The R.A.P.Project "Prosto o slozhnom" "Astro-ph za vtoruyu polovinu 2003 g." Nemnogo statistiki Predydushii vypusk (N69) Zvezdy AstroRuneta-2003 Slovar' astroterminov Spisok missii i teleskopov Obzory UFN Stat'i SOZh ANKa Dnya 04.02.2004. Rentgenogramma serdca Galaktiki Soderzhanie i bystryi perehod k razdelam obzora Stat'i nedeli "Luchshie iz luchshih" !!! astro-ph/0402468 RXJ1242.6-1119A - proverka scenariya prilivnogo razrusheniya astro-ph/0402385 Povtornoe mikrolinzirovanie v sobytii OGLE-2003-BLG-095 astro-ph/0402418 Shirokaya liniya poglosheniya v spektre odinochnoi neitronnoi zvezdy RX J1605.3+3249 Otdel'nye stat'i Kosmicheskaya topologiya: kratkii obzor Obrazovanie dvoinyh asteroidov v poyase Koipera za schet obmennyh vzaimodeistvii Modeli zvezd galo s ekstremal'no nizkoi metallichnost'yu Regulyarnye dvizheniya v sistemah ekzoplanet Vzveshivanie kaspa v Galakticheskom centre Moglo li chto-to raspadat'sya, isparyat'sya ili annigilirovat' vo vremya pervichnogo nukleosinteza? CFL zvezdy v dvoinyh sistemah i chernye dyry Astroseismologiya zvezdy nyu Eridana, peremennoi tipa beta Cefeya: interpretaciya i prilozhenie k spektru oscillyacii Astrofizicheskoe proishozhdenie kosmicheskih luchei sverhvysokih energii Kvantovaya pena O sootnoshenii mezhdu massami central'noi chernoi dyry i baldzha galaktiki Povtornoe mikrolinzirovanie v sobytii OGLE-2003-BLG-095: mikrolinzirovanie dvoinogo istochnika Evolyuciya magnitnogo polya v kore neitronnyh zvezd pod deistviem effekta Holla i omicheskogo zatuhaniya Dekonfaiment kvarkov i ego vliyanie na radiusy i predel'nye massy kompaktnyh zvezd Sil'naya shirokaya liniya poglosheniya v rentgenovskom spektre blizkoi odinochnoi neitronnoi zvezdy RX J1605.3+3249 Sil'noe padenie rentgenovskoi svetimosti neaktivnoi galaktiki RXJ1242.6-1119A i pervyi spektr posle vspyshki - proverka scenariya prilivnogo razrusheniya Sil'noe vzaimodeistvie mezhdu neitrino i nuklonami sverhvysokih energii kak reshenie zagadki GZK-obrezaniya Chernye dyry v teorii s protyazhennymi dopolnitel'nymi izmereniyami: obzor Iz razdela physics Mnogomernost' izmerenii Polnyi Arhiv predydushih vypuskov. Arhiv statei, voshedshih v vypuski s 01 iyulya 2002 g. po 31 marta 2003 g. Razdely arhiva (s aprelya 2003 g.): kosmologiya, neitrino, kosmicheskie luchi i gamma-astronomiya, galaktiki, AYaG, kvazary, nasha Galaktika, mezhzvezdnaya sreda, zvezdy, sverhnovye, ostatki sverhnovyh, chernye dyry, neitronnye zvezdy, linzirovanie, Solnce, ekzoplanety, Solnechnaya sistema, akkreciya, tesnye dvoinye sistemy, gamma-vspleski, gravitacionnye volny, mehanizmy izlucheniya, chislennoe modelirovanie, dinamika, mehanika metody obrabotki dannyh, MGD, metody nablyudenii, budushie nablyudatel'nye proekty, prochee. Poleznye astronomicheskie ssylki. Korotkoe esse ob elektronnyh preprintah. Obzornye stat'i v astro-ph s 2001 g. Obsudit' na forume Scientific.RU Obsudit' na forume Zvezdocheta Avtory proekta Sergei Popov Mihail Prohorov Postav'te u sebya nashu knopku! Proekt razmeshen na saitah: Vy mozhet takzhe razmestit' na svoem saite nashu lentu obzorov Novostnye lenty Novosti astronomii ot PRAO Tekushie otkrytiya v FECh Novosti kosmonavtiki Novosti ot UFN Informnauka Perst Podpiska na rassylku obzorov na Subscribe.Ru Druzhestvennaya rassylka "Okno vo Vselennuyu" Sozdavaemyi katalog on-lainovoi nauchnoi literatury

