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Coworking Spaces: Windows to the Future of Work? Changes in the Organizational Model of Work and the Attitudes of the Younger Generation

Ina Krause • Foresight and STI Governance (2019)

This paper analyzes how the organization of work has changed since the 1990s including the emergence of digital forms of employment. Following the evolution of work over the course of the 20th century and the start of the 21st, this paper i...

DOAJ Open Access (DOAJ) DOI: 10.17323/2500-2597.2019.2.52.60

The Algerian city is a space for protest movements: A study in the sociology of protest

Abdlhalim Mahourbacha • Journal of Umm Al-Qura University for Social Sciences (2022)

This study aims to provide a sociological view of the protest movements known to Algeria. And how the city streets turned in to a space for protest movements. In the first element, we discussed the urban policies and planning tools adopted ...

DOAJ Open Access (DOAJ) DOI: 10.54940/ss63539717

Course Design using an Authentic Studio Model / Restructuration de cours au moyen d’un authentique modèle de studio de design

Jay R Wilson • Canadian Journal of Learning and Technology (2013)

Educational Technology and Design 879 is a graduate course that introduces students to the basics of video design and production. In an attempt to improve the learning experience for students a redesign of the course was implemented for the...

DOAJ Open Access (DOAJ) DOI: 10.21432/T22S3P

Momentum-space Langevin dynamics of holographic Wilsonian RG flow: self-interacting massive scalar field with marginal deformation

Ji-seong Chae, Jae-Hyuk Oh • European Physical Journal C: Particles and Fields (2025)

Abstract We explore the mathematical relationship between the holographic Wilsonian renormalization group (HWRG) and stochastic quantization(SQ) motivated by the similarity of the monotonicity in RG flow with Langevin dynamics of non-equili...

DOAJ Open Access (DOAJ) DOI: 10.1140/epjc/s10052-025-14037-9

Where Galaxies Go to Die: The Environments of Massive Quiescent Galaxies at 3 < z < 5

Ian McConachie, Anna de Graaff, Michael V. Maseda, Joel Leja et al. • The Astrophysical Journal (2026)

At low redshift, massive quiescent galaxies (MQGs) are most frequently found in massive, rich galaxy clusters, but at high redshift the trend is less clear. Here, we present spectroscopic evidence of the effects of environment on the format...

DOAJ Open Access (DOAJ) DOI: 10.3847/1538-4357/aea6b5

Intergalactic Wandering Stars in the Local Universe: Theoretical Predictions for Their Distance and Luminosity Distribution

Jia-Hui Wang, Maosheng Xiang, Ji-Feng Liu • The Astrophysical Journal (2025)

Intergalactic wandering stars (IWSs) within 10 Mpc remain a poorly explored area of astronomy. Such stars, if they exist, are supposed to be wandering objects as they are not bound by the gravitational potential of any galaxy. We set out to...

DOAJ Open Access (DOAJ) DOI: 10.3847/1538-4357/adf8c8

Anti-de Sitter → de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Luis A. Anchordoqui, Ignatios Antoniadis, Dieter Lüst • Physics Letters B (2024)

Over the last few years, low- and high-redshift observations set off tensions in the measurement of the present-day expansion rate H0 and in the determination of the amplitude of the matter clustering in the late Universe (parameterized by ...

DOAJ Open Access (DOAJ) DOI: 10.1016/j.physletb.2024.138775

Scalar leptoquark effects on $$B \rightarrow \mu \bar{\nu }$$ B→μν¯ decay

Wei-Shu Hou, Tanmoy Modak, Gwo-Guang Wong • European Physical Journal C: Particles and Fields (2019)

Abstract Purely leptonic B meson decays provide unique probes for physics Beyond the Standard Model. We study the impact of a scalar leptoquark, $$S_1$$ S1 , on $$B \rightarrow \mu \bar{\nu }$$ B→μν¯ decay. We find that, for $$m_{S_1}\sim 1...

DOAJ Open Access (DOAJ) DOI: 10.1140/epjc/s10052-019-7490-0

An Investigation of Disk Thickness in M51 from Hα, Paα, and Mid-infrared Power Spectra

Bruce G. Elmegreen, Daniela Calzetti, Angela Adamo, Karin Sandstrom et al. • The Astrophysical Journal (2025)

Power spectra (PS) of high-resolution images of M51 (NGC 5194) taken with the Hubble Space Telescope and the James Webb Space Telescope (JWST) have been examined for evidence of disk thickness in the form of a change in slope between large ...

DOAJ Open Access (DOAJ) DOI: 10.3847/1538-4357/adcee6

On the Formation of Retrograde S-type Planets in Binaries with a Polar Circumbinary Disk

Cheng Chen, Philip J. Armitage, C. J. Nixon, Stephen H. Lubow et al. • The Astrophysical Journal Letters (2026)

Retrograde S-type planets have been observed in several binary systems, yet their formation pathway remains poorly understood. With high-resolution hydrodynamic simulations, we demonstrate that a polar circumbinary disk around an eccentric,...

DOAJ Open Access (DOAJ) DOI: 10.3847/2041-8213/ae9d4d

Radiative Processes in Astrophysics

G. B. Rybicki, Alan P. Lightman • Wiley eBooks (1985)

Chapter 1 Fundamentals of Radiative Transfer 1.1 The Electromagnetic Spectrum Elementary Properties of Radiation 1.2 Radiative Flux Macroscopic Description of the Propagation of Radiation Flux from an Isotropic Source-The Inverse Square Law...

OPENALEX DOI: https://doi.org/10.1002/9783527618170

Advances in Astrophysics

• Advances in Astrophysics (2021)

Astrophysics is the branch of astronomy that employs the principles of physics and chemistry to ascertain the nature of the heavenly bodies, rather than their positions or motions in space. Among the objects studied are the Sun, other s...

OPENALEX Open Access DOI: https://doi.org/10.22606/adap

Where Do Hot Jupiters Come from? Revisiting Tidal Disruption and Ejection in High-eccentricity Migration

Qianli Fan, Shang-Fei Liu • The Astrophysical Journal Letters (2026)

The origin of hot Jupiters remains a key open question. In the high-eccentricity migration scenario, traditional coreless models predict a strict tidal exclusion zone within ∼2.7 tidal radii r _t , in which giant planets are either fully di...

DOAJ Open Access (DOAJ) DOI: 10.3847/2041-8213/ae6659

Astronomy and Astrophysics

S. Darbon, A. Zavagno, J. M. Perrin, C. Savine et al. • The Physics Teacher (1986)

A parameter study is undertaken for steady symmetrical planar field-aligned MHD bow shock flows around a perfectly conducting cylinder.For sets of values of the inflow plasma β and Alfvénic Mach number (M A ) which allow for switch-on shock...

OPENALEX DOI: https://doi.org/10.1119/1.2342053