pulsars · discovered november 1982 by backer, kulkarni, heiles, goss, and davis -- pure...

29
Pulsars NRAO Summer Student Lecture Dan Stinebring 4 August 1984 general discovered in 1967 -- serendipity and Jocelyn Bell's perseverance radio astronomer's dream rich phenomenology interesting physics neutron star interiors coherent emission mechanism interesting astronomy neutron star formation scenarios binary system evolution Galactic supernova rate useful probes of ISM, Relativity basic model rotating neutron star strong a and rotation -- > strong surface E field surface effects primary positrons (Q * f < 0 case) large Lorentz factors pair creation cascade -- > ee - plasma plasma instability bunching coherent radio emission pulsar phenomena waveforms (average profiles) small duty cycle mode switching interpulses

Upload: others

Post on 10-Dec-2020

2 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

PulsarsNRAO Summer Student Lecture

Dan Stinebring

4 August 1984

general

discovered in 1967 -- serendipity and Jocelyn Bell's perseveranceradio astronomer's dream

rich phenomenologyinteresting physics

neutron star interiorscoherent emission mechanism

interesting astronomyneutron star formation scenariosbinary system evolutionGalactic supernova rate

useful probes of ISM, Relativity

basic model

rotating neutron starstrong a and rotation -- > strong surface E fieldsurface effectsprimary positrons (Q * f < 0 case)large Lorentz factorspair creation cascade -- > ee - plasmaplasma instability

bunchingcoherent radio emission

pulsar phenomena

waveforms (average profiles)small duty cyclemode switchinginterpulses

Page 2: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

2

single pulses

pulse energy variations

nulling

giant pulsessubpulses

drifting

micropulses

polarization

waveforms (Radhakrishnan and Cooke)high degree of linear and (sometimes) circular

single pulsesorthogonally polarized radiationdepolarizationsome pulses 100% polarized

pulsars as..probes

galactic distribution

scale height of progenitorsDM (Dispersion Measure) -- > ne

RM (Rotation Measure) and DM -- > <B>scintillation: ne variations; clumpiness; turbulence

binary pulsar: General Relativity probe

millisecond _oulsars

PSR 1937+214

discovered November 1982 by Backer, Kulkarni, Heiles, Goss, andDavis -- pure perseverance

1.577 millisecond period = 642 Hertzpulse and Interpulseextremely small P-dot (1.0 x 10-19 sec/sec)very young or very old?pulse emission under extreme conditions

low magnetic fieldproximity of light cylinder

0 .

Page 3: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

3

PSR 1953+290discovered April 1983 by Boriakoff, Bucheri, and FauciCos-B error box: gamma-ray source?

but P-dot is not very large6.1 millisecond period = 163 Hertz120-day binary orbitspin-up scenariovery large duty cycle

future workother searches: are there lots or only a few?

difficulty of periodicity searches -- P-2 dependencenon-pulsed searches

high polarizationscintillationsteep spectra

comparison of "vanilla" and millisecond pulsar propertiesbank of celestial clocks

astronomers could take back time-keeping function

Page 4: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

4

Pulsating Stars / and //, Nature reprints 1968 - 1974, MacMillan andCompany, Ltd.

ODoular leJel

Helfand, D. J., 1978, American Scientist, fbZ, 332.Weisberg, J. M. and Taylor, J. H., 1981, "The binary pulsar and general

relativity", Scientific American, 2A, 74.

monographs

Manchester, R. N. and Taylor, J. H., 1977, Pulsars, Freeman and Company.Smith, F. G., 1977, Pulsars, Cambridge University Press.

current esearch

Michel, F. C., 1982, "Theory of pulsar magnetospheres", Rev of ModPhysics, 5A, 1.

Reynolds, S. P. and Stinebring, D. R., editors, 1984, Millisecond Pulsars,NRAO Workshop Proceedings (in preparation).

Sieber, W. and Wielebinski, R., editors, 1981, Pulsars -- Proceedingsof /.A.U. Symposium No. 95, Dordrecht Reidel.

0 .

Page 5: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

5630 Sawtelle BoulevardCulver City, California 90230April 29, 1968

,:1is S. Jocelyn Bell.:ullard R:adio Astronomy ObservatoryCambridge University, England

Dear iss Bell:

I a writing to you about the unidentified radio emissions discovered by theastronomers at Cambridge University. These pulses have created greet excitementamong scientists, and I would like to suggest a new theory about these pulses.Sir Martin Ryle, head of Cambridge University's Radio Astronomy Department, saysthat the pulses are the most exciting astronomicsl discovery of all time.