Obzory preprintov astro-ph Vypusk N70 astro-ph za 16 - 22 fevralya 2004 goda: izbrannye stat'i Referaty otdel'nyh statei miniobzor astro-ph/0402324 Kosmicheskaya topologiya: kratkii obzor (Cosmic Topology: a Brief Overview) Authors: M.J. Reboucas, G.I. Gomero Comments: Revtex4, 9 pages, 2 figures. Ivited talk delivered at "XIV National Meeting of the Brazilian Physical Society, section Particles and Fields, Caxambu - MG, Brazil, from September 30 to October 04, 2003 Vopros o topologii Vselennoi vsegda byl populyaren. V poslednee vremya nekotoraya aktivnost' nablyudalas' v svyazi s dannymi sputnika WMAP, a osobenno v svyazi s rabotoi Lyumine i dr. V etoi stat'e avtory dayut kratkii obzor problematiki i osnovnyh rezul'tatov. V kachestve bolee populyarnogo izlozheniya mozhno prochest' stat'yu na Astronete. astro-ph/0402328 Obrazovanie dvoinyh asteroidov v poyase Koipera za schet obmennyh vzaimodeistvii (The formation of Kuiper-belt Binaries through Exchange Reactions) Authors: Yoko Funato et al. Comments: 12pages, 4 figures Neskol'ko procentov ob'ektov v poyase Koipera yavlyayutsya dvoinymi. Oni obladayut sleduyushimi svoistvami: massy kompan'onov dvoinoi primerno ravny, orbity dvoinyh sil'no ekscentrichny, orbity shirokie (v 100 i bolee raz prevoshodyat radius kompan'onov). Sushestvuyut problemy s ob'yasneniem etih svoistv, poskol'ku pri neposredstvennom obrazovanii dvoinyh asteroidov dolzhny byli voznikat' gorazdo bolee tesnye sistemy s pochti krugovymi orbitami. Avtory predlagayut svoyu model', v kotoroi dvoinye formiruyutsya na rannei stadii rosta transneptunovyh ob'ektov za schet gravitacionnoi neustoichivosti v pylevom protoplanetnom sloe. astro-ph/0402334 Modeli zvezd galo s ekstremal'no nizkoi metallichnost'yu (Models for extremely metal-poor halo stars) Authors: A. Weiss et al. Comments: submitted to Astron. Astrophys., 9 pages, 3 figures V galo nashei Galaktiki nablyudayutsya zvezdy s ochen' malym soderzhaniem elementov tyazhelee geliya. V etih ob'ektah nablyudaetsya nekotoroe kolichestvo ugleroda i azota, chto neobhodimo kak-to ob'yasnyat'. Sushestvuyut dve modeli. V pervoi iz nih zvezdy formiruyutsya "chistymi", a uglerod i azot narabatyvabtsya vo vremya gelievyh vspyshek v yadre. Vo vtoroi, nekotoroe kolichestvo tyazhelyh elementov iznachal'no vhodit v sostav zvezdy iz-za togo, chto protozvezdnoe veshestvo bylo obogasheno vzryvom blizkoi sverhnovoi. Avtory detal'no modeliruyut evolyuciyu zvezdy HE0107-5240 i prihodyat k vyvodu, chto vtoraya model' luchshe opisyvaet nablyudeniya. obzor astro-ph/0402335 Regulyarnye dvizheniya v sistemah ekzoplanet (Regular Motions in Extra-Solar Planetary Systems) Authors: S. Ferraz-Mello et al. Comments: 25 pages, 11 figures, to be published in "Chaotic Worlds: From Order to Disorder in Gravitational N-Body Systems" (B.A.Steves, ed.), Kluwer Acad. Publ. Eto obzor po dinamike planetnyh sistem v primenenii k ekzoplanetam. Stat'ya dostatochno tehnicheskaya, no vmeste s tem dostupnaya kazhdomu, kto pomnit standartnyi universitetskii (institutskii) kurs po teormehu. astro-ph/0402338 Vzveshivanie kaspa v Galakticheskom centre (Weighing the cusp at the Galactic Centre) Authors: N. Mouawad et al. Comments: 11 pages, 5 figures submitted to astron. and astroph Kak izvestno, v centre nashei Galaktiki nahoditsya chernaya dyra. Ee massa neploho izvestna: okolo 3-4 millionov mass Solnca. Eto bylo opredeleno po izmereniyam orbital'nogo dvizheniya zvezd v neposredstvennoi blizosti ot centra Galaktiki. Odnako chernaya dyra okruzhena nebol'shim zvezdnym skopleniem s bystro rastushei k centru plotnost'yu - kaspom. Massa kaspa namnogo men'she massy chernoi dyry, no vse ravno, on mozhet okazyvat' nebol'shoe vliyanie na dinamiku zvezdnyh orbit. Avtory detal'no issleduyut etot vopros. Osnovnoi vyvod sostoit v tom, chto massa kaspa sostavlyaet primerno 10 procentov ot massy chernoi dyry. Krome togo, oni obsuzhdayut prirodu ob'ektov, formiruyushih kasp. V chastnosti, po vsei vidimosti tam velika dolya "zvezdnyh ostatkov" - belyh karlikov, neitronnyh zvezd i chernyh dyr. astro-ph/0402344 Moglo li chto-to raspadat'sya, isparyat'sya ili annigilirovat' vo vremya pervichnogo nukleosinteza? (Did Something Decay, Evaporate, or Annihilate during Big Bang Nucleosynthesis?) Authors: Karsten Jedamzik Comments: 7 pages, 3 figures Processy tipa raspada adronov, ispareniya ili annigilyacii reliktov predydushih epoh (mikroskopicheskih pervichnyh chernyh dyr ili tyazhelyh chastic) proishodyashie vo vremya pervichnogo nukleosinteza mogut sushestvenno povliyat' na ego rezul'taty, v chastnosti na kolichestvo obrazuyushihsya izotopov litiya (6Li i 7Li). Detal'nomu rassmotreniyu takogo vliyaniya (na osnove chislennogo modelirovaniya processov sinteza) i posvyashena dannaya stat'ya. astro-ph/0402349 CFL zvezdy v dvoinyh sistemah: "pryachutsya" li oni sredi kandidatov v chernye dyry? (Self-bound CFL stars in binary systems : are they "hidden" among the black hole candidates?) Authors: J. E. Horvath, G. Lugones Comments: 4 pages, 3 figures My neodnokratno obrashali vashe vnimanie na raboty, posvyashennye probleme "identifikacii" chernyh dyr (Narayan et al.; Abramowicz et al.). Osobo hochetsya vydelit' nedavnyuyu stat'yu Ye-Fei Yuan et al.. Problema v obnaruzhenii neposredstvennogo proyavleniya gorizonta. Narayan et al. polagayut, chto lyuboi kompaktnyi ob'ekt s massoi bolee 3 mass solnca i bez rentgenovskih vspleskov pervogo tipa (oni svyazany s zagoraniem "termoyadernogo topliva" na poverhnosti) yavlyaetsya ochen' sil'nym kandidatom v chernye dyry. Horvat i Lugones v