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The R.A.P.Project "Prosto o slozhnom" "Astro-ph za 2006 g." Nemnogo statistiki Predydushii vypusk (N185) Slovar' astroterminov Spisok missii i teleskopov Obzory UFN Stat'i SOZh ANKa Dnya 22.01.2008. Chernaya dyra v Omega Centavra 11.01.2008. Dvoinoe einshteinovskoe kol'co 06.08.2007. Kto eto tam tak bumknul? 14.03.2007. Taina kolec sverhnovoi 06.03.2007. BL Lac v zhestkom gamma Soderzhanie i bystryi perehod k razdelam obzora Stat'i nedeli "Luchshie iz luchshih" arxiv/0805.2396 Millisekundnyi dvoinoi pul'sar s ekscentrichnoi orbitoi v ploskosti Galaktiki arxiv/0805.3371 Gigantskii disk iz holodnogo gaza vokrug blizkoi moshnoi radiogalaktiki NGC 612 (PKS 0131-36) arxiv/0805.4557 Sverhnovaya, porodivshaya Kassiopeyu A, otnosilas' tipu IIB Otdel'nye stat'i Gamma-izluchenie vysokoi energii ot gamma-vspleskov: do GLAST Mikrokvazary: svodka dannyh i perspektivy Millisekundnyi dvoinoi pul'sar s ekscentrichnoi orbitoi v ploskosti Galaktiki Antarkticheskaya astronomiya na submillimetrah i v dal'nem IK: perspektivy dlya bol'shogo teleskopa Sinteticheskaya model' evolyucii AYaG: rost sverhmassivnyh chernyh dyr i obratnye effekty Vozmozhnoe opticheskoe otozhdestvlenie starogo blizkogo pul'sara J0108-1431 Tak ty hochesh' byt' professional'nym astronomom! Gigantskii disk iz holodnogo gaza vokrug blizkoi moshnoi radiogalaktiki NGC 612 (PKS 0131-36) Eksperimental'nyi zond dlya inflyacionnoi kosmologii (EPIC): razrabotka proekta missii v ramkah programmy NASA "Einshteinovskii inflyacionnyi zond" Veivletnyi analiz vremennyh ryadov dlya AYaG: QPO u 3C 273? LOFAR: tranzienty i monitoring radioneba Rentgenovskoe mikrolinzirovanie v RXJ1131-1231 i HE1104-1805 Katalog dvoinyh zvezd s hromosfernoi aktivnost'yu (tret'ya versiya) Sverhnovaya, porodivshaya Kassiopeyu A, otnosilas' tipu IIB Bariony: chto, gde, kogda? Novyi katalog zvezd s bol'shimi sobstvennymi dvizheniyami KADoNiS- karlsruevskaya astrofizicheskaya baza dannyh po nukleosintezu v zvezdah Iz razdela physics f(R) Teorii gravitacii Tekushee sostoyanie proekta CLIO Kvantovaya gravitaciya vchera i segodnya Supersimmetriya i superstrunnaya fenomenologiya w-indeks: sushestvennoe uluchshenie h-indeksa Polnyi Arhiv predydushih vypuskov. Arhiv statei, voshedshih v vypuski s 01 iyulya 2002 g. po 31 marta 2003 g. Arhiv na 14.04.2006 odnim failom (36.9 Mb; *.tar.gz) gzip homepage 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 2001-2003 gg. Obsudit' na forume Scientific.RU Obsudit' na forume Zvezdocheta Obsudit' v bloge na Subscribe.ru Avtor proekta Sergei Popov Ranee uchastvovali: Mihail Prohorov Ekaterina Kasimova Diskussii po stat'yam Arhiva CosmoCoffee arXiv Blog Postav'te u sebya nashu knopku! Proekt razmeshen na saitah: Smotri takzhe diskussii i blogi: Informacionnye partnery Vy mozhet takzhe razmestit' na svoem saite nashu lentu obzorov Kniga avtora obzorov Novostnye lenty Novosti kosmonavtiki Novosti Nauchpopa Novosti ot UFN Informnauka Researcher@ Elementy.Ru Grani.Ru Perst Podpiska na rassylku obzorov na Subscribe.Ru Druzhestvennye rassylki: "Astronomiya segodnya" "Okno vo Vselennuyu" Spisok astrorassylok

