Search or ask a question

Will there be black holes in star citizen?

Galaxy formation and evolution

Micro black hole

Answers from top 5 papers

PDF

Open Access

More filters

Papers (5)	Insight
Open access•Journal Article•DOI Quenching as a Contest between Galaxy Halos and their Central Black Holes Zhu Chen, S. M. Faber, David C. Koo, Rachel S. Somerville, Rachel S. Somerville, Joel R. Primack, Avishai Dekel, Aldo Rodríguez-Puebla, Yicheng Guo, Guillermo Barro, Dale D. Kocevski, A. van der Wel, A. van der Wel, Joanna Woo, Joanna Woo, Eric F. Bell, Jerome J. Fang, Henry C. Ferguson, Mauro Giavalisco, Marc Huertas-Company, Fangzhou Jiang, Susan A. Kassin, Lin Lin, Fengshan Liu, Fengshan Liu, Yifei Luo, Zhijian Luo, Camilla Pacifici, Viraj Pandya, Samir Salim, Chenggang Shu, Sandro Tacchella, Bryan A. Terrazas, Hassen M. Yesuf - Show less +33 more 24 Sep 2019-arXiv: Astrophysics of Galaxies 48 Citations	Implications include: the radii of star-forming galaxies are an important second parameter in shaping their black holes; black holes are connected to their halos but in different ways for star-forming, quenched, and green-valley galaxies; and the same BH-halo quenching mechanism has been in place since $z \sim 3$.
Open access•Journal Article•DOI Are nuclear star clusters the precursors of massive black holes Nadine Neumayer, C. Jakob Walcher - Show less +1 more 24 Jan 2012-arXiv: Cosmology and Nongalactic Astrophysics 19 Citations	We confirm that this class of galaxies has black holes with masses less than 106M⊙, if any.
Open access•Journal Article•DOI Black hole formation in a contracting universe Jerome Quintin, Robert Brandenberger - Show less +1 more 08 Sep 2016-Journal of Cosmology and Astroparticle Physics 30 Citations	Yet, the formation of black holes might be an interesting feature for other models.
Open access•Journal Article•DOI The lifetime problem of evaporating black holes: mutiny or resignation Carlos Barceló, Raúl Carballo-Rubio, Luis J. Garay, Luis J. Garay, Gil Jannes - Show less +4 more 04 Sep 2014-arXiv: General Relativity and Quantum Cosmology 22 Citations	This scenario motivates the search for new forms of stellar equilibrium different from black holes.
Book Chapter•DOI Astrophysics of black holes. Valeri P. Frolov, Igor D. Novikov - Show less +1 more 01 Jan 1998-Gravitation & Cosmology 20 Citations	Thus, we have to conclude that the physics of black holes, as well as the physics of stars, is the physics of celestial bodies.

My columns

Related Questions

Is blackholes time ports?5 answersBlackholes are not mentioned in any of the provided abstracts.

How many people have died from a black hole?5 answers

How many people have died from black hole?4 answers

How many real black hole pictures are there?5 answers

Is it normal to have a black hole after wisdom teeth removal?10 answers

What are the odds of Earth being sucked into a black hole?4 answers

See what other people are reading

What are the potential environmental impacts of ZDEC's carbon emissions?

The potential environmental impacts of ZDEC's carbon emissions can vary based on industrial practices and material applications. Studies suggest that industrial activities significantly contribute to carbon emissions, affecting global warming and climate change, with an observed inverted U-shaped relationship between industrial practices and carbon emissions in different emission level countries. Additionally, the use of zirconia, including doped zirconia with metals like osmium, as catalysts or catalyst supports, aims to reduce harmful emissions like carbon monoxide, which pose environmental hazards such as respiratory illnesses and contribute to global warming. Furthermore, the formation of ZrC in carbon composites can impact the graphitization degree of the carbon matrix, affecting mechanical and ablation properties, with high ZrC content potentially leading to negative influences on the carbon phase structure.How does stellar evolution depend on mass?