svoei stat'e rassmatrivayut nekotoruyu ekzoticheskuyu al'ternativu - CFL zvezdy (CFL=color flavor locked). CFL zvezdy eto podvid togo, chto inogda ob'edinyayut obshim terminom "neitronnye zvezdy". Na samom dele v zavisimosti ot uravneniya sostoyaniya sostav kompaktnogo ob'ekta mozhet byt' sovsem ne "neitronnym". V chastnosti, mogut sushestvovat' kvarkovye zvezdy raznyh tipov. CFL zvezdy - odin iz nih. Eti ob'ekty otlichayutsya dovol'no bol'shimi maksimal'nymi massami i otsutstviem normal'noi poverhnosti. T.o. po mneniyu avotrov oni mogut pryatat'sya sredi kandidatov v chernye dyry "po Narayanu". Stat'ya korotkaya i ponyatnaya. Tak chto v nei legko razobrat'sya. astro-ph/0402354 Astroseismologiya zvezdy nyu Eridana, peremennoi tipa beta Cefeya: interpretaciya i prilozhenie k spektru oscillyacii (Asteroseismology of the Beta Cephei star Nu Eridani: Interpretation and applications of the oscillation spectrum) Authors: A. A. Pamyatnykh et al. Comments: 8 pages, 7 figures, accepted in MNRAS Posle togo, kak osnovnye teoreticheskie problemy gelioseismologii byli uspeshno resheny, metody nablyudenii razrabotany i oprobovany, i finansirovanie dannogo napravleniya issledovanii sokratilos', chast' issledovatelei obnaruzhili, chto vse eti metody mozhno primenyat' i k naibolee yarkim zvezdam. Tak voznikla astroseismologiya. U zvezdy ν Eri, yavlyayusheisya peremennoi tipa β Cephei, nablyudaetsya samyi bogatyi spektr kolebanii. Spektr interpretiruetsya v terminah normal'nyh mod kolebanii zvezdy. Dannye o tom, kakie iz vozmozhnyh mod kolebanii vozbuzhdeny, a kakie net, pozvolyayut postroit' "seismicheskuyu" model' etoi zvezdy. Nablyudayusheesya rassheplenie dipol'nyh mod pozvolyaet sdelat' zaklyuchenie o skorosti vrasheniya yadra zvezdy. obzor astro-ph/0402371 Astrofizicheskoe proishozhdenie kosmicheskih luchei sverhvysokih energii (Astrophysical Origins of Ultrahigh Energy Cosmic Rays) Authors: Diego F. Torres, Luis A. Anchordoqui Comments: 94 pages revtex, 9 .eps figures (higher resolution version of Fig. 7 is available at http://www.angelfire.com/id/dtorres/down3.html). Solicited review article prepared for Reports on Progress in Physics Bol'shoi obzor po kosmicheskim lucham sverhvysokih energii i po astrofizicheskim modelyam dlya ih istochnikov. Otmetim takzhe obzor, posvyashennyi modelyam t.n. "kolena" v spektre kosmicheskih luchei: Models of the Knee in the Energy Spectrum of Cosmic Rays. gr-qc/0401015 Kvantovaya pena (Quantum Foam) Authors: Y. Jack Ng Comments: 20 pages, 3 figures, talk given at the 10th Marcel Grossman Meeting (Rio de Janeiro, July 20 - 26, 2003) Avtor rassuzhdaet o svoistvah kvantovoi peny i vozmozhnosti zaregistrirovat' ee nalichie. astro-ph/0402376 O sootnoshenii mezhdu massami central'noi chernoi dyry i baldzha galaktiki (On the Black Hole Mass - Bulge Mass Relation) Authors: Nadine Haering and Hans-Walter Rix Comments: 11 pages, 3 figures, accepted in ApJ Letters Proizvedena ocherednaya pereproverka ukazannoi