Obzory preprintov astro-ph Vypusk N186 astro-ph za 16 - 31 maya 2008 goda: izbrannye stat'i Referaty otdel'nyh statei obzor arxiv:0805.2221 Gamma-izluchenie vysokoi energii ot gamma-vspleskov: do GLAST (High energy gamma-ray emission from Gamma-Ray Bursts -- before GLAST) Authors: Yi-Zhong Fan, Tsvi Piran Comments: 24 pages, An invited review article for Front. Phys. China. (Possible prompt and very early GeV-TeV emission from GRB 080319B are discussed in Sec. V) Hotya gamma-vspleski i nazyvayutsya gamma-vspleskami, no v samom dele zhestkoe gamma-izluchenie ot nih nablyudaetsya ne tak uzh chasto. Odnako est' neskol'ko primerov obnaruzheniya gamma-vspleskov na energiyah >20 MeV. V preddverii zapuska sputnika GLAST avtory summiruyut predydushie nablyudeniya i delayut nekotorye predskazaniya. miniobzor arxiv:0805.2378 Mikrokvazary: svodka dannyh i perspektivy (Microquasars: summary and outlook) Authors: I. F. Mirabel Comments: Review based on courses given at international schools for graduate students and post-docs; 13 pages, 7 color figures Nebol'shoi obzor po gruppe tesnyh dvoinyh sistem, v kotoryh pri akkreciyu na chernye dyry (hotya, pohozhe, est' sistemy i s neitronnymi zvezdami) voznikayut relyativistskie vybrosy (strui), za chto sistemy i prozvali mikrokvazarami. arxiv:0805.2396 Millisekundnyi dvoinoi pul'sar s ekscentrichnoi orbitoi v ploskosti Galaktiki (An Eccentric Binary Millisecond Pulsar in the Galactic Plane) Authors: D. J. Champion et al. Comments: 28 pages, 4 figures inc Supplementary On-Line Material. Accepted for publication in Science, published on Science Express: 10.1126/science.1157580 Obnaruzhen interesnyi dvoinoi millisekundnyi pul'sar. Po otdel'nosti ego svoistva ne byli by stol' interesny, no ih kombinaciya zadaet zagadki. Eto millisekundnyi (2.15 msek) pul'sar, u kotorogo kompan'onom yavlyaetsya normal'naya zvezda solnechnoi massy, pri etom orbita imeet vysokii ekscentrisitet (0.44) i bol'shoi period (95 dnei), a nahoditsya sistema v ploskosti Galaktiki. Krome togo, ocenka massy neitronnoi zvezdy daet 1.7-1.8 mass Solnca (no eta velichina eshe mozhet, na moi vzglyad, preterpet' pereocenku). Zagadka v tom, chto standartnye evolyucionnye shemy ne dayut takih sistem. Est' neskol'ko variantov ekzotichnosti, obsuzhdaemyh avtorami. Pervyi: pul'sar takim i rodilsya. Vtoroi: eto byla troinaya sistema. Tretii: pul'sar popal v ploskost' Galaktiki iz sharovogo skopleniya. Scenarii s troinoi vyglyadit naibolee privlekatel'nym. arxiv:0805.2487 Antarkticheskaya astronomiya na submillimetrah i v dal'nem IK: perspektivy dlya bol'shogo teleskopa (Submm/FIR astronomy in Antarctica: Potential for a large telescope facility) Authors: Vincent Minier et al. Comments: 19 pages, 2nd ARENA Conference: The Astrophysical Science Cases at Dome C, Potsdam : Allemagne (2006) Avtory obsuzhdayut usloviya na ploshadke Dome C v Antarktide s tochki zreniya ustanovki bol'shogo instrumenta, rabotayushego v oblasti 100 - 1000 mikron. Takoi instrument dolzhen zanyat' mesto mezhdu kosmicheskim proektom Gershel' (60-500 mikron) i nazemnoi ustanovkoi ALMA (350 mikron - 7 mm). U Gershelya budet malaya sobirayushaya ploshad', a ALMA budet imet' malen'koe