www.reddit.com/r/AskEconomics/comments/1m4l6am/whats_the_economic_science_take_on_the_massive/
YouTube/Instagram channels like [Garys Economics](https://youtube.com/@garyseconomics?si=EHBeJVvWpoUEREMe), have been pushing that the massive income inequality that happen in the past decades is the ...
www.bing.com/ck/a?!&&p=53b2f9786c79c941999c9839917b80765a76396945f00f79bfaf3a664f5174ecJmltdHM9MTc3Mjc1NTIwMA&ptn=3&ver=2&hsh=4&fclid=2dd21e8e-e248-6677-3d95-099ae34d674c&u=a1aHR0cHM6Ly9hcG5ld3MuY29tL2h1Yi93aWxkZmlyZXM&ntb=1
Wildfires LA firefighter says he warned brush fire wasn’t out before massive blaze ignited A Los Angeles firefighter has testified that the ground was still smoldering from a brush fire days before a massive …
arxiv.org/abs/2504.00075v1
Observations of supermassive black holes (SMBHs) at high redshifts challenge standard seeding scenarios. We examine a dissipative self-interacting dark matter (dSIDM) model in which gravothermal collapse leads to the formation of massive BH seeds ab...
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Warm your self up with March Massive deals! Save on prebuilt pcs, custom gaming pcs, and gaming laptops!
arxiv.org/abs/1105.3877v1
In this work we study, under the Stratonovich definition, the problem of the damped oscillatory massive particle subject to a heterogeneous Poisson noise characterised by a rate of events, λ(t), and a magnitude, Φ, following an exponential distribu...
arxiv.org/abs/1402.5881v1
This paper introduces filter bank multicarrier (FBMC) as a potential candidate in the application of massive MIMO communication. It also points out the advantages of FBMC over OFDM (orthogonal frequency division multiplexing) in the application of ma...
arxiv.org/abs/2207.12446v3
Galaxies with stellar masses as high as $\sim 10^{11}$ solar masses have been identified out to redshifts $z \sim 6$, approximately one billion years after the Big Bang. It has been difficult to find massive galaxies at even earlier times, as the Bal...
arxiv.org/abs/2107.08160v1
This is the first of two papers studying localization of massive bulk fields on a bane in 5D anti-de Sitter spacetime, and some of their cosmological consequences. Here we focus on a massive 5D scalar, which is known to lack a localized mode, and dis...
arxiv.org/abs/2308.09763v1
Due to the presence of a gravitational anomaly in topologically massive gravity (TMG), the geometric entropy is no longer simply the Hubeny-Rangamani-Takayanagi (HRT) area; instead, it is given by the HRT area plus an anomalous contribution. We study...
arxiv.org/abs/2209.13625v2
We consider the Hill four-body problem where three oblate, massive bodies form a relative equilibrium triangular configuration, and the fourth, infinitesimal body orbits in a neighborhood of the smallest of the three massive bodies. We regularize col...
arxiv.org/abs/0808.0062v1
The Casimir force on two-dimensional pistons for massive scalar fields with both Dirichlet and hybrid boundary conditions is computed. The physical result is obtained by making use of generalized $ζ$-function regularization technique. The influenc...
arxiv.org/abs/1304.3726v1
Luminous high-redshift QSOs are thought to exist within the most massive dark matter haloes in the young Universe. As a consequence they are likely to be markers for biased, over-dense regions where early galaxies cluster, regions that eventually gro...
arxiv.org/abs/2201.03907v3
Massive random access plays a central role in supporting the Internet of Things (IoT), where a subset of a large population of users simultaneously transmit small packets to a central base station. While there has been much research on the design of...
arxiv.org/abs/hep-ph/0303016v2
Two-loop corrections for the form factor in a massive Abelian theory are evaluated, which result from the insertion of massless fermion or scalar loops into the massive gauge boson propagator. The result is valid for arbitrary energies and gauge bo...
arxiv.org/abs/1010.0236v1
We present radiation hydrodynamics simulations of the collapse of massive pre-stellar cores. We treat frequency dependent radiative feedback from stellar evolution and accretion luminosity at a numerical resolution down to 1.27 AU. In the 2D approxim...
arxiv.org/abs/astro-ph/0611140v1
We review the main properties of solar metallicity massive stars in the range 11-120 Msun. The influence of the mass loss on the hydrostatic burning stages as well as the final explosion is discussed in some detail. We find that the minimum masses...
www.reddit.com/r/DestinyTheGame/comments/a64v3t/massive_breakdown_of_black_armory_forge_and/
**If you'd like to hear a more in-depth discussion of these weapons and their perks, check out the [Massive Breakdown Podcast, Episode 98](https://soundcloud.com/destinymassivebreakdowns/episode-98-bl...
arxiv.org/abs/astro-ph/9509096v1
Most large elliptical galaxies should now host a massive black hole leftover from an earlier quasar phase. Such galaxies also have an extensive hot gaseous halo. Here we consider why the nuclei of elliptical galaxies are not luminous sources due to...
www.reddit.com/r/videos/comments/1p01zfz/cnn_chief_data_analyst_harry_enten_breaks_down/
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arxiv.org/abs/1912.02702v2
Extensive surveys with the \textit{Hubble Space Telescope} (HST) over the past decade, targeting some of the most massive clusters in the sky, have uncovered dozens of galaxy-cluster strong lenses. The massive cluster strong-lens scale is typically $...