zavisimosti. Avtory nashli, chto zavisimost' pochti lineinaya Mbh ~ Mbulge1.12+/-0.06 Dlya baldzha s massoi Mbulge~5x1010 Mo srednyaya massa central'noi chernoi dyry sostavlyaet 0.14% +/- 0.04% ot massy baldzha. astro-ph/0402385 Povtornoe mikrolinzirovanie v sobytii OGLE-2003-BLG-095: mikrolinzirovanie dvoinogo istochnika (The repeating microlensing event OGLE-2003-BLG-095: A plausible case for microlensing of a binary source) Authors: Matthew J. Collinge (Princeton) Comments: 16 pages, 4 figures, 2 tables Kogda (s podachi Bogdana Pachin'skogo) byli nachaty pervye poiski gravitacionnogo mikrolinzirovaniya, eti sobytiya harakterizovalis' sleduyushim obrazom: monohromaticheskoe - krivaya bleska ne zavisit ot dliny volny sveta; simmetrichnaya kolokoloobraznaya krivaya bleska (dlya nee est' tochnaya formula); odnorazovost' - sobytie ne povtoryaetsya (v tom zhe meste na nebesnoi sfere). Pozzhe, kogda bol'shoe kolichestvo klassicheskih sobytii, udovletvoryayushih trem perechislennym kriteriyam, bylo uzhe obnaruzheno, nachali iskat' situacii, v kotoryh nekotorye iz etih uslovii mogli by narushat'sya. Monohromatichnost' krivoi bleska mozhet narushat'sya iz-za vliyaniya effekta potemneniya diska zvezdy k krayu ili iz-za togo, chto chast' sveta daet linza. Narushenie formy krivoi bleska mozhet byt' vyzvano dvoistvennost'yu linzy. Obychno v etom sluchae krivye bleska poluchayutsya ochen' slozhnymi iz-za peresecheniya kaustik. Drugaya prichina - vliyanie parallaksa - ona proyavlyaetsya tol'ko dlya samyh blizkih linz i v samyh dolgih (poryadka goda) sobytiyah mikrolinzirovaniya. Konechnyi parallaks linzy delaet krivuyu bleska slegka nesimmetrichnoi. Nenarushennym ostavalos' tol'ko poslednee pravilo - sobytiya ne povtoryalis'. Ono narushilos' v sobytii OGLE-2003-BLG-095. Krivaya bleska sobytiya OGLE-2003-BLG-095 V etom sobytie chetko vidny dva simmetrichnyh pika, razdelennyh intervalom primerno v 100 dnei. Vozmozhny dve interpretacii podobnogo sobytiya: eto linzirovanie dvoinoi zvezdy; zvezdy odinochnaya, no linza - shirokaya dvoinaya. Obe modeli horosho opisyvayut nablyudeniya - zelenaya i krasnaya krivye na risunke. Razlichit' ih, po-vidimomu, ne udastsya iz-za nebol'shoi sobstvennoi peremennosti linzirovannoi zvezdy. Eshe odnoi neobychnoi mikrolinze OGLE-2002-BLG-055 posvyashena stat'ya astro-ph/0402417. V etom klassicheskoi po svoistvam sobytii odna tochka ochen' sushestvenno, na 0.6 zvezdnoi velichiny, podskochila vverh. Krivaya bleska sobytiya OGLE-2002-BLG-055 Zdes' tozhe vozmozhny dve interpretacii: dvoinaya linza u kotoroi vtoroi komponent - planeta ili dvoinaya zvezda-istochnik slabyi komponent kotoroi okazalsya gorazdo blizhe k luchu zreniya, chem yarkii. astro-ph/0402392 Evolyuciya magnitnogo polya v kore neitronnyh zvezd pod deistviem effekta Holla i omicheskogo zatuhaniya (Magnetic Field Evolution in Neutron Star Crusts due to the Hall Effect and Ohmic Decay) Authors: Andrew Cumming et al. Comments: 18 pages, 13 