The period of silence between the pulses is exactly the same every time---1.3372795 seconds. During my research, I noticed that this figure could beindicated as 13-37-27-95. The next step would be to multiply 13 x 37, with theresult of 431. Three sepexrate encyclopedia's list an original height of481 feet for the Great Pyramid (circa 2600 E, C.).

It is possible that the 1.337 has somae special relationship to the engineeringdesign and site of the Great Pyramid. The balance of this 1.337 unit is 2795.To my astonishment, I discovered that these figures appear in order in pi--the ratio of the diameter of a circle to the circumference'.

3.14159653a979233462•43.3.-2--7--9-5....The Great Pyramid's height (481) and base-side (755) appears to show the approximateproportion: 1: 3.14159 :: 481 : 755 x 2.

I noticed that the units contain the logical pattern of 79-79, 32-32 and 38-38,with the center at 26.

The English alphabet has 26 letters.. Therefore, A equals. 1,..B equals 2, C equals

3, D euals 4--to Z equals the same 26.

A-B-C-D-E-G-G-H-I-J-K-L-M--O-P-Q-R-S-T-U-V-T;-X-Y-Z (totails) 351. Rechecking,I discovered that 13 x 27 (1.3 37 27 95) equals the same 351.

It is miy opinion that the radio pulses seem to have some special relationship to ,pi and to the matheatical design and location of the Great Pyramid. The pulsesmay be an attempt to ciirect our attention to the mathematical properties of theGreat Pyramid and to the possible mather tical-engineering design of the Eart.

urs ve", truliy

Kenneth Larson

VICTO Y Rh iS Cn '4•

?1

Page 6: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

1496t 19gZ3.D

15)-53 9lfl6S

-

tl2-fit 1i40-6t 1154 -52 1604-00

b 1 R1

A fl Li 3- A iA-U .Ji i' .S J W JL i2021.I51 2217.47 04 50-18: 201.2 iar-0ai 1t7:3-2 T.,ST -26

n A

C8<35-41 1426-66 1>1-04 1727-47 155a-S

,tliti I.

085-41 14 2-6 ip u-Fos 1727-47 1558-50

2111+46 1133+16 1700-32 0818-13

4i1S t

15s.55) 17 7-46

Ar't- 0

0.031-0i7-

0628-28 0934 06

0809+74 1919+21 1237+25 0959-54 2303.30 2045-16 0525+21

900

2-1 Integratecd pu e profiles for 45 pulsars, all plotted on the same longitude scale (a 9Xbar is giscr in the bottom of the figurea. These profiles were rc cded at frequencies

betwcn 4) and 650 MHz. and are arranged in order of incre ,ing pulse per Ld

P

. 6

kz (~cc

-- /. G

07c25

74

0833- S

'isn

Ii

Q950lu*Q8 1556-44

sec

sc-CLLsex:-

&.

Page 7: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

I

+90* . .

**/ i./o.. ,. ' oo ' ".* ,\

*" 1200 60° * . 0* 300'

I * ... . . *•~~~ • • • • , o I e

*'* * *. - * .." * .- ,. .. *., ; . ...- , * /.. s* .... ,o* . . * .* ***..•.% ~~ \

9* .

\ '~~~~ . -.' . ". /-. " " / I. :.' :

- 90

Fla. 1. An equal-area projection of the distribution of the 330 known pulsars in galactic coordinates. The galactic center is in theitmiddle of t hk

figure and longitude increases to the left.

1953 Astron. J. 86(12), December 1981 0004-6256/81/121953-21500.90 1981 Am. Astron.So 1§8j

Page 8: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

:E

100 200Longitude (degrees )

260

k,

E

0CL

/

300

--

PSR 0950+082000 pulse overage430 MHz

Interpulse -

. f!1. n Ce

01 ...... . 1

Page 9: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

PSR 1133 + 16

AVERAGE

- 20 - 0 O io 20

TI ME

100I O

50

ccw

C)Co

-t~J(Dr.I)

0

M

rl

t

i

i

. J

i

i

(ms)

C Bcc- E- y

Page 10: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

LONGITUDE

C c

(DEG)

JE'c,3 AS4

P7 -2

j

WwzW

1? it, 41 J 3 (3

Page 11: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

\r /

t

wZW3

R.'v. k-4st4 e s4/ 't, Prs . AS B A

z C3) ,t so,

( -RAY

.RADiO

1 -1 - - -• - -

.. ..

