The lectures will present subjects which are at the interface between particle physics, astrophysics and cosmology. Topics to be discussed include high-energy cosmic rays, neutrino astrophysics and dark matter

Spiro, Michel

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— A . OCR Output` \\~\\~—. . , \`~Y¥$I\., QC j; [fr/~ /4/%=—OQafi[QF ‘£Qs.}Y; O UE\»Jneutrino astrophysics and dark matter.astrophysics and cosmology. Topics to be discussed include high energy cosmic ray,These lectures will present subjects which ure at the inferface between particle physics,ABSTRACTM, 1 §QQ 3Aud1tor1PLAACM} "(/,w/‘14, 1E, 1E, 17 & 18 February from 11.00 to 12.00JiParticle Astrophysics {/mxSPEAER : M. SPIRO /CERN-PPE 2LECTURE SERIES1993 — 1994 ACADEMIC TRAINING PROGRAMMEATO0O00O19pf. T.; _ \»“. ‘TQ, g ;é$s;¤;és;».;s;ész; *:?>;,.. i , ;\\"~ —f—.. — ` »\» vi \ \ `_~` *I \ ~ ;.—{_` \\ `. _\__¤ .·—‘»·`.·»‘~?i‘·:~*:i\>\`1;·>:i\2· `—‘— y·— _‘·:—¤\l, —‘·»‘ ;c·>*;1·»¤>—is*§\>;e·§<s»>—¤~>*:`·—><\~: —\i~.;Tt·~*$;;~>~—_<·\·$\‘~i·—~i¥·‘·3-5rw ·—·—»~ ~__» ;\®—»·?`~i¥·—.··>T·sT§~»*Y·»>~.\—»‘~\}—».~·§—\>$Q·~>¢~\¤\~~~—‘*¤r ·:0LAR OCR OutputArnosewcknA. NEUTR1 Nosv·ASTR••lonRH AS1’R¤v•\1WMRECT DE1‘€¢‘r•auMRELT BETE¢1‘•a:~•3. W\HPgM`Ai\-\0 GAS, BUSTZ. TBARYONH. DARK MATTER R`¤‘·‘Q'···· * ‘Q‘\•·’» -Q-JakOCR OutputI. COSMO LO 65. ov£R vaE\./ OCR Output6ALA¢‘r•c HALO§6RLPeXy FonnrnoTHE NEE¤S FOR DARK NATTGKBARv¤~•c”` 3` Q2. E. (vAR¤0uS DE`TERHIUAT•0N`§1_FRAHEWORK(Rss? 0<= ?1COSHOLOGY (BAS ¢S 06)Hm*2 R UUSB A/Eme dw ’ »¢><r=<>$ OCR OutputiiA-¤·(•.£»¢·r•·• (a$u·;·1)Fnvron €0¤‘*¤**"“‘g(A\_g COHOVINLcr=.·:C : .9.1T R O:J. on A SPHEREB M"mk`.\RCLE OF RMMU';SPHERE(\\O¥f\O&€h¢0¤.S/ LSOIZTOQLLCURVED SPACE*r0bAy OCR Output04<%<4HO :·. Rx ’100hv~• [Mpa/SH¤/c.RsusunvrAe RU?}-1Z: }\,,-X¢ ., *12)({4% MvfAg: OS=¢m RWhz | sn|~ev&·. (b> = _ De<e\c»·4 kohz ,| PULLJQQ HuguiH [bx :hz OI- hL L·|.VA°+TS;:0A.A .AS = C at ` Ru) ;g 1‘ 2 2Freutmhh _ Robcvbgm, _ wack, (FR U( re` GtwisttzQ k Z O OCR OutputSHA LLVERVERPREDICTSINFLATIONESITYV>\CouCURV"~7;?£QEZEYW= ¤<·-;¤>n= Q *· * —¢an°*=Pnéi sa: Q.*$%°’° = ~°mug" Achg;* ·— Pd(+ L; EY=$>EJQVA7 chSC· <(.) ·:. — -E-Ig'MANN EQUATIOIUS} vlO J ba/L,XZ;ALfHOUE ··|» f -5 H +¥Z: IOnA·v1·£R ERAng} OCR Output6uT_) Z·:|O_’ RELA`HV|S`ULtvAcuuu) 6*:;: 60 u~»F•,A·r»o}:(T > $*0* —-» REL ERA I T'7Scsw/m¤0STANDARDwaneVE*ll:) _kcvA ¢2 s yt. A VA EN;— : :4}( H = QP:—°[zERA =>T0m>R<2ow?OCR OutputOCR OutputACUUM4 d u-H i>OCR Output··»••.•&{ww Rn" Q F?;$Erm.HRTTER ERAR€HEAr•ug guns, 0VAwv¤ ERA -·.» NFL'T; `C"REL. ERAT>`I}¢a•·••¢>T4 Tcvg; T>T‘NIWDHV/G OCR OutputO O L{`~ COCR Output9 IIwan OCR Outputnppnnnl magnitude mi5 25[my •\ •|. 90Yyvon IlI•\cnll••\ AL 90I0 ybumblnowyailnlanh •\ nl 66K•o Il, Joan •\ nl. 90, hrvls and Tyson Il,0q • Ptlenoa •\ nl. 79UO QV.·5l0O0,... •°' \IOQA = O.,I0hint galaxy .·>u..·• In B,.£}‘?1c(—· 0-FOCR OutputOCR OutputEX TIN CT ION (2](sie. OCR OutputV1- < G" u>N'IE?~A¢.T|••J E"PA"’$'0VwwwFREEZE OurT N{-;\·=Y¥Q,°x¤°/z·Z Q F §.