figures, Submitted to ApJ Eshe odna stat'ya pro evolyuciyu magnitnogo polya u neitronnyh zvezd. Ee osobennost' - uchet effekta Holla (naryadu s drugimi effektami). Privedeny rezul'taty chislennogo modelirovaniya, pokazany vozmozhnye konfiguracii polei. [Effekt Holla zaklyuchaetsya v vozniknovenii v provodnike s tokom I, pomeshennom v magnitnoe pole B, elektricheskogo polya v napravlenii, perpendikulyarnom k I i B. Svyazan s otkloneniem dvizhushihsya v provodnike elektronov silami Lorenca.] obzor astro-ph/0402404 Dekonfaiment kvarkov i ego vliyanie na radiusy i predel'nye massy kompaktnyh zvezd (Quark deconfinement and implications for the radius and the limiting mass of compact stars) Authors: Ignazio Bombaci et al Comments: 34 pages, 10 figures Avtory yavlyayutsya storonnikami shiroko rasprostranennoi segodnya gipotezy, chto v kompaktnyh (neitronnyh) zvezdah vozmozhen perehod ot nuklonnogo veshestva k kvarkovoi plazme, no v otlichie ot bol'shinstva issledovatelei oni priderzhivayutsya mneniya, chto takoi perehod budet proishodit' postepenno i zvezda mozhet nadolgo zaderzhat'sya v metastabil'nom "gibridnom" perehodnom sostoyanii. Avtory podrobno rassmatrivayut svoi variant teorii, razlichnye ego sledstviya i, v chastnosti, ee prilozhenie k "zaderzhannym" gamma-vspleskam, kotorye proishodyat cherez nekotoroe vremya posle kollapsa massivnoi zvezdy. !!! astro-ph/0402418 Sil'naya shirokaya liniya poglosheniya v rentgenovskom spektre blizkoi odinochnoi neitronnoi zvezdy RX J1605.3+3249 (A Strong, Broad Absorption Feature in the X-ray Spectrum of the Nearby Neutron Star RX J1605.3+3249) Authors: M. H. van Kerkwijk et al. Comments: 30 pages, 7 figures, accepted in ApJ Nablyudeniya observatorii XMM-N'yuton pokazali, chto v spektre tret'ei po yarkosti odinochnoi neitronnoi zvezdy nablyudaetsya shirokaya i moshnaya absorbcionnaya osobennost' (proshe govorya, liniya poglosheniya). Centr etoi linii prihoditsya na Dlinu volny 27 angstrem ili na energiyu 0.45 keV. V stat'e podrobno opisana metodika provedeniya i obrabotki nablyudenii, no osnovnoe mozhno pocherpnut' iz privedennogo nizhe risunka. Srektr ob'ekta RX J1605.3+3249, sploshnoi i punktirnoi liniyami pokazany kontinuumy dvuh naibolee udachnyh ego approksimacii (bez ucheta linii poglosheniya). Avtory prihodyat k zaklyucheniyu, chto eto protonnaya ciklotronnaya liniya, oslablennaya kvantovymi vakuumnymi effektami. V etom sluchae magnitnoe pole na poverhnosti dolzhno bylo by sostavlyat' 7x1013 Gs (bez ucheta gravitacionnogo pokrasneniya). astro-ph/0402468 Sil'noe padenie rentgenovskoi svetimosti neaktivnoi galaktiki RXJ1242.6-1119A i pervyi spektr posle vspyshki - proverka scenariya prilivnogo razrusheniya (A Huge Drop in X-ray Luminosity of the Non-Active Galaxy RXJ1242.6-1119A, and First Post-Flare Spectrum - Testing the Tidal Disruption Scenario) Authors: S. Komossa et al. Comments: 11 pages, to appear in March 1 issue of ApJ Letters (submitted Nov. 10, accepted in Dec. 2003); background