Tag: cosmology

  • We’ve just doubled the number of gravitational waves we can find

    We’ve just doubled the number of gravitational waves we can find

    [ad_1]

    Gravitational wave detectors use laser beams in tubes that span kilometres

    The Virgo Collaboration

    Gravitational waves that span thousands to billions of miles can be obscured in our detectors by the smallest of quantum fluctuations that permeate space-time. But now, researchers at the Laser Interferometer Gravitational-Wave Observatory (LIGO) have found a way to beat this quantum noise. And as a result, they are finding nearly twice as many cosmic events as before.

    “We realised that quantum noise will be limiting us a long time ago. It’s not just a fancy [quantum] thing to demonstrate, it’s something that really affects the actual detector,” says Wenxuan Jia at the Massachusetts Institute of Technology.

    LIGO detects gravitational waves, ripples in the fabric of space-time created by dramatic cosmic events like collisions between black holes. To do so, it fires a laser beam along each of its two 4-kilometre-long arms, which sit perpendicular to each other. A passing gravitational wave squashes and expands the part of space-time where these arms reside, introducing a small difference between the distances travelled by the two beams.

    But that discrepancy is so tiny it can be hard to tell when it is caused by gravitational waves and when it is due to the nearly-imperceptible flickers of quantum fields that permeate all of space, including the laser light itself. The researchers found changing the quantum properties of the light could help them suppress the crackles of quantum fields and get a more distinct gravitational wave signal.

    They added a series of devices to the detector, including a special crystal and several lenses and mirrors, which all work together to “squeeze” LIGO’s light into a quantum state where correlations between light particles diminish the flickering.

    LIGO completed its first run with squeezed light in 2020, but the method only worked for gravitational waves with relatively high frequencies – those with lower frequencies actually produced more noisy signals than before. Jia and his colleagues modified the squeezing process to work equally well at both high and low frequencies before LIGO’s 2023 run. This change had a stunning effect: the number of gravitational waves it detected nearly doubled, effectively allowing the machine to reveal a larger part of our universe.

    “Pushing the boundaries of quantum measurement has pushed the boundaries of space-time measurement, which is truly a beautiful thing,” says Chad Hanna at the Pennsylvania State University. He says this advanced precision will enable LIGO to see black hole mergers “all the way back to the formation of the first stars”.

    Bruce Allen at the Max Planck Institute for Gravitational Physics in Germany says there are several new kinds of gravitational waves physicists would like to see with LIGO’s newfound precision. This includes those emitted constantly by bumpy neutron stars as they rotate, as opposed to the ones they emit when they collide with something, which has been the origin of most gravitational waves detected to date.

    The upgrade also opens the door for fully new discoveries, as it could help probe the gravitational wave background that permeates space-time. “Every time you increase the sensitivity [of your detectors], you increase your chances of encountering the unexpected,” says Allen.

    Topics:

    [ad_2]

    Source link

  • We physicists could learn a lot by stepping beyond our specialisms

    We physicists could learn a lot by stepping beyond our specialisms

    [ad_1]

    Atomic molecule on blackboard; Shutterstock ID 635006972; purchase_order: -; job: -; client: -; other: -

    Shutterstock/Creative-To​uch

    A century ago, it was possible for a physicist to know almost everything there was to know about physics. Now, this is far from the case. It isn’t that the physicists of today are less competent. The problem is that humans simply know so much about the inner workings of the universe that it is impossible for someone to be deeply familiar with all of it. As a result, today’s tendency is to produce specialists.

    For example, I trained initially as a relativist: general relativity and quantum extensions of it, applied to cosmology, were my specialist areas of physics. Eventually,…

    [ad_2]

    Source link

  • Hardcastle, M. J. et al. Radio-loud AGN in the first LoTSS data release. The lifetimes and environmental impact of jet-driven sources. Astron. Astrophys. 622, A12 (2019).

    Article 
    CAS 

    Google Scholar
     

  • Perucho, M., Martí, J.-M. & Quilis, V. Long-term FRII jet evolution: clues from three-dimensional simulations. Mon. Not. R. Astron. Soc. 482, 3718–3735 (2019).

