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| 03.01.10. astro-ph za 01 - 10 2002 goda: izbrannye stat'i |
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Authors: Massimo Turatto
Authors: Andrew R. King
Authors: F. Halzen
Authors: Clifford M. Will
Authors: Mario Hamuy (OCIW) Commets: 26 pages, 15 figures, Review for `Core Collapse of Massive Stars'', Ed. C.L. Fryer, Kluwer, Dordrecht Daetsya podrobnyi i ponyatnyi obzor svoistv sverhnovyh, gde, kak polagayut, imel mesto kollaps yadra massivnoi zvezdy (tipy II, Ib,c). Avtor obrashaet osoboe vnimanie na to, chto pri vsem raznoobrazii nablyudatel'nyh proyavlenii svoistva etogo fenomena menyayutsya nepreryvno i, sledovatel'no, mehanizm vzryva u vseh sverhnovyh etogo klassa dolzhen byt' odinakov. Sm. takzhe nizhe astro-ph/0301107.
Authors: Lawrence M. Krauss Commets: 20 pages, To appear in Proceedings, ESO-CERN-ESA Symposium on Astronomy, Cosmology and Fundamental Physics, March 2002 Nazvanie govorit samo za sebya. Obzor sovremennyh nablyudenii kosmologicheskih parametrov, a takzhe sledstvii, kotorye iz etogo vytekayut. Formul malo, i oni prostye. Sm. takzhe stat'yu " Cosmological Parameters: Fashion and Facts" astro-ph/0301137.
Authors: A.J. Drake and K.H. Cook Commets: 13 pages, 9 figures, submitted to ApJ Celyi ryad nablyudatel'nyh faktov ukazyvaet na sushestvovanie temnyh gazovyh oblakov nebol'shogo razmera: otkrytie populyacii slabyh submillimetrovyh istochnikov, izbytok gamma-fona ot galo Galaktiki i izbytochnoe rasseyanie izlucheniya ot vnegalakticheskih radioistochnikov. Eti oblaka dolzhny proyavlyat'sya pri nablyudenii obychnyh zvezd v vide pokrytii. Dlya poiska byli vzyaty nablyudatel'nye dannye eksperimenta MACHO v kotorom dlya poiska gravitacionnogo mikrolinzirovaniya odnovremenno nablyudalos' 48 x 106 zvezd baldzha Galaktiki i Magellanovyh Oblakov. Ukazanii na sushestvovanie oblakov s poglosheniem Av > 0.2 i massami v intervale 10-4-10-2 Mo obnaruzheno ne bylo.
Authors: Mairi Sakellariadou Commets: Invited lectures in the NATO ASI / COSLAB (ESF) School `Patterns of symmetry breaking'', September 2002 (Cracow). 28 pages Sovremennye nablyudeniya isklyuchayut vozmozhnost' dominirovaniya topologicheskih defektov (kosmicheskih strun) v ob'yasnenii ryada problem kosmologii. Odnako, teriya razvita, a zakryt' effekt na 100 procentov trudno. Avtor (posle horoshego vvedeniya) rassuzhdaet, gde eshe v kosmologii mozhno primenit' kosmicheskie struny tak, chtoby eto ne protivorechilo sovremennym nablyudatel'nym dannym.
Authors: Alfredo B. Henriques and Luis E. Mendes Commets: 8 pages My horosho znaem fermionnye zvezdy - k nim otnosyatsya belye karliki, neitronnye i, poka gipoteticheskie, kvarkovye zvezdy. Bolee dvadcati let nazad byla razrabotana teoriya bozonnyh zvezd - sostoyashih iz tak i ne otkrytyh do segodnyashnego dnya skalyarnyh chastic. No okazyvaetsya est' i smeshannye bozonno-fermionnye konstrukcii, kotorye nastol'ko gibki, chto pozvolyayut s pomosh'yu odnoi modeli ob'yasnit' ogromny ryad yavlenii - ot ob'ektov s atomnymi razmerami i massoi 1018 g, do ob'ektov s galakticheskimi massami, v kotoryh nebol'shoe yadro okruzheno protyazhennoi obolochkoi. Na segodnya eta model' - skoree igra uma, no vdrug zavtra kto-to Obnaruzhit takuyu zvezdu (ili galaktiku:?)