pole zreniya (da i usloviya nablyudenii budut ne ideal'ny). S tochki zreniya uslovii nablyudenii mozhno stavit' pribory na sharah ili samoletah, no luchshe, konechno, naiti chto-to podhodyashee na Zemle. Vyvod avtorov sostoit v tom, chto Dome C luchshee v mire mesto dlya takogo teleskopa. Krome togo, obsuzhdayutsya nauchnye zadachi dlya takogo instrumenta (zvezdoobrazovanie, formirirovanie i rannyaya evolyuciya galaktik, malye tela v solnechnoi sisteme i tp.). arxiv:0805.2499 Sinteticheskaya model' evolyucii AYaG: rost sverhmassivnyh chernyh dyr i obratnye effekty (A synthesis model for AGN evolution: supermassive black holes growth and feedback modes) Authors: Andrea Merloni, Sebastian Heinz Comments: 22 pages, 14 color figures. Accepted for publication in MNRAS Avtory stroyat evolyucionnuyu populyacionnuyu model' dlya aktivnyh yader galaktik. Napomnim, chto populyacionnyi sintez yavlyaetsya populyarnym metodom v sovremennoi astrofizike, v tom chisle i pri izuchenii aktivnyh yader galaktik. Avtory pytayutsya, poka vozmozhno, osnovyvat'sya na nablyudeniyah, a ne zadavat' kakie-to zavisimosti i korrelyacii rukami. Modeliruetsya evolyuciya funkcii svetimosti AYaG s krasnym smesheniem. arxiv:0805.2586 Vozmozhnoe opticheskoe otozhdestvlenie starogo blizkogo pul'sara J0108-1431 (A possible optical counterpart to the old nearby pulsar J0108-1431) Authors: R.P. Mignani, G.G. Pavlov, O. Kargaltsev Comments: 5 pages, 4 figures, submitted to A&A Avtory raportuyut o vozmozhnom obnaruzhenii v opticheskom diapazone blizkogo (130 pk) starogo (166 millionov let) radiopul'sara. Vse govorit o teplovom izluchenii (T=90 000K) vsei poverhnosti (R=13 km) neitronnoi zvezdy. Esli eto i v samom dele tak, to eto ves'ma interesno, t.k. standartnye modeli ohlazhdeniya (bez dopolnitel'nyh istochnikov tepla, naprimer iz-za raspada magnitnyh polei ili vnutrennego treniya) ne dayut takie temperatury dlya stol' staryh ob'ektov. arxiv:0805.2624 Tak ty hochesh' byt' professional'nym astronomom! (So you want ti be a professional astronomer!) Authors: Duncan A. Forbes Comments: 6 pages, accepted for publication in Mercury Dovol'no zabavnaya pamyatka-putevoditel' dlya teh, kto hochet stat' astronomom. V osnovnom eto dlya studentov, prichem v osnovnom ne dlya nashih, no i nashi naidut tam koe-chto poleznoe (i ne tol'ko studenty). arxiv:0805.3371 Gigantskii disk iz holodnogo gaza vokrug blizkoi moshnoi radiogalaktiki NGC 612 (PKS 0131-36) (Enormous disc of cool gas surrounding the nearby powerful radio galaxy NGC 612 (PKS 0131-36)) Authors: B.H.C. Emonts et al. Comments: 13 pages, 9 figures. MNRAS in press Po nablyudeniyam na ATCA (Australia Telescope Compact Array) obnaruzheno, chto blizkaya linzovidnaya galaktika NGC 612, soderzhashaya odin iz blizkih moshnyh radioistochnikov (PKS 0131-36), pogruzhena v gigantskii (140 kpk) disk holodnogo neitral'nogo vodoroda. Massa diska slegka prevoshodit milliard solnechnyh mass. Izuchenie diska pozvolyaet takzhe sdelat' vyvod o tom, chto u etoi galaktiki est' ochen' massivnoe galo temnoi materii. arxiv:0805.4207 Eksperimental'nyi zond dlya inflyacionnoi kosmologii (EPIC): razrabotka proekta missii v ramkah programmy