    Article 
    ADS 
    CAS 

    Google Scholar
     

  • Dabhade, P., Saikia, D. J. & Mahato, M. Decoding the giant extragalactic radio sources. J. Astrophys. Astron. 44, 13 (2023).

    Article 
    ADS 

    Google Scholar
     

  • Ayromlou, M., Nelson, D. & Pillepich, A. Feedback reshapes the baryon distribution within haloes, in halo outskirts, and beyond: the closure radius from dwarfs to massive clusters. Mon. Not. R. Astron. Soc. 524, 5391–5410 (2023).

    Article 
    ADS 
    CAS 

    Google Scholar
     

  • Beck, A. M., Hanasz, M., Lesch, H., Remus, R. S. & Stasyszyn, F. A. On the magnetic fields in voids. Mon. Not. R. Astron. Soc. 429, L60–L64 (2013).

    Article 
    ADS 

    Google Scholar
     

  • Vazza, F. et al. Simulations of extragalactic magnetic fields and of their observables. Class. Quantum Gravity 34, 234001 (2017).

    Article 
    ADS 

    Google Scholar
     

  • Willis, A. G., Strom, R. G. & Wilson, A. S. 3C236, DA240; the largest radio sources known. Nature 250, 625–630 (1974).

    Article 
    ADS 

    Google Scholar
     

  • Machalski, J., Kozieł-Wierzbowska, D., Jamrozy, M. & Saikia, D. J. J1420–0545: the radio galaxy larger than 3C 236. Astrophys. J. 679, 149–155 (2008).

    Article 
    ADS 
    CAS 

    Google Scholar
     

  • Oei, M. S. S. L. et al. The discovery of a radio galaxy of at least 5 Mpc. Astron. Astrophys. 660, A2 (2022).

    Article 

    Google Scholar
     

  • Correa, C. M. et al. Redshift-space effects in voids and their impact on cosmological tests. Part I: the void size function. Mon. Not. R. Astron. Soc. 500, 911–925 (2021).

    Article 
    ADS 
    CAS 

    Google Scholar
     

  • Perucho, M. Dissipative processes and their role in the evolution of radio galaxies. Galaxies 7, 70 (2019).

    Article 
    ADS 

    Google Scholar
     

  • Andernach, H., Jiménez-Andrade, E. F. & Willis, A. G. Discovery of 178 giant radio galaxies in 1059 deg2 of the Rapid ASKAP Continuum Survey at 888 MHz. Galaxies 9, 99 (2021).

    Article 
    ADS 

    Google Scholar
     

  • Dabhade, P. et al. Giant radio galaxies in the LOFAR Two-metre Sky Survey. I. Radio and environmental properties. Astron. Astrophys. 635, A5 (2020).

    Article 

    Google Scholar
     

  • Oei, M. S. S. L. et al. Measuring the giant radio galaxy length distribution with the LoTSS. Astron. Astrophys. 672, A163 (2023).

    Article 

    Google Scholar
     

  • Mostert, R. I. J. et al. Constraining the giant radio galaxy population with machine learning and Bayesian inference. Preprint at https://arxiv.org/abs/2405.00232 (2024).

  • Hardcastle, M. J. et al. The LOFAR Two-Metre Sky Survey. VI. Optical identifications for the second data release. Astron. Astrophys. 678, A151 (2023).

    Article 

    Google Scholar
     

  • Heckman, T. M. & Best, P. N. The coevolution of galaxies and supermassive black holes: insights from surveys of the contemporary universe. Annu. Rev. Astron. Astrophys. 52, 589–660 (2014).

    Article 
    ADS 

    Google Scholar
     

  • Hardcastle, M. Interpreting radiative efficiency in radio-loud AGNs. Na. Astron. 2, 273–274 (2018).

    Article 
    ADS 

    Google Scholar
     

  • Buttiglione, S. et al. An optical spectroscopic survey of the 3CR sample of radio galaxies with z < 0.3. II. Spectroscopic classes and accretion modes in radio-loud AGN. Astron. Astrophys. 509, A6 (2010).