**xA=%c/T ( hz 2;~<¢:2 XXT»OCR OutputHERMO. Mm EXPANS•oNYG OCR OutputSm~~.., \p[S¢M.E °> N~\·/*=`** $0**4v,. no ¢,». s".0., 2 4AT FREGZC QUT_ <¤r’v>/ no uma:Sly Q- =X = WW1 PANNIHILHTWNE)¢?ANS\0NF¤E£2£ ouT(e` "/1* )lsovrznav svrnisxsb""‘"‘°S XX @3 V7? XXNEUTRAGUFmzeze our cx. x® comNOT SEENAT GALALTIL SCALE ( <¤°} OCR OutputI0H ¤L 1 $9 4 252: no H ;_-;> 5\F ONL BA¢?Vm1SX BELHQL MATTER an~BACK m ‘rmE YQ. ~4Q¤(Z~2\CAI,. FOR\1AT•oNTHE STANDARB LOR€OCR OutputOCR OutputOCR OutputOCR OutputOCR OutputOCR OutputOCR OutputOCR OutputOCR OutputOCR OutputOCR OutputOCR OutputOCR OutputFORHATIGNGALAXYHALO 2 #10 MV; OCR OutputENERAL c;0wc;Lus10Mdistance to the center { R Q c 50 5 10152025 503550.9 ‘ 2*z.Qmx»— s;. 1001:-••••••••••bgiP§28•¤v E26rr 5 •,__ Visible edge•»-·` .*.124zzE E UnOCR OutputOCR OutputOCR OutputOCR OutputIn QNccswa20F sPxRA•. GRLAMESROTAT¤0M cUR\/Ewe STANDARD¤* Biowu Dvhxrr OCR Output$"V*L’— USUNS" or ABome1> STARSBmw HpL.ES’ weurnw xmas%AK~{c>u¤e DARK WATTER(\-\P<Lv) OBAELTSHASSNE ASTROPHy§\LA;_ CO;-,,¤/myMACHO :·? xoctué»m44T;J/ ’ 4/M''’··»°» %»*—S°>< §2§°.,§L.§©~ELHT)U\ST\L K1 F “`"“cow DARK MATTER x>&`c¤us=·L&` www ww\·H\§$\VE Pf\K`\`\LLESVIN? : MJEAKL7 mvzehwmg\`e¢¢-p‘nRELATNKTILHOTDIA•< HATTE12. I1CCOUfLE` wasp/{OTLEO EVye O" Vp 0** 3/e~\.\G\·\T NEUTRINOQ .·.·;OCR OutputOCR OutputT E R M x M 0 Lo 4F ig.1 Present status 0f I2 determinations(.001 < Q .,0.,< 2.)Q = IOr light VDARK MATTERWIMPSINTERGALACTIC \///Y€\\.01 <Qm; .15 .01 < Q;A°`;0H§ .15or light v01 w1M1>sMACHOSMAC!-IOs.001 < cz f,._f< .01'‘"4/{ 0·4 < O. <‘¥A . at 400k»· i`Hq·2STARS A&£ .t EXP.OCR OutputOCR OutputOCR Output0 0 4 < D. . < 2.Lu OCR Outputmassive object close to the line of sightTelescopeStar OCR Outputmassive object far from the line of sightTelescope(radius RD: Einsteins"cross-section"lensingmassive objectStarm¤V¤¤9OCR OutputOCR OutputOCR OutputOCR OutputGRAVITATIONNAL LENSING EFFECThaving the same mass and, kkc same. xfefocat OCR OutputFor stars in the LMC, and all deflectors(Mm)10 1010 deflector1 10Mass ofduring one year 10000-1stars observed"' 100of events for 16Number- 1010100— 0.11000event (days)Duration ofNew 100 > #{.3A 11 <> L x F 4 4 ATA rea : 2 V L` REb /"\Duration vs Mass of DeflcctorOCR OutputOCR OutputOCR OutputOCR OutputYKESO CH!LE OCR OutputLA Sl LL AAvenue de Cointe, 5, B -4000 Liege, BelgiumInstitut d'Ast:rophysique de LiegeO. MOREAU13120 Marseille, FranceTraverse du Siphon, Les Trois Lacs,Laboratoire d'Astr0nomie Spatiale de Marseille,C. GRY2 place Le Verrier, 13248 Marseille Cedex 04, FranceObservatoire de Marseille,E. MAURICE, L. PREv0T61 avenue de l'Observatoire, 75014 Paris, FranceObservatoire de Paris,I. GUIBERT, F. TAJAHMADY98 bis boulevard Arago, 75014 Paris, FranceInstitut.d’Astrophysique de Paris,J.-P. BEAULIEU, R. FERLEI`, PH. GRISON, A. VIDAL—MADJARCentre d‘Orsay, 91405 Orsay Cedex, FranceLaboratoire de l'Accé1érateur LinéaireR. ANSARI, F. CAVALIER, M. MONIEZDAPNIA, CE Saclay,9l191 Gif—sur-Yvette, FranceS. ZYLBERAJCHL. MOSCOSO, F. QUEINNEC, J. RICH, M. SPIR0 , L. VIGROUX,B. LAURENT, E. LESQUOY, C. NLAGNEVILLE, A. MILSZTAIN,E. AUBOURG, P. BAREYRE, S. BREHIN, M. Gnos, M. LACHIEZE-REY,(Experience de Recherche d'Objets Sombres)

Particle astrophysics

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