NASA "Einshteinovskii inflyacionnyi zond (The Experimental Probe of Inflationary Cosmology (EPIC): A Mission Concept Study for NASA's Einstein Inflation Probe) Authors: James Bock et al. (for the EPIC Science and Technology Teams) Comments: 196 pages V NASA razrabatyvayutsya proekty, kotorye mogli by dat' informaciyu ob inflyacionnoi stadii vselennoi (esli ona byla). Vidimo, edinstvennyi real'nyi put' v blizhaishee vremya - detal'noe izuchenie polyarizacii reliktovogo izlucheniya. V kakom-to ob'eme takie izmereniya mozhno provodit' s Zemli (i eto delaetsya). Odnako kosmicheskii proekt nesravnenno luchshe. Sputnik Planck, zapuskaemyi v etom godu, budet pervym shagom v dannom napravlenii. No nuzhny bolee sovershennye apparaty. V ramkah proekta Einstein Probes budet sdelano tri missii: The Joint Dark Energy Mission (JDEM), Inflation Probe, Black Hole Finder Probe. Obsuzhdaemyi v dannoi stat'e proekt EPIC - eto odin iz variantov Inflation Probe. Poka idet pervaya faza prorabotki proekta. T.e., rassmatrivayutsya raznye varianty komponovki (chto vlechet raznuyu stoimost' proektov), izuchayutsya neobhodimye tehnologii, rassmatrivaetsya, kak budet vliyat' fon i tp. Material horosh tem, chto daetsya ponyatnyi obzor po raznym aspektam, svyazannym s zadachami proekta. Sovetuyu prochitat' stranicy 8-18 i 31-34 (nomera stranic po poryadku, a ne soglasno ih napechatannym nomeram, dlya poslednih eto 1-11 i 24-27). V vysokom razreshenii stat'ya dostupna zdes'. arxiv:0805.4342 Veivletnyi analiz vremennyh ryadov dlya AYaG: QPO u 3C 273? (Wavelet Analysis of AGN X-Ray Time Series: A QPO in 3C 273?) Authors: C. Espaillat, J. Bregman, P. Hughes, E. Lloyd-Davies Comments: 34 pages, 15 figures, ApJ, 679:182-193, 2008 May 20 QPO- eto kvaziperiodicheskie oscillyacii. T.e., v izmenenii potoka izlucheniya ot istochnika est' kakoi-to ne slishkom chetkii, no dostatochno stabil'nyi periodicheskii process. Est' raznye tipy QPO i raznye modeli. Prakticheski vsegda rech' idet o diskovoi akkrecii na neitronnye zvezdy i chernye dyry. Esli akkreciya idet na chernuyu dyru, to u diska est' vnutrennyaya granica, t.k. nachinaya s nekotorogo rasstoyaniya net ustoichivyh orbit, t.e. disk ne mozhet podoiti pryamo k gorizontu. Rasstoyanie zavisit ot massy chernoi dyry i ee vrasheniya. V prosteishem sluchae medlenno vrashayusheisya dyry mozhno poluchat' ocenku massy. No mogut byt' i drugie modeli. Naprimer, eto mogut byt' kakie-to gidrodinamicheskie neustoichivosti v diske. Poka QPO nablyudalis' tol'ko v tesnyh dvoinyh sistemah, t.e. ni odnogo sluchaya dostovernogo QPO u aktivnyh yader galaktik ne bylo naideno (pravda, est' kvaziperiod u chernoi dyry v centre nashei Galaktiki, no eto uzhe drugaya istoriya). Avtory predstavlyayut analiz, soglasno kotoromu u pervogo identificirovannogo kvazara 3C273 (umestno upomyanut', chto Martin Shmidt 28 maya etogo goda poluchil premiyu Kavli za otkrytie kvazarov) est' kvazaperiod. Esli schitat', chto eto period obrasheniya po poslednei ustoichivoi orbite, to ocenka massy poluchaetsya ot 7.3 milliona mass solnca do 81 milliona (pri maksimal'nom vrashenii). Odnako rannie ocenki massy chernoi dyry po metodu reverberacionnogo