    Article 

    Google Scholar
     

  • Williams, W. L. et al. LOFAR-Boötes: properties of high- and low-excitation radio galaxies at 0.5 < z < 2.0. Mon. Not. R. Astron. Soc. 475, 3429–3452 (2018).

    Article 
    ADS 
    CAS 

    Google Scholar
     

  • Oei, M. S. S. L. et al. Luminous giants populate the dense Cosmic Web. The radio luminosity–environmental density relation for radio galaxies in action. Astron. Astrophys. 686, A137 (2024).

    Article 

    Google Scholar
     

  • Wen, Z. L. & Han, J. L. A catalog of 1.58 million clusters of galaxies identified from the DESI Legacy Imaging Surveys. Astrophys. J. Suppl. Ser. 272, 39 (2024).

    Article 
    ADS 

    Google Scholar
     

  • Planck Collaboration et al. Planck 2015 results. XXVII. The second Planck catalogue of Sunyaev-Zeldovich sources. Astron. Astrophys. 594, A27 (2016).

    Article 

    Google Scholar
     

  • Ineson, J. et al. Radio-loud active galactic nucleus: is there a link between luminosity and cluster environment? Astrophys. J. 770, 136 (2013).

    Article 
    ADS 

    Google Scholar
     

  • Ineson, J. et al. The link between accretion mode and environment in radio-loud active galaxies. Mon. Not. R. Astron. Soc. 453, 2682–2706 (2015).

    Article 
    ADS 

    Google Scholar
     

  • Forero-Romero, J. E., Hoffman, Y., Gottlöber, S., Klypin, A. & Yepes, G. A dynamical classification of the cosmic web. Mon. Not. R. Astron. Soc. 396, 1815–1824 (2009).

    Article 
    ADS 

    Google Scholar
     

  • van Weeren, R. J. et al. Radio observations of ZwCl 2341.1+0000: a double radio relic cluster. Astron. Astrophys. 506, 1083–1094 (2009).

    Article 
    ADS 

    Google Scholar
     

  • Hardcastle, M. J. A simulation-based analytic model of radio galaxies. Mon. Not. R. Astron. Soc. 475, 2768–2786 (2018).

    Article 
    ADS 

    Google Scholar
     

  • Planck Collaboration et al. Planck 2018 results. VI. Cosmological parameters. Astron. Astrophys. 641, A6 (2020).

    Article 

    Google Scholar
     

  • van Haarlem, M. P. et al. LOFAR: the LOw-Frequency ARray. Astron. Astrophys. 556, A2 (2013).

    Article 

    Google Scholar
     

  • Shimwell, T. W. et al. The LOFAR Two-metre Sky Survey. V. Second data release. Astron. Astrophys. 659, A1 (2022).

    Article 

    Google Scholar
     

  • Shimwell, T. W. et al. The LOFAR Two-metre Sky Survey. I. Survey description and preliminary data release. Astron. Astrophys. 598, A104 (2017).

    Article 

    Google Scholar
     

  • Tasse, C. et al. DDFacet: facet-based radio imaging package. Astrophysics Source Code Library, record ascl:2305.008 (2023).

  • van Weeren, R. J. et al. LOFAR observations of galaxy clusters in HETDEX. Extraction and self-calibration of individual LOFAR targets. Astron. Astrophys. 651, A115 (2021).

    Article 

    Google Scholar
     

  • Offringa, A. R. et al. WSCLEAN: an implementation of a fast, generic wide-field imager for radio astronomy. Mon. Not. R. Astron. Soc. 444, 606–619 (2014).

    Article 
    ADS 

    Google Scholar
     

  • Morabito, L. K. et al. Sub-arcsecond imaging with the International LOFAR Telescope. I. Foundational calibration strategy and pipeline. Astron. Astrophys. 658, A1 (2022).

    Article 

    Google Scholar
     

  • Jackson, N. et al. LBCS: the LOFAR Long-Baseline Calibrator Survey. Astron. Astrophys. 595, A86 (2016).