10tLONItUBt

tOtO0W)

o

Page 12: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

'0ot.

C! 'C'

/O kf

/DYa O p., led

$4 .r f'ii

S: . .4p'

L1 1 /I i''

P ja ~V &1' Ig

7 'O°

-7~(~l7 i~

.

I I -

Ct !

(/L~

a,9

..

a

.

a -r ; 0, .

Page 13: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

Pc Sa r

I.

; ?

§ as*

V

AG

-, '

5 * : i.

I- c ; 7-

R7 ~

S /

_ _s _~m_vt Apc~ ,,6a

Ap

5,

4 .10,

Page 14: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

D sA

lo f

tl;2,

0r q

-a A)Ca,

6/%e d1eJ 7"

- ( sc)

0. /IO

/. G

l!~E

I

P.Ss

o. Z

- 1L --

rM

D~r tS ,/

~L~e qS e~to

L~pZ/ pJ7P

r {

F f : :" ,

=c(4

.

, :

PS ; ~'i pr

be'e a A

f PI

-42. //ir

Page 15: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

E l -

DM.=.-a0m

alomot

3

/..

A'

d 4 / y

ro- 3"s

4 Yro

-% A00 1"

z/

te o a 5

c so)

)4 P

Lt2C

.-

ot4hcz

sa-e4.

1a S

~SoK

dsr&.

c. Ic 4*thL

- 3 o ,c.

Ac]

I)

-

teS e

*dIs -rVt ces

<.1/ h...

4 I klp'di

ALgo

7o

I . -' J

40*

z

Page 16: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

F , e. AA r.f I4 &S

fL

=

e1 8 Cd 0 ds

at

r~g V-s9 D

)\ iF ,{at a-Zt

ro e. .

4L t 5eo 0

A

Ia 1

--

pop

A/

ds

fCbaet a]

a ~

s 4

k 8RM

Page 17: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

f <ca ..s

~ie

2 '

Is

I?1fla /V 41

ere ct te Cs t,4 l SChet tI6J

/. eI4rjad

at 3"?

'cs1 4 CeSk no ff

C a c r7 4e ic

KB

r

rez fp .,"S

7)

/vlv4)

3)

1/

4/ VI d 4 ,, .,,

J ls ", /

-r IC I

0I,/

rr .8 -

'000

'J

. : 1

r

! s

Page 18: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

+5b

090.

7-5 Mean line-of-sight magnetic feld components in the paths to pulsars. For fieldsgreater than 0,1 pG the area of the eir le is proportional to the field strength (a circlerepresenting a 1 po field i htiwn in the lower right corner). A cross within a circlemeans the rotation measufe i~ iositive (field directed toward the observer). [FromManchester et al.; 1977:i

Page 19: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

100

DIALOCITY

o

y1I

SRAVEL

ri

i

JK

300

0 2 4 6 7.75 HOURS

.059C 50

PULSE

PERIOD

.0590

K

r- I-

.058 970.

RADIAL VELOCITY CURVE,

MEC

200

0.1-0.9 a- 4p .1 glop*~~~- ~ ~ - , ~ ~ - lr *r~, ~ M~rt ~ qc L~F~--

s .. _ _ ._.- -.. - .. __ . __ . :.: .. r w - - r'+ +±a..a,.i..::.,a. w wr~w ,.. i. . .rrr . .:N. .. y -. v «,. .riw ... s",: . w..... Im

i

--- ftz

1011 111 0 q_;_lnlnpi= -nl-c-i-.- 7_ ---. 17.- -- -rTi-v .9-1 - .:p- - - rr it t I __ = im~~r u.-;= ~ "7------;~~;~ i r ~ ~ C" ~ - .A .,_

FIGURhE 1CL

Page 20: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

I

; -

/r

J~

.1 Reldw, A/blt*Cc f r.-s

t

.a..ya

sEmA h.e

S4o */ eis

D. o ifY6P'

to 5s

14 4 a < C,

S

YOt6 c't'_/ af

$ eo.

4sL/y,

r - ---- / L - e ; 4 -L ,--- --

_

3..

