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Letteratura scientifica selezionata sul tema "Strange stars"

Autore: Grafiati

Pubblicato: 10 dicembre 2022

Ultima modifica: 28 gennaio 2023

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Articoli di riviste sul tema "Strange stars"

1

Weiss, Peter. "Strange Stars?" Science News 161, n. 16 (20 aprile 2002): 246. http://dx.doi.org/10.2307/4013349.

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2

Alcock, Charles. "Strange stars". Nuclear Physics B - Proceedings Supplements 24, n. 2 (dicembre 1991): 93–102. http://dx.doi.org/10.1016/0920-5632(91)90305-x.

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3

Alcock, Charles, Edward Farhi e Angela Olinto. "Strange stars". Astrophysical Journal 310 (novembre 1986): 261. http://dx.doi.org/10.1086/164679.

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4

Reddy, Sanjay. "Strange crusts on strange stars". Journal of Physics G: Nuclear and Particle Physics 32, n. 12 (17 novembre 2006): S267—S274. http://dx.doi.org/10.1088/0954-3899/32/12/s33.

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5

Gondek, Dorota. "Neutron stars and strange stars". International Astronomical Union Colloquium 160 (1996): 133–34. http://dx.doi.org/10.1017/s0252921100041282.

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Abstract (sommario):

If strange quark plasma is the real ground state of baryonic matter (Witten 1984), then some of neutron stars (NS) could actually be strange stars (SS). It is difficult to distinguish SS from NS observationally. They have similar radii and masses and their crusts are built of the same matter. It seems that a good method for testing the existence of SS would be the studies of phenomena related to the stellar pulsations. In 1976 Boriakoff proposed that radial oscillations of NS could be observed within radio subpulses of pulsars. While various modes of pulsations of NS were studied by a number of authors, little attention was paid to seismological signatures of SS. The radial oscilations of bare SS were studied by Väth & Chanmugam (1992). Recently Weber (this volume) studied properties of stars made of matter described by BPS equation of state (EOS) (Baym et al. 1971) with a ball of strange matter inside, but they mainly concentrated on stability of white-dwarf-like SS. In this work I present fully relativistic calculations of the radial oscillation frequencies of SS. I determined the fundamental frequency for bare SS and SS with two different types of crusts depending on origin (Alcock et al. 1986) of SS and showed differences between them.

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6

Weber, Fridolin, e Norman K. Glendenning. "Neutron Stars, Strange Pulsars and Strange Dwarfs". International Astronomical Union Colloquium 160 (1996): 135–36. http://dx.doi.org/10.1017/s0252921100041294.

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The hypothesis that strange quark matter may be the absolute ground state of the strong interaction (not56Fe) has been raised independently by Boder and Witten. If the hypothesis is true, then a separate class of compact stars could exist, which are calledstrange matter stars. The properties of the complete sequence of such stars, which range from compact neutron-star-like strange stars to strange dwarfs to strange planets. The latter two constitute the strange counterparts of ordinary white dwarfs and planets, respectively. The properties of these objects are discussed in this paper.

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7

Haensel, Pawel, e Julian L. Zdunik. "Accreting strange stars". Nuclear Physics B - Proceedings Supplements 24, n. 2 (dicembre 1991): 139–43. http://dx.doi.org/10.1016/0920-5632(91)90312-3.

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8

Glendenning, N. K., Ch Kettner e F. Weber. "From Strange Stars to Strange Dwarfs". Astrophysical Journal 450 (settembre 1995): 253. http://dx.doi.org/10.1086/176136.

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9

Xu, R. X. "Strange Quark Stars — A Review". Symposium - International Astronomical Union 214 (2003): 191–98. http://dx.doi.org/10.1017/s0074180900194392.

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A pedagogical overview of strange quark matter and strange stars is presented. After a historical notation of the research and an introduction to quark matter, a major part is devoted to the physics and astrophysics of strange stars, with attention being paid to the possible ways by which neutron stars and strange stars can be distinguished in astrophysics. Recent possible evidence for bare strange stars is also discussed.