    Article 

    Google Scholar
     

  • Jackson, N. et al. Sub-arcsecond imaging with the International LOFAR Telescope. II. Completion of the LOFAR Long-Baseline Calibrator Survey. Astron. Astrophys. 658, A2 (2022).

    Article 

    Google Scholar
     

  • Gupta, Y. et al. The upgraded GMRT: opening new windows on the radio Universe. Curr. Sci. 113, 707–714 (2017).

    Article 
    ADS 

    Google Scholar
     

  • Intema, H. T. SPAM: Source Peeling and Atmospheric Modeling. Astrophysics Source Code Library, record ascl:1408.006 (2014).

  • Mohan, N. & Rafferty, D. PyBDSF: Python Blob Detection and Source Finder. Astrophysics Source Code Library, record ascl:1502.007 (2015).

  • Blandford, R. D. & Znajek, R. L. Electromagnetic extraction of energy from Kerr black holes. Mon. Not. R. Astron. Soc. 179, 433–456 (1977).

    Article 
    ADS 

    Google Scholar
     

  • Alam, S. et al. The eleventh and twelfth data releases of the Sloan Digital Sky Survey: final data from SDSS-III. Astrophys. J. Suppl. Ser. 219, 12 (2015).

    Article 
    ADS 

    Google Scholar
     

  • Dey, A. et al. Overview of the DESI Legacy Imaging Surveys. Astron. J. 157, 168 (2019).

    Article 
    ADS 
    CAS 

    Google Scholar
     

  • Duncan, K. J. All-purpose, all-sky photometric redshifts for the Legacy Imaging Surveys Data Release 8. Mon. Not. R. Astron. Soc. 512, 3662–3683 (2022).

    Article 
    ADS 
    CAS 

    Google Scholar
     

  • Oke, J. B. et al. The Keck low-resolution imaging spectrometer. Publ. Astron. Soc. Pac. 107, 375 (1995).

    Article 
    ADS 

    Google Scholar
     

  • McCarthy, J. K. et al. in Proc. SPIE Conference on Optical Astronomical Instrumentation (ed. D’Odorico, S.) 81–92 (SPIE, 1998).

  • Steidel, C. C. et al. A survey of star-forming galaxies in the 1.4 z 2.5 redshift desert: overview. Astrophys. J. 604, 534–550 (2004).

    Article 
    ADS 
    CAS 

    Google Scholar
     

  • Rockosi, C. et al. in Proc. Ground-based and Airborne Instrumentation for Astronomy III (eds McLean, I. S., Ramsay, S. K. & Takami, H.) 77350R (SPIE, 2010).

  • Prochaska, J. et al. PypeIt: the Python spectroscopic data reduction pipeline. J. Open Source Softw. 5, 2308 (2020).

    Article 
    ADS 

    Google Scholar
     

  • Dawson, K. S. et al. The Baryon Oscillation Spectroscopic Survey of SDSS-III. Astron. J. 145, 10 (2013).

    Article 
    ADS 

    Google Scholar
     

  • Chambers, K. C. et al. The Pan-STARRS1 surveys. Preprint at https://arxiv.org/abs/1612.05560 (2019).

  • Jarrett, T. H. et al. The Spitzer–WISE survey of the ecliptic poles. Astrophys. J. 735, 112 (2011).

    Article 
    ADS 

    Google Scholar
     

  • Calistro Rivera, G., Lusso, E., Hennawi, J. F. & Hogg, D. W. AGNfitter: a Bayesian MCMC approach to fitting spectral energy distributions of AGNs. Astrophys. J. 833, 98 (2016).

    Article 
    ADS 

    Google Scholar
     

  • Martínez-Ramírez, L. N. et al. AGNFITTER-RX: Modeling the radio-to-X-ray spectral energy distributions of AGNs. Astron. Astrophys. 688, A46 (2024).

  • Pasini, T. et al. Radio galaxies in galaxy groups: kinematics, scaling relations, and AGN feedback. Mon. Not. R. Astron. Soc. 505, 2628–2637 (2021).