kartirovaniya davali sushestvenno bolee vysokuyu ocenku - 235 millionov mass solnca. Znachit, pishut avtory, vozmozhno, chto nablyudaemye QPO - eto kakie-to kolebatel'nye mody v diske, a ne period na vnutrennei ustoichivoi orbite (nu, ili ocenka po reverberacionnomu kartirovaniyu ne verna). arxiv:0805.4349 LOFAR: tranzienty i monitoring radioneba (LOFAR Transients and the Radio Sky Monitor) Authors: Rob Fender, the LOFAR Transients Key Science Project Comments: 11 pages, In "Bursts, Pulses and Flickering: wide-field monitoring of the dynamic radio sky", Tzioumis, Lazio & Fender (Eds), Proceedings of Science, 2007 LOFAR - novyi kompleks nizkochastotnyh radioteleskopov, kotoryi dolzhen vstupit' v stroi v blizhaishie gody (tochnee, stancii budut postepenno sooruzhat'sya v neskol'kih evropeiskih stranah, a pervaya uzhe rabotaet). V stat'e privoditsya kratkii obzor proekta i perechislyayutsya osnovnye zadachi. Zatem avtory koncentriruyutsya na odnoi iz nih - monitoringe neba s cel'yu obnaruzheniya vspyhivayushih (tranzientnyh) ob'ektov. Provodit' nablyudeniya tranzientnyh ob'ektov v radio ochen' trudno, na nizkih chastotah osobenno. Esli LOFAR zarabotaet kak nado, to mozhno ozhidat' ochen' interesnyh otkrytii. arxiv:0805.4492 Rentgenovskoe mikrolinzirovanie v RXJ1131-1231 i HE1104-1805 (X-ray Microlensing in RXJ1131-1231 and HE1104-1805) Authors: G. Chartas, C. S. Kochanek, X. Dai, S. Poindexter, G. Garmire Comments: 20 pages, includes 8 figures, submitted to ApJ Ne ustayu udivlyat'sya, kakie vozmozhnosti daet gravitacionnoe mikrolinzirovanie dlya izucheniya nerazlichimyh s pomosh'yu sovremennyh priborov ob'ektov. Ideya prosta, prodstav'te sebe linzirovanie dalekogo kvazara: est' kvazar, est' my, a mezhdu nami galaktika, vystupayushaya v roli linzy. No v etoi galaktike est' zvezdy. I oni mogut davat' effekt mikrolinzirovaniya. Istochnikom v dannom sluchae yavlyaetsya akkrecionnyi disk vokrug sverhmassivnoi chernoi dyry v kvazare. V rezul'tate, my mozhem poluchat' ocenki razmera izluchayushei chasti diska. Eto ispol'zovalos' dlya proverki modelei diska (model' Shakury-Syunyaeva horosho podhodit), dlya izucheniya korrelyacii razmera diska s massoi cherynoi dyry i t.d. V ocherednoi stat'ei avtory izuchayut linzirovanie v rentgenovskom diapazone, chto dovol'no netrivial'no. Mozhno ocenit' razmer izluchayushei oblasti. Rezul'tat (menee 6 gravradiusov) nalagaet sushestvennye ogranicheniya na modeli koron diskov v aktivnyh yadrah. katalog arxiv:0805.4517 Katalog dvoinyh zvezd s hromosfernoi aktivnost'yu (tret'ya versiya) (A catalog of chromospherically active binary stars (third edition)) Authors: Z. Eker et al. Comments: 5 pages, including 2 figures and 3 tables, accepted for publication in MNRAS Sam katalog, konechno zhe, dostupen po seti na saite CDS, a v stat'e dano kratkoe opisanie. V katalog vhodit 409 sistem, iz kotoryh polovina - novye otozhdestvleniya. arxiv:0805.4557 Sverhnovaya, porodivshaya Kassiopeyu A, otnosilas' tipu IIB (The Cassiopeia A Supernova was of Type IIB) Authors: Oliver Krause et al. Comments: 17 pages, 4 figures, including online supporting material; to be published in Science on 30 May 2008 Ostatok