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10

Olinto, Angela. "Converting neutron stars into strange stars". Nuclear Physics B - Proceedings Supplements 24, n. 2 (dicembre 1991): 103–9. http://dx.doi.org/10.1016/0920-5632(91)90306-y.

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Tesi sul tema "Strange stars"

1

Ng, Chi-yung, e 吳志勇. "Theories of strange stars". Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 2001. http://hub.hku.hk/bib/B29868646.

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2

Ng, Chi-yung. "Theories of strange stars /". Hong Kong : University of Hong Kong, 2001. http://sunzi.lib.hku.hk:8888/cgi-bin/hkuto%5Ftoc%5Fpdf?B23316548.

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3

Harko, Tiberiu. "Properties of strange stars". Thesis, Hong Kong : University of Hong Kong, 2001. http://sunzi.lib.hku.hk:8888/cgi-bin/hkuto%5Ftoc%5Fpdf?B23242280.

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4

朱德權 e Tak-kuen Chu. "The structure and cooling of strange stars". Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 1998. http://hub.hku.hk/bib/B31220691.

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5

Chu, Tak-kuen. "The structure and cooling of strange stars /". Hong Kong : University of Hong Kong, 1998. http://sunzi.lib.hku.hk:8888/cgi-bin/hkuto%5Ftoc%5Fpdf?b20127182.

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6

Norsen, Travis T. "Strange phases in neutron star matter /". Thesis, Connect to this title online; UW restricted, 2002. http://hdl.handle.net/1773/9726.

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鄧敬來 e King-loy Tang. "The magnetic field evolution and cooling of superconducting strange stars". Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 2000. http://hub.hku.hk/bib/B3122345X.

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Tang, King-loy. "The magnetic field evolution and cooling of superconducting strange stars /". Hong Kong : University of Hong Kong, 2000. http://sunzi.lib.hku.hk/hkuto/record.jsp?B22535330.

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9

李浩然 e Ho-yin Lie. "A three dimensional approach for determining the surface magnetic field of strange stars". Thesis, The University of Hong Kong (Pokfulam, Hong Kong), 2000. http://hub.hku.hk/bib/B31224805.

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Lie, Ho-yin. "A three dimensional approach for determining the surface magnetic field of strange stars". Hong Kong : University of Hong Kong, 2000. http://sunzi.lib.hku.hk/hkuto/record.jsp?B23234532.

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Più fonti

Libri sul tema "Strange stars"

1

Brock, Randall. Stranger to the stars. Anchorage, Alaska: Calliopes Corner, 1986.

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2

Slavens, Kerry. Stranger under the stars: Poems. Victoria, B.C: Published for the Hawthorne Society by Reference West, 1992.

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3

Cohen, Daniel. Strange & amazing facts about Star Trek. New York: Pocket Books, 1986.

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4

Wesley, Smith Dean, Ordover John J e Block Paula M, a cura di. Strange New Worlds VI: Star Trek. New York: Pocket Books, 2003.

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5

Wesley, Smith Dean, Ordover John J e Block Paula M, a cura di. Strange New Worlds III: Star Trek. New York: Pocket Books, 2000.

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6

Wesley, Smith Dean, Ordover John J e Block Paula M, a cura di. Strange New Worlds IV: Star Trek. New York: Pocket, 2001.

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7

Wesley, Smith Dean, Ordover John J e Block Paula M, a cura di. Strange New Worlds V: Star Trek. New York: Pocket Books, 2002.

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8

Wesley, Smith Dean, Ordover John J, Kassin Elisa J e Block Paula M, a cura di. Strange New Worlds VII: Star Trek. New York: Pocket Books, 2004.

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9

Talis, Aurora. Strange Stars. Independently Published, 2020.

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10

United States. National Aeronautics and Space Administration., a cura di. Converting neutron stars into strange stars. [Batavia, Ill.?]: Fermi National Accelerator Laboratory, 1991.