Page 21: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

oc

...a eii I

.. :;~bi e*( i,r i-~S- iI ~:

.:. i''C'r;k?;V: I1IL

-I : ~?.';tr tr ;;

.1~21. E.' ~ "" '; rc~~s ''''IIlii~-; L~I

:i n- if";:7'i ;~.i:ij~!l"?.iLii''

c ?~-;: tz iilal~cF~L~P ~; i ,.~.arli 'c.sr. ~y~-..ilh;Li: "i.\ :$ $~ '"1. ,. .1:i-s ~9 i

...'chi-C r:'d.-~U *!, .i;.U x;i

5'.:iC~PI-''tF: L; r

~r-y~f r

'ir* sS

I~k;3~i, ~

.j~-'.. i ' ~T!J~'~r .:;irbZ B,.I i ,o,~,~:,, I ,~,;u ~~'' ;' ''~ h E:'I ~D.iiI I.Drr. ~a ie

")WiQ F~ii- ~t:r

~iiil:c;C -~~.:~ ~~:Y"i

.r a tr .

-;Pf'p~C~ .a; 1r; f~ij

i;.~?,bnP .C-j Z I

t : \"'~it.~ .:

21~d;i~ii~F1'Li* tzr;s rci,, ~: z ~ ?r'

0

LL.

CI:

c-2C1D'-'D

d

S

i

rr

"I

i=

.:

i,

..

n',

{=.

ri "

i':

,1-

L,

' .

t;:

S''

;t

.

f1

I I O 5aerv4 1P

' i"

. ; r: .,'

. " y I.1 /."

i ,

- s' :.

, l:

, , e 1

} : ~

'' " t '

CO)

"i5 }~

r. -

t ? r

>,1

=J Q

1

J

- 0 -3

74 75 76 77 78 79 80DATE

_ -2.4 ! 01.(3

81 82

A I I

--- -- -- --- wwr- -- w

7' _c~ -

,..

. ; .,

i ' .c=

.::

t . '

' .t,.I

Y~;

fi

w . 4

i; .F.~

,i

.. s " " ' ;S

Page 22: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

R

5

A s., eril~sC .

1) 0j ' , '

db/cdvrd-eola'4se;

cc Z,

Loce.

S cC

9/

j#' ,b/A/e

A/ e ,s :S QN4

s1I Ye ne m/

ai 'j %s /4,~ Sv* Co..r-

, .4a -- _ >

,2)

A 'Olt tt., atc

lee. S /4z Q

p,,x,~

ri j

.. 1 Ss

T Q i~re

.. 3^

Page 23: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

PS 4.llij3 16

10

P,00% o*4 57 A.. ~ @8

Page 24: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

Iy

Ir sk5~

Longitude (degrees)

Page 25: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

. :90

O.e- 'f

-- -I I - 'li

WvV

" 4 ~ Sr: ; !;{:: .'go ,tf ; : i : {fe:: ' i

dt~TsB,,r23a :isti .;it, i .

1. 431.1.i i;; : : ors f : .

1{{ '"y- ; . - . ' '

t -""'" - {i1 ' "i ill 17 - ti t" Y't M

1. 1 ?.." Y . y.L j . ::r'%;,L"i"5::., :."il

Longitude -*

4W

iD

o

a.

IS

r~r

CV

A t.A

' r

'-4 '". ;3

. - .:v

Otto,~Nj4m ,

O lf a f4lotIIII Y I

101 4;850

0

C

Cr w

w

A

" r

4

_ _ _ --- L- .- L ~- -rl-~---~- r--

iI

_ - - - - - - _ -- r" . w .siu .s+ a " a w . a twra ...

d

,'-

-- 5

,.

=

c..-,J

*t.,

- F r

. )b.

c

~4rr

; '~ ir' 18. '~'t :~;~;~ ':"! !~::; ..

;~~~p, i -.. :~L;tss: :t.r. ~~:~I: :.:. ~~. .r~::;~~: ;u

::::

Page 26: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

5b4 6 '

C1~se/

V d i * C4

5360Longitude (dre)

E

v

,"4)

cQ)

0

LL.

18

C)C

C0

.r.

0CL

9

0 ..

a(=0

90., Ar

Page 27: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

-3 IS90 / /.

Lonitude (dura.n)

: . I'4

.u 9 o 1 t ou , - .......

Page 28: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

rya16

Page 29: Pulsars · discovered November 1982 by Backer, Kulkarni, Heiles, Goss, and Davis -- pure perseverance 1.577 millisecond period = 642 Hertz pulse and Interpulse extremely small P-dot

3 6o

4xa

I

4

0

hgk ;f*~~