Authors: M. Zannoni et al. Commets: 12 pages, 10 figures, Astronomical Telescopes and Instrumentation (Polaimetry in Astronomy) Hawaii August 2002 SPIE Meeting Opisan eksperiment BaR-SPOrt. Pro SPOrt my uzhe rasskazyvali. Eto ital'yansko-rossiiskii proekt dlya MKS po issledovaniyu reliktovogo izlucheniya. BaR-SPOrt - eto balonnyi eksperiment, na kotorom ustanovlena analogichnaya apparatura.
Stat'ya korotkaya, no pri etom dovol'no tehnicheskaya.
Kogda sobirayutsya puskat' "sharik" neponyatno.
Odnako, priyatno, chto delo dvizhetsya.
Author: David Langlois (GReCO/IAP, Paris) Commets: 8 pages; Review talk in the XXXVIIth Rencontres de Moriond, "The Cosmological Model", Les Arcs, France, March 2002 Kosmologiya vo Vselennoi-na-Brane (Cosmology in a brane-universe) Author: David Langlois (GReCO/IAP, Paris) Commets: 12 pages; Invited review talk at the JENAM 2002 workshop on "The cosmology of extra dimensions and varying fundamental constants", Porto, Portugal, September 2002 Dve pohozhie obzornye zametki molodogo (i ochen' citiruemogo) francuzskogo teoretika o roli "lishnih" izmerenii v sovremennoi kosmologii. Nesmotrya na kratkost' i obzornyi harakter stat'i ne yavlyayutsya legkimi dlya chteniya (dlya nespecialista kosmologa ili fizika-teoretika). Avtor rassmatrivaet kosmologicheskii scenarii dlya Vselennoi na brane v 5-mernom prostranstve i pokazyvaet kakie osobennosti pri etom voznikayut. Otmetim otsutstvie (naskol'ko nam izvestno) horoshego populyarnogo izlozheniya brannoi kosmologii na russkom yazyke (est' tol'ko dovol'no slozhnaya stat'ya Rubakova v UFN).
Authors: Joshua S. Bloom Commets: Ph.D. thesis, Caltech. 196(!) pages including low-resolution figures. Zhalko, chto u nas net nekoego edinogo saita, kuda mozhno bylo by vykladyvat' dissertacii. Nespecialistam budet interesno pochitat' vvedeniya k kazhdoi glave. Krome togo, na moi vzglyad, v dissertacii sobrana horoshaya bibliografiya. Tak kak eto dissertaciya i avtor ne byl ogranichen ob'emom, mnogie voprosy v nei rassmotreny ochen' podrobno. Vyvody dissertanta takovy:
Vryad li vy naidete v etom manuskripte chto-to radikal'no novoe, no Koe-chto interesnoe v nem nesomnenno est'.
Dlya ekonomii mesta v dissertacii privedeny risunki nizkogo razresheniya.
Vysokokachestvennyi PDF-fail dissertacii mozhno vzyat' po adresu:
Authors: J.-P. Eckmann et al. Fraktal'naya razmernost' D, vychislennaya dlya vidimogo mnozhestva galaktik daet D~2. Etot rezul'tat vnov' podnimaet diskussiyu o protivorechii dannogo fakta s modelyami, osnovannymi na predpolozhenii ob odnorodnosti Vselennoi. Odnako, po-vidimomu, etot rezul'tat ne protivorechit tomu, chto deistvitel'noe znachenie D mozhet lezhat' mezhdu 2 i 3. Na prostoi fraktal'noi modeli pokazano, kak mozhno uluchshit' ocenku D, chtoby razreshit' dannyi vopros.
Authors: H. J. de Vega, N. Sanchez Commets: LaTex, 15 pages, 2 .ps figures. Based on lectures at the Fourth International Workshop on ew Worlds in Astroparticle Physics' in Faro, Portugal and at the SOWG EUSO meeting, Roma, Italia Top-down eto kogda kosmicheskie luchi sverhvysokih energii ob'yasnyayut ne s pomosh'yu kakogo-to mehanizma uskoreniya (v aktivnyh yadrah galaktik, pri sliyaniyah neitronnyh zvezd, pri gamma-vspleskah i t.p. - eto kak raz Bottom-up), a s pomosh'yu raspada ekzoticheskih elementarnyh chastic. Avtory sravnivayut dva podhoda i golosuyut za Bottom-up.