    Article 
    ADS 
    CAS 

    Google Scholar
     

  • Arnaud, M. et al. The universal galaxy cluster pressure profile from a representative sample of nearby systems (REXCESS) and the YSZ – M500 relation. Astron. Astrophys. 517, A92 (2010).

    Article 

    Google Scholar
     

  • Sun, M. et al. The pressure profiles of hot gas in local galaxy groups. Astrophys. J. Lett. 727, L49 (2011).

    Article 
    ADS 

    Google Scholar
     

  • Cooke, R. J. & Fumagalli, M. Measurement of the primordial helium abundance from the intergalactic medium. Nat. Astron. 2, 957–961 (2018).

    Article 
    ADS 

    Google Scholar
     

  • Lovisari, L., Reiprich, T. H. & Schellenberger, G. Scaling properties of a complete X-ray selected galaxy group sample. Astron. Astrophys. 573, A118 (2015).

    Article 
    ADS 

    Google Scholar
     

  • Ricciardelli, E., Quilis, V. & Planelles, S. The structure of cosmic voids in a ΛCDM Universe. Mon. Not. R. Astron. Soc. 434, 1192–1204 (2013).

    Article 
    ADS 

    Google Scholar
     

  • Upton Sanderbeck, P. R., D’Aloisio, A. & McQuinn, M. J. Models of the thermal evolution of the intergalactic medium after reionization. Mon. Not. R. Astron. Soc. 460, 1885–1897 (2016).

    Article 
    ADS 

    Google Scholar
     

  • Tuominen, T. et al. An EAGLE view of the missing baryons. Astron. Astrophys. 646, A156 (2021).

    Article 
    CAS 

    Google Scholar
     

  • Hardcastle, M. J. & Krause, M. G. H. Numerical modelling of the lobes of radio galaxies in cluster environments. Mon. Not. R. Astron. Soc. 430, 174–196 (2013).

    Article 
    ADS 

    Google Scholar
     

  • Barrows, R. S., Comerford, J. M., Stern, D. & Assef, R. J. A catalog of host galaxies for WISE-selected AGN: connecting host properties with nuclear activity and identifying contaminants. Astrophys. J. 922, 179 (2021).

    Article 
    ADS 
    CAS 

    Google Scholar
     

  • Chen, Z.-F., Pan, D.-S., Pang, T.-T. & Huang, Y. A catalog of quasar properties from the Baryon Oscillation Spectroscopic Survey. Astrophys. J. Suppl. Ser. 234, 16 (2018).

    Article 
    ADS 

    Google Scholar
     

  • Sweijen, F. GitHub repository for legacystamps. https://github.com/tikk3r/legacystamps (2021).

  • LOFAR Collaboration. Website for LOFAR surveys data, including LoTSS DR2. https://lofar-surveys.org (2022).

  • Hardcastle, M. J. GitHub repository for ‘A simulation-based analytic model of radio galaxies’. https://github.com/mhardcastle/analytic (2021).

  • Oei, M. S. S. L. Code Ocean capsule for ‘Black hole jets on the scale of the cosmic web’. https://codeocean.com/capsule/3908804/tree (2024).

  • Lang, D., Hogg, D. W. & Schlegel, D. J. WISE photometry for 400 million SDSS sources. Astron. J. 151, 36 (2016).

    Article 
    ADS 

    Google Scholar
     

  • Gordon, Y. A. et al. A quick look at the 3 GHz radio sky. I. Source statistics from the Very Large Array Sky Survey. Astrophys. J. Suppl. Ser. 255, 30 (2021).

    Article 
    ADS 
    CAS 

    Google Scholar
     

  • Helfand, D. J., White, R. L. & Becker, R. H. The last of FIRST: the final catalog and source identifications. Astrophys. J. 801, 26 (2015).

    Article 
    ADS 

    Google Scholar
     

[ad_2]

Source link

  • We finally know exactly how dark deep space is

    We finally know exactly how dark deep space is

    [ad_1]

    NASA’s New Horizons spacecraft in deep space

    NASA, APL, SwRI, Serge Brunier (ESO), Marc Postman (STScI), Dan Durda

    We finally know just how dark it is in deep space. NASA’s New Horizons spacecraft has made the first precise measurements of the ambient light that suffuses the universe, called the cosmic optical background.