Stellar evolution significantly depends on mass. For massive single stars (8-30 solar masses), the implementation of cool supergiant mass loss affects their evolution, impacting Type II-P supernova light curves and progenitor masses determination. The evolution of galaxy ensembles at early times is directly related to the average acceleration of baryons onto dark matter halos, showing assembly bias and influencing the cosmic star formation rate density. Hot, massive stars lose mass through radiation-driven winds, affecting their evolution and surroundings, with lower mass-loss rates challenging the creation of classical Wolf-Rayet stars. Low-mass stars' angular momentum evolution is influenced by wind braking, dynamo, and mass-loss rate prescriptions, with differential rotation developing in the stellar interior and mass-dependent braking efficiency. White dwarfs' pollution fractions vary with mass, suggesting constraints on asteroid belt survival around main-sequence stars of different masses.What is wavelength?

A wavelength is a fundamental concept in various fields, including art, physics, and technology. In art, Michael Snow's film "Wavelength" exemplifies the concept through a forty-five-minute zoom shot. In physics, the wavelength of light plays a crucial role in measuring phenomena and enabling various scientific advancements through interference phenomena. Technologically, devices like wavelength measurement systems and wavelength detecting devices are designed to precisely measure and control wavelengths of light for different applications. Overall, a wavelength represents the distance between successive points of a wave, whether it's in the form of light, sound, or other waves, and its measurement and control are essential for a wide range of artistic, scientific, and technological endeavors.What are the common proposed solution connected to the statement of the problem about quasar travel agency?

The problem of quasars emitting large amounts of energy and exhibiting high redshifts has led to various proposed solutions. One common proposed solution is the idea that quasars could be close binary star systems, where a superstar orbits a supermassive black hole. Another proposed solution suggests that quasars are condensed central cores of galaxies at a certain point in their evolution. Additionally, recent discoveries of high-redshift quasars like J0313-1806 have provided insights into the formation mechanisms of supermassive black holes and their host galaxies, imposing constraints on seed black hole models and highlighting the need for further observational studies. These proposed solutions aim to address the perplexing nature of quasars and their extraordinary properties.What are the common proposed solutions for the given statement of the problem in quasar travel in tour?

The enigmatic nature of quasars has led to various proposed solutions to the problems they pose. Quasars, despite their small size, emit vast amounts of energy, exhibit high red-shifts, and are linked to both radiosources and visible stars. The powerful energy emission from quasars could potentially be explained by assuming that the emission is concentrated in a specific direction. Additionally, the study of distant quasars could play a role in determining the validity of quantum entanglement. To address the complexities surrounding quasars, the Given-Find-In Order To-Subjected To (GFIS) method has been proposed as a systematic approach to defining design problems and requirements, particularly in engineering contexts, enhancing decision-making abilities and solution feasibility.What are the demographic characteristics that define the Generation Z population?

Generation Z, often defined as the cohort born between 1995 and 2010, exhibits a range of demographic characteristics that distinguish it from previous generations. This group is recognized for its diversity, technological savviness, and progressive attitudes towards social and environmental issues. According to Barbara Pavlíková et al., Generation Z in Slovakia shows a decreasing trend in smoking behaviors, indicating a shift towards healthier lifestyle choices compared to older generations. Diana Bogueva and Dora Marinova's research highlights Generation Z's awareness of climate change and their inclination towards sustainable food choices, despite a significant portion still lacking understanding of the environmental impacts of their dietary habits. Financial literacy and management also define Generation Z, as Farizka Shafa Nabila et al. point out the influence of financial attitudes on their financial satisfaction, mediated by their financial management skills. This generation's engagement with technology and digital platforms significantly shapes their financial behaviors and investment decisions. In terms of health and wellness, Israel Martínez-Navarro et al. discuss the association between zinc levels and obesity in children, suggesting a focus on dietary factors that could influence Generation Z's physical health. Furthermore, L. Larsson et al. address the COVID-19 vaccine acceptance among youth in Zimbabwe, revealing disparities in vaccination rates based on sex, age, educational attainment, and socioeconomic status, which could reflect broader global trends within Generation Z. These characteristics underscore Generation Z's unique position at the intersection of health, technology, and environmental consciousness. Their behaviors and attitudes towards smoking, climate change, financial management, and health interventions like vaccination are indicative of a generation that is both informed and impacted by the global challenges of their time.What is three bodies problem?