Authors: Guenther Hasinger Commets: 13 pages, 6 figures, review to appear in "High Energy Processes and Phenomena in Astrophysics, IAU Symposium 214, X. Li, Z. Wang, V. Trimble (eds) Rech' idet o nablyudeniyah dalekih vnegalakticheskih ob'ektov (vnosyashih osnovnoi vklad v rentgenovskii fon) i mezhgalakticheskoi plazmy na novyh rentgenovskih observatoriyah. Teplyi i goryachii mezhgalakticheskii gaz v skopleniyah galaktik, parametry veshestva v centrah galaktik i ih skoplenii, linzirovannye rentgenovskie izobrazheniya, spektry i himicheskih sostav kvazarov, zhestkii fon, kotoryi bolee vsego pohozh na izluchenie nerazreshennyh akkreciruyushih chernyh dyr i koe-chto eshe, i vse eto na vsego lish' na 13 stranicah. Krome opisaniya novyh rezul'tatov (i togo, pochemu oni vazhny i interesny) avtor daet kratkie opisaniya kazhdogo sputnika.
Authors: M. Konacki et al. Commets: 8 pages, 2 figures, to appear in Nature on 30 January 2003 Zamet'te, stat'ya idet v Nature. Otkryta planeta s massoi primerno kak u Yupitera na ochen' nebol'shom rasstoyanii ot svoei zvezdy. Eto rekordno goryachaya planeta (estestvenno rech' idet ob ocenke, a ne ob izmerenii temperatury) - 1900K! Otkrytie takogo ob'ekta yavlyaetsya ser'eznym vyzovom dlya terii obrazovaniya planet.
Authors: Brad K. Gibson Commets: 2 pages, Summary of a Talk Presented at the 2001 Harley Wood Winter School, June 2001, Lorne, Victoria, Australia Journal-ref: Astron. Soc. Aus. Newsletter 26 (2002) 4 Est' takoi poleznyi (dlya nekotoryh) sait AAS Job register (hotya, naprimer, mne poziciya nashlas' drugim sposobom - ital'yancy redko vystavlyayut na etot sait informaciyu o svoih poziciyah). Za god tam poyavilos' okolo 300 ob'yavlenii o novyh postdok poziciyah. Avtor daet nekotoryi obzor etogo rynka. Interesno tem, dlya kogo aktual'no :).
Authors: P. Haensel Commets: 35 pages, 11 figures, uses eas.cls, to be published in `Final Stages of Stellar Evolution'', edts. J.-M. Hameury and C. Motch, EAS Publications Series (EDP Sciences, 2003) Teoretikov mnogo, a priroda odna.... Uravnenie sostoyaniya dolzhno byt' edinstvennym, no poka net dostatochno detal'nyh nablyudatel'nyh dannyh. A potomu sushestvuet mnozhestvo modelei, o kotoryh i rasskazyvaetsya v stat'e.
Authors: Renata Kallosh, Andrei Linde Commets: 7pages, 6 figs Esli znak potnosti temnoi energii (Lyambda-chlena) polozhitelen, to Vselennaya rasshiryaetsya s uskoreniem. Esli on obrashaetsya v nol' - to my vozvrashaemsya k klassicheskim Fridmanovskim modelyam. A vot esli on stanovitsya otricatel'nym, to Vselennaya kollapisruet i etot process dlitsya vremya sravnimoe s ee vozrastom. Otricatel'naya plotnost' temnoi energii tipichna dlya ryada teorii, osnovannyh na supergravitacii. V dannoi stat'e Renata Kallosh i ee suprug Andrei Linde pokazyvayut, chto smena znaka plotnosti temnoi energii na otricatel'nyi - gorazdo bolee obshee yavlenie. Pri etom po sovremennomu hodu rasshireniya Vselennoi prakticheski nevozmozhno opredelit' smenitsya li ono bystrym kollapsom ili net. Neskol'ko primerov razlichnogo hoda rasshireniya pokazany na grafike.
Authors: Lucio Mayer et al. Commets: 13 pages, 2 Figures. Text and artwork are slightly different from the version published on Science. More hi-res picture and movies can be found at http://www.astro.washington.edu/mayer Journal-ref: Science, 2002, 298, 1756 My ploho znaem, kak obrazuyutsya planety. Modelirovanie etogo processa yavlyaetsya ochen' slozhnoi zadachei. V stat'e predstavleny rezul'taty nedavnih raschetov, odnih iz samyh detal'nyh na segodnyashnii den'. "Mnogoe sdelano, no mnogoe eshe predstoit". Sm. takzhe stat'yu "Three-dimensional Calculations of High and Low-mass Planets Embedded in Protoplanetary Discs" astro-ph/0301089.