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Capitoli di libri sul tema "Strange stars"

1

Glendenning, Norman K. "Strange Stars". In Compact Stars, 337–61. New York, NY: Springer US, 1997. http://dx.doi.org/10.1007/978-1-4684-0491-3_10.

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2

Glendenning, Norman K. "Strange Stars". In Compact Stars, 414–40. New York, NY: Springer New York, 2000. http://dx.doi.org/10.1007/978-1-4612-1212-6_12.

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3

Zhou, Enping. "Triaxially Rotating Strange Stars". In Springer Theses, 63–72. Singapore: Springer Singapore, 2020. http://dx.doi.org/10.1007/978-981-15-4151-3_4.

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4

Ng, Kin-Wang. "Conversion of Neutron Stars Into Strange Stars". In Stellar Astrophysics, 143–48. Dordrecht: Springer Netherlands, 2000. http://dx.doi.org/10.1007/978-94-010-0878-5_17.

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5

Vartanyan, Yu L. "SUPERDENSE STARS CONTAINING STRANGE BARYONS". In Ambartsumian’s Legacy and Active Universe, 179–92. New York, NY: Springer New York, 2011. http://dx.doi.org/10.1007/978-1-4614-0182-7_11.

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6

Weber, Fridolin. "Strange Quark Matter Inside Neutron Stars". In Handbook of Supernovae, 1–24. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-20794-0_71-1.

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7

Ng, C. Y., K. S. Cheng e M. C. Chu. "Properties of Cloudy Bag Strange Stars". In Astrophysics and Space Science Library, 83–90. Dordrecht: Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-0403-8_12.

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8

Seargent, David A. J. "Strange Stars and Star-Like Objects". In Astronomers' Universe, 163–97. New York, NY: Springer New York, 2010. http://dx.doi.org/10.1007/978-1-4419-6424-3_5.

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9

Deb, Debabrata, Sourav Roy Chowdhury, Saibal Ray, Farook Rahaman e B. K. Guha. "A Model for Anisotropic Strange Stars". In XXII DAE High Energy Physics Symposium, 65–68. Cham: Springer International Publishing, 2018. http://dx.doi.org/10.1007/978-3-319-73171-1_13.

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10

Weber, Fridolin. "Strange Quark Matter Inside Neutron Stars". In Handbook of Supernovae, 1423–46. Cham: Springer International Publishing, 2017. http://dx.doi.org/10.1007/978-3-319-21846-5_71.

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Atti di convegni sul tema "Strange stars"

1

Madsen, Jes. "Strange stars". In INTERSECTIONS BETWEEN PARTICLE AND NUCLEAR PHYSICS. ASCE, 1997. http://dx.doi.org/10.1063/1.54281.

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2

Weber, Fridolin, e Rodrigo Negreiros. "QCD in Neutron Stars and Strange Stars". In T(R)OPICAL QCD II WORKSHOP. AIP, 2011. http://dx.doi.org/10.1063/1.3587579.

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3

HARKO, TIBERIU, e KWONG SANG CHENG. "CAN STRANGE STARS BE DISTINGUISHED FROM NEUTRON STARS?" In Proceedings of the MG11 Meeting on General Relativity. World Scientific Publishing Company, 2008. http://dx.doi.org/10.1142/9789812834300_0099.

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4

Weber, F., Ch Kettner e N. K. Glendenning. "Properties of strange-matter stars". In The 3rd international symposium on nuclear astrophysics: Nuclei in the Cosmos III. AIP, 1995. http://dx.doi.org/10.1063/1.47327.

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5

Alaverdyan, Grigor, Yu L. Vartanyana, G. S. Hajyana, G. B. Alaverdyana, A. K. Grigoryan, A. R. Harutyunyan e H. A. Shahinyan. "Strange quark matter in compact stars". In The Modern Physics of Compact Stars 2015. Trieste, Italy: Sissa Medialab, 2016. http://dx.doi.org/10.22323/1.262.0006.