sverhnovoi Kassiopeya A yavlyaetsya odnim iz samyh molodyh v Galaktike. V ego centre nablyudaetsya zagadochnyi kompaktnyi ob'ekt. Vse vremya idut spory o tom, k kakomu tipu otnosilas' sverhnovaya, porodivshaya ostatok i kompaktnyi ob'ekt. Avtory analiziruyut opticheskii spektr, poluchennyi po nablyudeniyam svetovogo eha. Ideya sostoit v tom, chto my mozhet seichas nablyudat' otrazhenie samogo vzryva, i po spektru opredelit' tip sverhnovoi. Analiz pokazal, chto vzorvalos' gelievoe yadro krasnogo giganta. T.e., sverhnovaya otnosilas' k tipu IIB. Sm. takzhe arxiv:0805.4607, gde drugaya gruppa nablyudatelei takzhe privodit novyi dannye po ostatku Cas A. obzor arxiv:0805.4635 Bariony: chto, gde, kogda? (Baryons: What, When and Where?) Authors: Jason X. Prochaska, Jason Tumlinson Comments: Proceedings Review for "Astrophysics in the Next Decade: JWST and Concurrent Facilities", ed. X. Tielens, 38 pages, 10 color figures Bol'shoi obzor, posvyashennyi voprosu o tom, gde nahodyatsya bariony na raznyh krasnyh smesheniyah, i kak ih mozhno nablyudat'. Istoriya nachinaetsya s epohi reionizacii, a osoboe vnimanie udeleno krasnym smesheniyam 3, 1 i 0. katalog arxiv:0805.4736 Novyi katalog zvezd s bol'shimi sobstvennymi dvizheniyami (A New All-Sky Catalog of Stars with Large Proper Motions) Authors: Sebastien Lepine et al. Comments: 5 pages, To appear in proceedings of IAU Symposium No. 248 - A Giant Step: from Milli- to Micro-arcsecond Astrometry, Shangai : China (2007) Avtory kratko opisyvayut novyi katalog zvezd s bol'shimi (>0.15 sekund v god) sobstvennymi dvizheniyami. Katalog pokryvaet vse nebo. Pravda, avtory ne opisyvayut, gde katalog skachat'. baza dannyh arxiv:0805.4749 KADoNiS- karlsruevskaya astrofizicheskaya baza dannyh po nukleosintezu v zvezdah (KADoNiS- The Karlsruhe Astrophysical Database of Nucleosynthesis in Stars) Authors: I. Dillmann, M. Heil, F. Kppeler, R. Plag, T. Rauscher, F.-K. Thielemann Comments: 5 pages Conference Proccedings "CGS12", Notre Dame/ USA (4.-9. Sep. 2005) A vot eti avtory privodyat ssylku na svoyu bazu. I opisyvayut ee v neskol'kih zametkah (arxiv:0805.4755, arxiv:0805.4747, arxiv:0805.4756). V baze privodyat eksperimental'nye dannye po secheniyam, aktual'nym dlya raschetov s- i p-processov. arxiv:0805.4758 Pobit predel na gravitacionnye volnya ot pul'sara v Krabe po dannym i zamedlenii (Beating the spin-down limit on gravitational wave emission from the Crab pulsar) Authors: The LIGO Scientific Collaboration: B. Abbott, et al Comments: 6 pages, 1 figure Po rezul'tatam neskol'kih mesyacev nablyudenii komanda LIGO smogla postavit' pryamoi (t.e. poluchennyi po dannym gravvolnovogo detektora) predel na gravizluchenie ot pul'sara v Krabe. I predel etot luchshe kosvennogo predela, poluchennogo po detal'nomu taimingu pul'sara. S odnoi storony, rezul'tat nulevoi. S drugoi - LIGO eshe raz pokazyvaet, chto predely, ustanavlivaemye etim eksperimentom, luchshe kosvennyh. My budem starat'sya hotya by perechislit' interesnye (dlya shirokoi publiki) stat'i, poyavivshiesya v razdele physics (vklyuchaya cross-listing). arxiv:0805.1726 f(R) Teorii gravitacii (f(R) Theories Of Gravity) Authors: Thomas