Authors: S. Pustilnik, A.Kniazev, A. Pramskij, A. Ugryumov Commets: 4 pages, 3 figures. To appear in the proceedings of Euroconference "The evolution of galaxies. III. From simple approaches to self-consistent models" Kiel, Germany, July 2002 Rossiiskie nablyudateli dayut korotkii obzor issledovanii (v osnovnom sobstvennyh) galaktik s ekstremal'no nizkim soderzhaniem metallov.
Authors: F.P. Gavriil, V.M. Kaspi, P.M. Woods Commets: 10 pages, 7 figures, to appear in the proceedings of the 34th Cospar Scientific Assembly Avtory dayut obzor svoih nablyudenii i obrabotki arhivnyh dannyh po anomal'nym rentgenovskim pul'saram. Osoboe vnimanie udeleno povedeniyu proizvodnoi perioda na bol'shih vremennyh otrezkah, a takzhe vspyshkam v rentgenovskom diapazone (kotorye rodnyat ARP s MPG).
Authors: Mordecai-Mark Mac Low, Ralf S. Klessen Commets: Invited review for "Reviews of Modern Physics", 86 pages, 33 figures. This is the first draft. Comments and suggestions are very welcome, please contact mordecai@amnh.org or rklessen@aip.de Klassicheskoe (Dzhinsovskoe) uslovie nachala kollapsa protozvezdnogo oblaka vyvoditsya iz balansa energii. No sreda iz kotoroi obrazuyutsya zvezdy ochen' sil'no turbulizovana. I avtory predlagayut "novuyu paradigmu" soprovozhdaya ee etoi knigoi. Rabota mne kazhetsya ochen' interesnoi i poleznoi, no ona, bezuslovno, prednaznachena dlya specialistov - astronomov, fizikov, gidrodinamikov.
Authors: Michael Feast Commets: 26 pages, no figs, to appear in "Stellar Candles for the Extragalactic Distance Scale" Lecture Notes in Physics (Springer) ed. D. Alloin and W. Gieren Avtor podrobno rassmatrivaet metodiku nalibrovki svetimosti cefeid v nashei Galaktike i ucheta ih mezhzvezdnogo pokrasneniya. Eti izmereniya, sovmestno s izmereniyami cefeid v galaktike NGC4258 pokazyvayut, chto tochnost' etoi kalibrovki ne huzhe 0.1m, po krainei mere dlya cefeid s solnechnym himsostavom. Razlichie v himicheskom sostave vnosit primerno takuyu zhe oshibku. Dlya togo, chtoby uvelichit' tochnost' predskazanniya svetimosti cefeid neobhodimy obshirnye raboty po izucheniyu ih metallichnosti, uchet nelineinosti v zavisimostyah period-svetimost' i period-cvet, a takzhe tochnoe opredelenie v kakoi mode proishodyat ih pul'sacii - na osnovnoi chastote ili na pervom obertone.
Authors: C. Motch, O. Herent, P. Guillout Commets: Proceedings of the "X-ray surveys, in the light of the new observatories" workshop, Astronomische Nachrichten, in the press (4 pages, 3 figures, uses an.cls) Apparatura sputnika XMM-Newton ochen' chuvstvitel'na, chto pozvolyaet videt' slabye istochniki. Eto oznachaet, kak nablyudeniya dalekih vnegalakticheskih ob'ektov, tak i issledovaniya blizkih slabyh istochnikov - zvezd, akkreciruyushih dvoinyh v "vyklyuchennom" sostoyanii i t.d. Dlya issledovanii vnegalakticheskih istochnikov obychno vybirayut napravleniya vdali ot ploskosti Galaktiki. Svyazano eto s "perenaselennost'yu" izobrazhenii, sdelannyh v +/- 20 gradusah ot galakticheskogo ekvatora (krome togo, mozhet byt' vazhno pogloshenie). Razobrat'sya v meshanine mnozhestva slabyh istochnikov ochen' trudno, no mozhno. Imenno ob etom rasskazyvayut avtory v svoei korotkoi zametke. Oni opisyvayut popytku opticheskogo otozhdestvleniya galakticheskih istochnikov XMM-Newton. V osnovnom obnaruzheny aktivnye zvezdy, no est' i drugie ob'ekty.