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6

Arbañil, José D. V., e Manuel Malheiro. "Stability of charged strange quark stars". In THE SECOND ICRANET CÉSAR LATTES MEETING: Supernovae, Neutron Stars and Black Holes. AIP Publishing LLC, 2015. http://dx.doi.org/10.1063/1.4937190.

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7

Dai, Z. G. "STRANGE STARS AND THEIR ASTROPHYSICAL IMPLICATIONS". In Proceedings of the Third Joint Meeting of Chinese Physicists Worldwide. WORLD SCIENTIFIC, 2002. http://dx.doi.org/10.1142/9789812776785_0056.

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8

Wiktorowicz, Grzegorz, A. Drago, G. Pagliara e S. Popov. "Formation scenarios of strange quark stars". In SN 1987A, Quark Phase Transition in Compact Objects and Multimessenger Astronomy. Институт ядерных исследования Российской академии наук, 2018. http://dx.doi.org/10.26119/sao.2020.1.52363.

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9

Usov, Vladimir V. "Extreme Plasmas Near Pulsars and Strange Stars". In PLASMA PHYSICS: 11th International Congress on Plasma Physics: ICPP2002. AIP, 2003. http://dx.doi.org/10.1063/1.1594042.

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10

Arbañil, José D. V., e Manuel Malheiro. "Equilibrium and stability of strange anisotropic stars". In Proceedings of the MG14 Meeting on General Relativity. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813226609_0148.

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Rapporti di organizzazioni sul tema "Strange stars"

1

Grassi, F. Quark core stars, quark stars and strange stars. Office of Scientific and Technical Information (OSTI), gennaio 1988. http://dx.doi.org/10.2172/5237159.

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2

Varriale, Amedeo. Institutionalized Populism: The “Strange Case” of the Italian Five Star Movement. European Center for Populism Studies (ECPS), giugno 2021. http://dx.doi.org/10.55271/op0009.

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The Five Star Movement (M5S) is one of those populist parties that is often misunderstood. Throughout the years, the media, independent journalists, and bloggers—as well as well-known academics and commentators—have struggled to define this “strange political creature.” Some have labeled it a polymorphous “hybrid-party” and others a “movement-party.” The mistake most analysts make when discussing the M5S is that they somehow forget the party’s left-wing origins.

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3

Willi, Joseph, Keith Stakes, Jack Regan e Robin Zevotek. Evaluation of Ventilation-Controlled Fires in L-Shaped Training Props. UL's Firefighter Safety Research Institute, ottobre 2016. http://dx.doi.org/10.54206/102376/mijj9867.

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Investigations of recent firefighter line of duty deaths caused by rapid fire progression have highlighted a deficiency in firefighters’ understanding of how certain tactics affect the fire dynamics of ventilation-controlled fires. Many fires are in a ventilation-limited, decay state by the time firefighters arrive at the scene, meaning that introducing additional ventilation to the environment has the potential to cause rapid and intense fire growth. To more effectively teach firefighters about the potential effects of ventilation on a compartment fire, ventilation-controlled fires should be gener- ated during training. Safely creating such fires while maintaining compliance with NFPA 1403: Standard on Live-Fire Training Evolutions allows instructors to educate students on this important principle of fire dynamics in the training environment. Structures utilized for live-fire training have evolved from typical concrete burn buildings to now include smaller purpose-built props, like those constructed from steel shipping containers or wood and gypsum board. Such props have been embraced by organizations due to their cost-effectiveness and potential to improve fire behavior training. Obtaining a thorough understanding of the capa- bilities and limitations of such props is critical for instructors to convey accurate messages during training and properly prepare firefighters for scenarios they’ll encounter in the field. Experiments were conducted to quantify the fire environment in L-shaped props with different wall constructions. One prop had an interior wall lining of gypsum board over wood studs and fiberglass insulation. The two other props were constructed from metal shipping containers with corrugated steel walls; one had ceilings and walls comprised solely of the corrugated steel, while the other had ceilings and walls comprised of rolled steel sheeting over mineral wool insulation with the corrugated steel wall as its backing. Three fuel packages were compared between the props: one contained furnishings mainly composed of synthetic materials and foam plastics; another contained wooden pallets and straw; and the third contained wooden pallets, straw, and oriented strand board (OSB). A stochastic approach was used to compare data between replicate tests and quantify the repeatability of the different props and fuel packages, all of which were deemed sufficiently repeatable. Comparisons of data between the three props revealed that thermal conditions between experiments in the two metal props were indistinguishable, suggesting that the additional layer of insulation did not significantly alter the fire environment. Additionally, thermal conditions in the gypsum-lined prop were more severe than those in the metal props. The effects of ventilation changes on fire conditions were also analyzed across various prop and fuel load combinations. Lastly, the response of the thermal environment in each prop during interior suppression was evaluated, and the results implied that the thermal exposure to the firefighter was more severe in the metal props than the gypsum prop for a brief period following the start of suppression.