P. Sotiriou, Valerio Faraoni Comments: 47 pages, review commissioned by Rev. Mod. Phys; Bol'shoi obzor po stavshim populyarnymi f(R) teoriyam gravitacii. Lyudi davno pytayutsya rasshirit' OTO, sobstvenno, s momenta ee poyavleniya byli popytki kak-to ee uluchshit', da i pri svoem rozhdenii OTO byla okruzhena konkurentami. f(R) teorii osnovyvayutsya na modifikacii deistviya Gil'berta-Einshteina putem zameny skalyara Richi na bolee obshuyu funkciyu (sm. formulu 3 na str. 3 v obzore), prichem f(R) chatso predstavlyayut v vide ryada, sohranyaya chleny do opredelennogo poryadka. Dal'neishie detali - v obzore. arxiv:0805.2384 Tekushee sostoyanie proekta CLIO (Current status of the CLIO project) Authors: K. Yamamoto et al. Comments: 8 pages, 9 figures, Amaldi7 proceedings, J. Phys.: Conf. Ser. CLIO - Cryogenic Laser Interferometer Observatory. Eto prototip yaponskogo proekta LCGT (Large-scale Cryogenic Gravitational Telescope). On nahoditsya v shahte Kamioka, gde budet stroit'sya i LGCT. CLIO - nebol'shoi proekt, dlina plecha vsego lish' 100 metrov. Sootvetstvenno, ego zadachi ne nauchnye, a tehnicheskie. Poka prototip uspeshno otrabotal pri komnatnoi temperature, a pri rabote v rezhime s ohlazhdeniem vyyavilis' problemy. Obo vsem etom i blizhaishih planah - v stat'e. arxiv:0805.2935 Kvantovaya gravitaciya vchera i segodnya (Quantum gravity yesterday and today) Authors: Bryce DeWitt Comments: 9 pages, 2 figures, 31 references. Accepted by GRG Publikuetsya ranee neizvestnyi tekst Bryusa DeVitta, umershego chetyre goda nazad. Tekst byl obnaruzhen v zapisyah uchenogo bez ukazaniya togo, dlya chego on byl napisan. Zapiska posvyashena istorii kvantovoi gravitacii i nekotorym osnovnym koncepciyam. Obsudit' v ZhZh-soobshestve ru_astroph. Obsudit' na Astroforume v Nauchnoi panorame. arxiv:0805.3726 Supersimmetriya i superstrunnaya fenomenologiya (Supersymmetry and Superstring Phenomenology) Authors: Mary K. Gaillard, Bruno Zumino Comments: 18 pages. To be published in `Supersymmetry on the Eve of the LHC'', a special volume of the European Physical Journal C (EPJC) dedicated to the memory of Julius Wess Nebol'shoi obzor po supersimmetrii, superstrunam i istorii razvitiya etih napravlenii. Ne skazat', chto stat'ya legkodostupna, no mnogie veshi neizbezhno napisany dostatochno prosto, po krainei mere dlya fizikov i primknuvshih k nim. arxiv:0805.4650 w-indeks: sushestvennoe uluchshenie h-indeksa (The w-index: A significant improvement of the h-index) Authors: Qiang Wu Comments: 7 pages, 3 tables Etot kitaec ot skromnosti ne umret! :) Na samom dele, vryad li zagolovok otrazhaet real'nost', a uzh srazu vstavlyat' pervuyu bukvu svoei familii v nazvanie indeksa .... Sut' indeksa kraine prosta: w=1, esli u cheloveka est' 10 statei s citiruemost'yu bol'she 10. Indeks raven 2, esli est' 20 statei s citiruemost'yu vyshe 20. U Vittena, skazhem, etot indeks 41, t.e. u Vittena 410 statei s citiruemost'yu vyshe 410. T.o., indeks ceplyaet samyi top statei. Stat'ya zhe interesna tablicei, gde sravnivaetsya mnogo raznyh indeksov, a potom smotryatsya korrelyacii mezhdu nimi. Vernut'sya k nachalu stranicy

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