Authors: Massimo Turatto Commets: 16 Pages, 4 figures, to be published in "Supernovae and Gamma-Ray Bursters," ed. Kurt W. Weiler
Opisyvaetsya sovremennaya klassifikaciya sverhnovyh.
Vo mnogom stat'ya pereklikaetsya s
astro-ph/0301006,
potomu luchshe chitat' ih vmeste (vozmozhno takzhe budet interesno posmotret'
nedavnii obzor po mehanizmam vzryvov massivnyh zvezd
astro-ph/0212314 i sverhnovyh tipa Ia
astro-ph/0212530).
Dolgoe vremya imenno nablyudeniya kompaktnyh dvoinyh nashei Galaktiki sostavlyali nablyudatel'nuyu osnovu teorii akkrecii. Eshe sovsem nedavno (neskol'ko let nazad) akkreciya v takih sistemah schitalas' stacionarnoi, a izluchenie ot takih sistem - izotropnym (v pervom priblizhenii). Segodnya my vidim, chto bol'shinstvo rentgenovskih sistem - tranzienty, akkreciruyushee na nih veshestvo vybrasyvaetsya vetrom ili dzhetami, izluchenie ispuskaetsya rezko anizotropno, v diskah sushestvenny proyavleniya razlichnyh neustoichivostei. Krome togo, v sosednih galaktikah obnaruzheny rentgenovskie istochniki, kotoryh prosto net v Mlechnom Puti (v pervuyu ochered' - ultraluminous sources). Pohozhe, chto i zdes' menyaetsya paradigma. Rekomenduyu prochitat' vsem. No chtenie ne budet legkim, hotya v obzore pochti net formul.
Authors: Andrew S. Wilson Commets: 6 pages, To be published in the proceedings of the Bologna conference `The Physics of Relativistic Jets in the Chandra and XMM Era'', New Astronomy Review Obzor fizicheskih processov, otvetstvennyh za rentgenovskoe izluchenie radiodzhetov i soputstvuyushih yavlenii.
Authors: R.I. Hynes (Texas), D. Steeghs (CfA), J. Casares (IAC), P.A. Charles (Southampton), K. O'Brien (ESO) Commets: 12 pages; accepted for publication in ApJ Letters Pohozhe poyavilsya eshe odin kandidat v chernye dyry. Funkciya mass kompaktnogo ob'ekta (t.e. nizhnyaya granica ego massy) prevyshaet 2.0Mo (znachimost' 95%), a po luchshim dannym poluchennym za odin orbital'nyi oborot (okolo 1.7 dnya) -- 5.8+/-0.5Mo.
Authors: I.A.Maslov et al. Commets: submitted to Astronomical and Astrophysical Transactions, 7 pages Predlozhena sistema iz neskol'kih nebol'shih opticheskih teleskopah dlya obzora neba s cel'yu issledovaniya nebol'shih meteornyh tel i issledovaniya mezhplanetnoi sredy.
Authors: Arthur Kosowsky Commets: 11 pages, to appear in "The Emergence of Cosmic Structure," Proceedings of the 13th Annual Astrophysics Conference in Maryland, eds. S. Holt and C. Reynolds, AIP Press, 2003 Nablyudeniya reliktovogo izlucheniya uzhe seichas yavlyayutsya odnim iz vazhneishih (samym vazhnym?) istochnikom nashih kosmologicheskih znanii. A v nedalekom budushem ozhidaetsya novyi vitok progressa v etoi oblasti. Avtor rassuzhdaet ob etom nedalekom budushem i opisyvaet planiruemyi eksperiment ACT. Sm. takzhe "What can we learn on the thermal history of the Universe from future CMB spectrum measures at long wavelengths?" astro-ph/0301133.
Authors: Xiaohui Fan et al. Commets: AJ in press (Apr 2003), 26 pages, 9 figures V obshem-to vse yasno iz nazvaniya. Pri obrabotke Sloanovskogo cifrovogo obzora neba naideny eshe tri kvazara s predel'nymi krasnymi smesheniyami: J114816.64+525150.3 (z=6.43), J104845.05+463718.3 (z=6.23) i J163033.90+401209.6 (z=6.05). Za podrobnostyami - v stat'yu.