The three-body problem involves studying the interactions and motion of three masses, such as planets or celestial bodies, under gravitational forces. Unlike the simpler two-body problem with analytical solutions, the three-body problem is complex and chaotic, lacking a general solution despite centuries of research. While some special cases have analytical solutions, they are often impractical, leading to the need for alternative approaches like neural networks. In a different perspective, the classical three-body problem can be formulated as geodesic flows on a Riemannian manifold, revealing hidden symmetries and complexities in the system. This problem's relevance extends to astrophysical phenomena like black hole mergers, where statistical solutions have been proposed, offering insights with fewer assumptions.How James Webb stirs values in cosmology?

The James Webb Space Telescope (JWST) revolutionizes cosmology by providing unprecedented capabilities for studying various aspects of the universe. JWST's infrared observations enable the exploration of galaxy formation and evolution, including high-redshift star-forming galaxies and trans-Neptunian objects, shedding light on the early universe and solar system evolution. Additionally, JWST's ability to characterize high-redshift quasars with exceptional depth and resolution offers insights into the most extreme objects in the universe, as well as the assembly of black holes at high redshifts, crucial for understanding cosmological simulations and the co-evolution of galaxies and black holes. The telescope's measurements challenge the Standard Cosmological Model, suggesting that cosmological data may have a microscopic origin rather than solely being attributed to the universe's expansion.Has anyone expanded on Lim?

Line-intensity mapping (LIM) has garnered attention as a technique to explore the large-scale structure of the Universe by capturing integrated spectral line intensities from various sources, shedding light on galaxy evolution and cosmological parameters. Researchers have developed computational frameworks like SkyLine to simulate realistic LIM observations, considering observational challenges like contamination and non-Gaussian fields. Studies have focused on modeling the LIM power spectrum, addressing degeneracies with astrophysical factors to enhance cosmological parameter extraction accuracy. LIM has been utilized to measure the baryon acoustic oscillation (BAO) scale, offering insights into the Universe's expansion history and aiding in resolving discrepancies in expansion rate measurements. These advancements in LIM technology and methodology pave the way for improved cosmological constraints and a deeper understanding of the Universe's evolution.What data exists on the Armenian song Shogher-jan or lovely Shoger?

The Armenian song "Shogher-jan" or "Lovely Shoger" is not directly addressed in the provided contexts. However, the research by Pavlova and Romanovafocuses on the poetics of color in Russian poetry dedicated to Armenia, highlighting the dominance of blue shades in describing the country. Additionally, the Armenian Data Cube initiativediscusses the deployment of an Armenian Data Cube for environmental monitoring, showcasing the collaboration between Switzerland and Armenia in utilizing Earth observation data. While these contexts do not specifically mention the song "Shogher-jan," they provide insights into cultural representations of Armenia through poetry and technological advancements in environmental monitoring, which could indirectly contribute to a broader understanding of Armenian cultural expressions like traditional songs.What are the 2 rrl local with diagram about SPTC HR information system?

The Soldier-Pile-Tremie-Concrete (SPTC) wall system is analyzed in the context of excavation support. The SPTC wall supported a 19.5m high cut with unique structural features like internal braces, including a horizontal steel truss and a post-tensioned reinforced concrete beam. The HR diagram, a key tool for locating stars, can be applied to low-luminosity stars, showing various types of diagrams based on observables or derived quantities. The HR diagram can also be used for galactic studies, incorporating the frequency of stars at different coordinates. The Hipparcos satellite detected variable stars, emphasizing stability areas and their significance in the HR diagram. By integrating these insights, a comprehensive understanding of the SPTC HR information system can be achieved, combining structural analysis with stellar classification methodologies.