    The cosmic optical background is so dim that it is impossible to measure with any precision from Earth – the glow of objects in the inner solar system far outshines it. “Every time you try to measure it from Earth, or from near Earth, you’re going to…

    [ad_2]

    Source link

  • How Einstein was both right and wrong about gravitational waves

    How Einstein was both right and wrong about gravitational waves

    [ad_1]

    Gravitational waves are vibrations in space-time itself

    Peter Jurik/Alamy

    The following is an extract from our Lost in Space-Time newsletter. Each month, we hand over the keyboard to a physicist or mathematician to tell you about fascinating ideas from their corner of the universe. You can sign up for Lost in Space-Time for free here.

    From our current vantage point, gravitational waves appear to be a ubiquitous phenomenon in the cosmos. The first detection of these ripples in space-time came in September 2015 at the Laser Interferometer Gravitational-Wave Observatory (LIGO). The waves captured were the by-product of a…

    [ad_2]

    Source link

  • This mind-blowing map shows Earth’s position within the vast universe

    This mind-blowing map shows Earth’s position within the vast universe

    [ad_1]

    New Scientist. Science news and long reads from expert journalists, covering developments in science, technology, health and the environment on the website and the magazine.

    This story is part of our Cosmic Perspective series, in which we confront the staggering vastness of the cosmos and our place in it. Read the rest of the series here.

    This map shows the circle of the cosmos that surrounds us, extending to a distance of 200 million light years. At this scale, space is comprised of clusters of galaxies and voids, the latter being areas with relatively few galaxies. The Milky Way, at the centre, is part of the Local Group of galaxies, with the Virgo cluster our nearest neighbour.

    Majestic spiral

    The Milky Way’s spiral structure is dominated by two main arms called Scutum-Centaurus and Perseus. It also features a dense region known as the central bar. Our solar system lies on a more modest structure called the Orion spur.

    However tangled the question of our metaphorical place in the universe, we can use astronomy to grasp Earth’s physical location.

    Earth orbits the sun at a distance of 150 million kilometres and the sun orbits the centre of the Milky Way. Specifically, we are in the Orion arm, around 26,500 light years from the centre.

    The Milky Way resides in the Local Group of galaxies. About 2.5 million light years away is our closest neighbouring galaxy, Andromeda, the largest galaxy in the Local Group. Right now, we are hurtling towards Andromeda at more than 100 kilometres per second; in about 4 billion years, the two galaxies will collide.

    The Local Group

    That will shake up the Local Group, but it will be barely a blip on the radar of the wider cosmic neighbourhood.…

    [ad_2]

    Source link

  • The universe is built a lot like a giant brain – so is it conscious?

    The universe is built a lot like a giant brain – so is it conscious?

    [ad_1]

    Head star made with 3d illustration image.; Shutterstock ID 1765794698; purchase_order: -; job: -; client: -; other: -

    An astrophysicist and a surgeon walk into a bar. No, this isn’t the start of a bad joke. A few years ago, astrophysicist Franco Vazza met his childhood friend Alberto Feletti, who had become a neurosurgeon. As they reminisced and chatted about their work – Vazza modelling the structure of the universe, Feletti poring over the composition of the brain – a thought struck them: why not compare the two?

    Vazza, based at the University of Bologna, Italy, did just that. He used statistical methods to compare the neurons in one area of the brain, the cortex, with the cosmic web, the pattern of matter distribution across the universe. Vazza looked at the number of nodes in each network and how densely each node was connected. The results surprised him. “It is a tantalising level of similarity,” he says. The structures differ in size by some 27 orders of magnitude. But if you ignore that, “the two patterns sort of overlap”, says Vazza.

    For some physicists, this likeness is too tempting to ignore. Some have even suggested the possibility that the universe “thinks” or is in some sense conscious, an idea with roots in the philosophy of panpsychism.