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4

Sheridan, Anne. Annual report on migration and asylum 2016: Ireland. ESRI, novembre 2017. http://dx.doi.org/10.26504/sustat65.

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Abstract (sommario):

The Annual Report on Migration and Asylum 2016 provides an overview of trends, policy developments and significant debates in the area of asylum and migration during 2016 in Ireland. Some important developments in 2016 included: The International Protection Act 2015 was commenced throughout 2016. The single application procedure under the Act came into operation from 31 December 2016. The International Protection Office (IPO) replaced the Office of the Refugee Applications Commissioner (ORAC) from 31 December 2016. The first instance appeals body, the International Protection Appeals Tribunal (IPAT), replacing the Refugee Appeals Tribunal (RAT), was established on 31 December 2016. An online appointments system for all registrations at the Registration Office in Dublin was introduced. An electronic Employment Permits Online System (EPOS) was introduced. The Irish Short Stay Visa Waiver Programme was extended for a further five years to October 2021. The Second National Action Plan to Prevent and Combat Human Trafficking was published. 2016 was the first full year of implementation of the Irish Refugee Protection Programme (IRPP). A total of 240 persons were relocated to Ireland from Greece under the relocation strand of the programme and 356 persons were resettled to Ireland. Following an Oireachtas motion, the Government agreed to allocate up to 200 places to unaccompanied minors who had been living in the former migrant camp in Calais and who expressed a wish to come to Ireland. This figure is included in the overall total under the IRPP. Ireland and Jordan were appointed as co-facilitators in February 2016 to conduct preparatory negotiations for the UN high level Summit for Refugees and Migrants. The New York Declaration, of September 2016, sets out plans to start negotiations for a global compact for safe, orderly and regular migration and a global compact for refugees to be adopted in 2018. Key figures for 2016: There were approximately 115,000 non-EEA nationals with permission to remain in Ireland in 2016 compared to 114,000 at the end of 2015. Net inward migration for non-EU nationals is estimated to be 15,700. The number of newly arriving immigrants increased year-on-year to 84,600 at April 2017 from 82,300 at end April 2016. Non-EU nationals represented 34.8 per cent of this total at end April 2017. A total of 104,572 visas, both long stay and short stay, were issued in 2016. Approximately 4,127 persons were refused entry to Ireland at the external borders. Of these, 396 were subsequently admitted to pursue a protection application. 428 persons were returned from Ireland as part of forced return measures, with 187 availing of voluntary return, of which 143 were assisted by the International Organization for Migration Assisted Voluntary Return Programme. There were 532 permissions of leave to remain granted under section 3 of the Immigration Act 1999 during 2016. A total of 2,244 applications for refugee status were received in 2016, a drop of 32 per cent from 2015 (3,276). 641 subsidiary protection cases were processed and 431 new applications for subsidiary protection were submitted. 358 applications for family reunification in respect of recognised refugees were received. A total of 95 alleged trafficking victims were identified, compared with 78 in 2015.

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