrotron background at frequencies below about 3 GHz. Neither extragalactic radio sources nor diffuse Galactic emission can…

高能天体物理现象 · 物理学 2021-01-27 Martin G. H. Krause , Martin J. Hardcastle

The hypothesis of the self-induced collapse of the inflaton wave function was proposed as responsible for the emergence of inhomogeneity and anisotropy at all scales. This proposal was studied within an almost de Sitter space-time…

宇宙学与河外天体物理 · 物理学 2016-12-28 Micol Benetti , Susana J. Landau , Jailson S. Alcaniz

Sonoluminescence occurs when tiny bubbles rilled with noble gas atoms are driven by a sound wave. Each cycle of the driving field is accompanied by a collapse phase in which the bubble radius decreases rapidly until a short but very strong…

其他凝聚态物理 · 物理学 2010-11-11 Andreas Kurcz , Antonio Capolupo , Almut Beige

We revisit an inflationary scenario in which primordial inhomogeneities arise from a quantum collapse, a stochastic mechanism described in the context of quantum collapse theories in its continuous version and within semiclassical gravity.…

广义相对论与量子宇宙学 · 物理学 2026-03-04 María Pía Piccirilli , Gabriel León , Rosa-Laura Lechuga-Solis , Daniel Sudarsky

Many analyses of microwave background experiments neglect the correlation of noise in different frequency or polarization channels. We show that these correlations, should they be present, can lead to severe misinterpretation of an…

天体物理学 · 物理学 2009-10-22 Scott Dodelson , Arthur Kosowsky , Steven T. Myers

We provide a detailed analysis of quantum field theory around a collapsing shell and discuss several conceptual issues related to the emission of radiation flux and formation of black holes. Explicit calculations are performed using a model…

广义相对论与量子宇宙学 · 物理学 2009-11-19 Aseem Paranjape , T. Padmanabhan

We report on experimental observations of the bending of a dust acoustic shock wave around a dust void region. This phenomenon occurs as a planar shock wavefront encounters a compressible obstacle in the form of a void whose size is larger…

等离子体物理 · 物理学 2025-09-17 Sachin Sharma , Rauoof Wani , Prabhakar Srivastav , Meenakshee Sharma , Sayak Bose , Sanat Tiwari , Abhijit Sen

Neutron resonance spectrometry (NRS) has been used to measure the temperature inside Mo samples during shock loading. The temperatures obtained were significantly higher than predicted assuming ideal hydrodynamic loading. The effect of…

其他凝聚态物理 · 物理学 2008-03-06 Damian C. Swift , Achim Seifter , David B. Holtkamp , Vincent W. Yuan , David Bowman , David A. Clark

In the past years, large particle-physics experiments have shown that muon rate variations detected in underground laboratories are sensitive to regional, middle-atmosphere temperature variations. Potential applications include tracking…

We have analyzed recently published XENONnT data for the spontaneous X-ray emission signature predicted by the objective wave function collapse model of quantum mechanics. With extremely low background and large exposure, XENONnT data can…

量子物理 · 物理学 2023-01-05 Inwook Kim

The spatial and temporal noise properties of diffuse radiation is investigated in the context of the cosmic microwave background (CMB), although generic formulae that enable application to any other forms of incoherent light of a prescribed…

宇宙学与河外天体物理 · 物理学 2009-06-02 Richard Lieu , Bizhu Jiang

This paper discusses a quantum optical heating mechanism which might play an important role in sonoluminescence experiments. We suggest that this mechanism occurs during the final stages of the bubble collapse phase and accompanies the…

量子物理 · 物理学 2012-07-31 Almut Beige , Antonio Capolupo , Andreas Kurcz

The preheating of intergalactic medium(IGM) by structure collapsing and ultraviolet background(UVB) are investigated in cosmological hydrodynamical simulations. When gravitational collapsing is the sole heating mechanism, we find that (1)…

星系天体物理 · 物理学 2017-09-27 Weishan Zhu , Long-Long Feng

We confirm at the $5.7\sigma$ level previous studies reporting Cosmic Microwave Background (CMB) temperatures being significantly lower around nearby spiral galaxies than expected in the $\Lambda$CDM model. Results from our earlier work was…

宇宙学与河外天体物理 · 物理学 2025-04-23 Frode K. Hansen , Diego Garcia Lambas , Heliana E. Luparello , Facundo Toscano , Luis A. Pereyra

The effect of background dynamics of the universe on formation of large scale structures in the framework of Modified Newtonian Dynamics (MOND) is investigated. A spherical collapse model is used for modeling the formation of the…

广义相对论与量子宇宙学 · 物理学 2015-05-28 M. Malekjani , H. Haghi , D. M. Z Jassur

It is proposed that shock wave dynamics within the gas of a small bubble explain sonoluminescence, the emission of visible radiation. As the bubble radius oscillates, shock waves develop from spherical sound waves created inside the gas…

等离子体物理 · 物理学 2007-05-23 Sohrab Rahvar

The collapse of marginally Jeans unstable primordial gas clouds in the presence of UV radiation field is discussed. Assuming that the dynamical collapse proceeds approximately in an isothermal self-similar fashion, we investigate the…

天体物理学 · 物理学 2009-10-31 Hajime Susa , Tetsu Kitayama

We propose a non-Gaussianity test for gravitational wave backgrounds by combining data streams of multiple detectors. This simple method allows us to check whether a detected background is "smooth" enough to be consistent with an…

天体物理学 · 物理学 2009-11-13 Naoki Seto

To understand the boiling crisis mechanism, one can take advantage of the slowing down of boiling at high pressures, in the close vicinity of the liquid-vapor critical point of the given fluid. To preserve conventional bubble geometry, such…

The background spectrum of a germanium detector, shielded from the radiations arriving from the lower and open for the radiations arriving from the upper hemisphere is studied, both in a ground level and in an underground laboratory. It is…

仪器与探测器 · 物理学 2015-06-15 R. Banjanac , D. Maletić , D. Joković , N. Veselinović , A. Dragić , V. Udovičić , I. Aničin