    Traditionally, researchers explained consciousness in one of two ways. Materialists say matter is all there is and consciousness – somehow – emerges from it. Dualists say there are fundamentally two kinds of stuff: matter stuff and consciousness stuff. Much ink has been spilled on the shortcoming of both ideas. For instance, how exactly does consciousness arise from pure matter?

    Panpsychism

    For some,…

    [ad_2]

    Source link

  • We are closer than ever to finally proving the multiverse exists

    We are closer than ever to finally proving the multiverse exists

    [ad_1]

    the surface of an multiverse with a lot of universes 3d rendering; Shutterstock ID 2256998119; purchase_order: -; job: -; client: -; other: -

    Shutterstock/Dr. Norbert Lange

    We think our universe contains everything that exists, has ever existed and will exist in the future. But this might not be the case: there are many ways other universes could exist.

    One is that we could be a single part of a branch of infinite universes known collectively as the multiverse. These universes might have appeared shortly after the big bang, they might be hiding in extra dimensions or they could pop into existence whenever a quantum property goes from a cloud of possible states to a single reality.

    Multiverse ideas gained scientific weight in the 1980s with the invention of inflation, a period when the early universe suddenly expanded. Inflation explains why the cosmos is so flat and smooth, but it also predicts the creation of a multitude of independent bubble universes.

    Cyclic universes

    Yet inflation is just one route to a multiverse, and it has its critics. In recent years, many cosmologists have turned to alternatives like cyclic universe theories, which say the universe is on an unending cycle between ballooning and compressing. These theories still invoke multiple universes, but at different times.

    “What I didn’t like about inflation was that there are very few genuine predictions – you don’t get out much more than you put in,” says Neil Turok, a physicist at the University of Edinburgh, UK, who helped develop a model for a cyclic universe, published in 2001, as a rival for inflation. “It just struck me that there has to be a better explanation.”

    The cyclic universe has its…

    [ad_2]

    Source link

  • Odd black holes smaller than protons may have once littered the cosmos

    Odd black holes smaller than protons may have once littered the cosmos

    [ad_1]

    Colour-charged black holes may have formed in the early universe

    betibup33/Shutterstock

    The universe may have once been speckled with tiny black holes with a strange property called colour charge. These exotic objects, if they existed, would have formed in the instants after the big bang and evaporated just as quickly, but they could have upset the balance of elements that formed in the early universe.

    Minuscule black holes formed right at the beginning of the cosmos are known as primordial black holes. Because of their…

    [ad_2]

    Source link

  • What “naked” singularities are revealing about quantum space-time

    What “naked” singularities are revealing about quantum space-time

    [ad_1]

    New Scientist. Science news and long reads from expert journalists, covering developments in science, technology, health and the environment on the website and the magazine.

    adbobe stock/Erika Eros/Alamy/collarge ryan wills

    Deep inside a black hole, the cosmos gets twisted beyond comprehension. Here, at some infinitesimal point of infinite density, the fabric of the universe gets so ludicrously warped that Albert Einstein’s general theory of relativity, which describes how mass bends space-time, ceases to make sense. At the singularity, our understanding falls apart.

    As daunting as singularities are, each one is at least safely tucked away inside the event horizon of a black hole, the boundary beyond which we can’t see. This not only cloaks them from view, but also stops unknown effects they herald, namely the horrors of unpredictability, from leaching out into the wider universe. But what if singularities could exist outside black holes after all?

    That question, given fresh impetus in recent years by demonstrations that general relativity allows for this, has spurred theorists to probe singularities from a deeper perspective, folding in insights from the latest forays into the possible quantum foundations of gravity. Already, they are realising that this new approach “flips the script” on how we think about singularities, says Netta Engelhardt at the Massachusetts Institute of Technology.

    Fair warning: the work takes us into some labyrinthine physics. But by grappling with singularities in this way, Engelhardt and her colleagues are deciphering the enigmatic connections between the quantum realm and classical gravity – and reinforcing the revolutionary idea that…

    [ad_2]

    Source link