information available at http://www.xray.mpe.mpg.de/~skomossa/ Eto original raboty, vyzvavshei nebyvalyi rezonans (vozmozhno ne sovsem opravdano). Populyarnoe izlozhenie luchshe vsego posmotret' na Astronete. Krome togo otmetim stat'i Pashi Ivanova i soavtorov, posvyashennyh modelirovaniyu takih sliyanii. Ssylki na stat'i mozhno naiti zdes'. hep-ph/0402102 Sil'noe vzaimodeistvie mezhdu neitrino i nuklonami sverhvysokih energii kak reshenie zagadki GZK-obrezaniya Authors: Z. Fodor, S.D. Katz, A. Ringwald, H. Tu Comments: 20 pages, 12 figure Soglasno sovremennym teoreticheskim predstavleniyam fotony s energiyami vyshe 4x1019 erg ne mogut preodolevat' kosmologicheskie rasstoyaniya iz-za vzaimodeistviya s myagkimi fotonami reliktovogo izlucheniya, i v spektre kosmicheskih luchei vyshe etoi energii dolzhen nablyudat'sya zaval (kotoryi nosit imena Greisena-Zacepina-Kuz'mina). Pohozhe, odnako, chto etot zaval ne nablyudaetsya (v dannyh raznyh observatorii est' nekotorye protivorechiya). Avtory dannoi stat'i predlagayut novoe ob'yasnenie - bolee sil'noe vzaimodeistvie neitrino s nuklonami (protonami i neitronami) na etih energiya. obzor hep-ph/0402168 Chernye dyry v teorii s protyazhennymi dopolnitel'nymi izmereniyami: obzor (Black Holes in Theories with Large Extra Dimensions: a Review) Authors: Panagiota Kanti (Univ. of Oxford) Comments: 53 pages, 17 figures Samye sovremennye teorii elementarnyh chastic luchshe vsego opisyvayut fiziku nashego mira, kogda on yavlyaetsya desyati- ili odinnadcatimernym. My "ne vidim" dopolnitel'nye izmereniya potomu, chto oni zamknutye i kompaktnye. Odnako v poslednee vremya predpolozhenie o tom, chto protyazhennost' etih izmerenii poryadka plankovskoi dliny, stanovitsya neobyazatel'nym, odno ili dva iz kompaktnyh izmerenii mogut byt' gorazdo bol'she, vplot' do neskol'kih nanometrov. Dannyi ochen' podrobnyi obzor posvyashen osobennostyam chernyh dyr v mnogomernyh mirah s neskol'kimi protyazhennymi dopolnitel'nymi izmereniyami. Rassmotreny sleduyushie voprosy: rozhdenie mnogomernyh chernyh dyr, radius ih gorizonta, temperatura, vremya zhizni, isparenie i t.d. My budem starat'sya hotya by perechislit' interesnye (dlya shirokoi publiki) stat'i, poyavivshiesya v razdele physics (vklyuchaya cross-listing). physics/0402105 Mnogomernost' izmerenii (The Many Dimensions of Dimension) Authors: S. Deser Comments: 7 pages. Invited lecture, Nordstrom Memorial Symposium, Helsinki, August 2003, to appear in Proceedings Navernoe mnogie pomnyat knigu "Supersila" - ochen' horoshuyu, na nash vzglyad. Kazhetsya, tam est' glava s nazvaniem "Ne zhivem li my v 11-mernom prostranstve?" Seichas podobnye rassuzhdeniya kazhutsya dovol'no privychnymi i estestvennymi. A kogda-to .... Vspomnite hotya by Kanta. V etoi korotkoi stat'e avtor brosaet vzglyad na razvitie ponyatiya "razmernost' prostranstva" za poslednie primerno 100 let. Vernut'sya k nachalu stranicy

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