Authors: F. Halzen Commets: Latex2.09, uses crckapb.sty (included), 31 pages, 13 postscript figures placed with epsfig.sty. Talk presented at the 9th Course of Astrofundamental Physics, International School of Astrophysics D. Chalonge, Palermo, Sicily, Sept. 2002 Obzor po sovremennoi astronomii neitrino vysokih energii s sootvetstvuyushim istoricheskim vvedeniem. Mnogo vnimaniya udelyaetsya sovremennym eksperimentam - AMANDA, DUMAND, IceCube. Obzor horosho proillyustrirovan, naprimer, tak vyglyadit spektr zhestogo fona fotonov na energiyah vyshe 1 GeV.
Authors: Clifford M. Will Commets: 15 pages, 1 figure, to be submitted to the Astrophysical Journal Ochen' ostraya kriticheskaya stat'ya, opublikovannaya srazu posle press-konferencii Fomalona i Kopeikina na s'ezde Amerikanskogo Astronomicheskogo Obshestva (press konferenciya byla 7 yanvarya, a stat'ya vyshla uzhe 9-go). Avtor utverzhdaet, chto v provedennom eksperimente izmeryalas' ne skorost' rasprostraneniya gravitacii, a odin iz postn'yutonovskih parametrov, kotoryi izvesten s ochen' vysokoi tochnost'yu po ryadu eksperimentov (tipa lazernoi lokacii Luny) v Solnechnoi sisteme. Polovinu stat'i zanimayut slozhnye formuly, no vvedenie i zaklyuchenie prosto zahvatyvayushi.
Authors: M. Kramer (Manchester University, Jodrell Bank), O. Loehmer, A. Karastergiou (MPIfR Bonn) Commets: 4 pages,to appear in "Radio Pulsars" (ASP Conf. Ser.), eds. M. Bailes, D. Nice, & S. Thorsett V ochen' korotkoi stat'e sobrany sovremennye dannye po geodezicheskoi precessii neitronnoi zvezdy (precessii v iskrivlennom tyagoteniem prostranstve-vremeni) v Hals-Teilorovskom dvoinom pul'sare (eta sistema byla otkryta pervoi i nablyudaetsya dol'she vseh ostal'nyh).
Poskol'ku k sozhaleniyu nikto ne vzyalsya za obzory razdela physics,
my budem starat'sya hotya by perechislit' interesnye (dlya shirokoi publiki)
stat'i, poyavivshiesya v etoi chasti Arhiva.
Authors: Metod Saniga Commets: 10 pages, 4 figures, to appear in the proceedings of the NATO ARW "The Nature of Time: Geometry, Physics and Perception," edited by R. Buccheri, M. Saniga and W.M. Stuckey, Kluwer Academic Publishers, Dordrecht / Boston / London, 2003, pp. 131-143 Na moi vzglyad - eto otlichnyi primer nauchnoi "al'ternativy". Obratite vnimanie, chto rabota podderzhana grantami ves'ma i ves'ma ser'eznyh organizacii. Tak chto "v ocherednoi raz nepravy" te, kto polagaet, chto sredi professional'nyh uchenyh sushestvuet zagovor protiv al'ternativnyh teorii.
Mozhno sdelat' dva
zamechaniya.
Authors: Roberto Assumpcao Commets: 7 pages,4 figures Kak "na pal'cah" izlagat' teoriyu otnositel'nosti? Delo neprostoe. Napomnim, chto u nas osnovy STO vhodili v normal'nyi shkol'nyi kurs fiziki. Odnako, po svoemu opytu mogu skazat': mne bylo neponyatno, kogda uchilsya, a kogda uchil - ne do vseh smog donesti.
Authors: Iwona Mroz Commets: 17 pages, 6 figures Navernoe, mnogie chitali interesnye issledovaniya S. Kapicy po povodu dinamiki naseleniya Zemli i t.p. Esli chitali, i ponravilos', to prochtite i eto.
Authors: Blaise Aguera y Arcas, Adrienne Fairhall Commets: 18 pages, 10 figures Po nazvaniyu mozhet pokazat'sya, chto stat'ya populyarnaya, no eto ne tak. Eto original'noe issledovanie.
Authors: B.G. Sidharth Commets: 29 pages, TeX, Invited Talk at the Fifth International Symposium on "Frontiers of Fundamental Physics", January 8-11, 2003 Slozhnaya stat'ya. Mnogo matematiki. Odnako, ....
Arhiv statei, voshedshih v predydushie vypuski.
Razdely arhiva (s iyulya 2002 g.): Poleznye astronomicheskie ssylki. Obzornye stat'i v astro-ph s 2001 g. |
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