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COMMISSION ORNL - TM - 2282 COPY NO. DATE

PRELIMINARY

STUDY

OF A MOLTEN-SALT

BURST REACT0

A. M. Perry H. F. Bauman )W. B. McDonald J. T. Mihalczo Distribution 1. 2. 3.4.

F,

Dr. Victor Raievski, M. J. Skinner DTIE

ISPRA

NOTICEThis document contains information of o preliminary noture and was prepared primarily for internal use at the Oak Ridge National It is subicct to revision or correction ond therefore does Laboratarv.

- July

3

.

lo,

1968


..

3

..

A. M. Perry E. F. Bauman

w.

:B. McknaEd J. T. Mihslczo

The cpestion has been poscd whether one could. pulse a molten-salt

r e a c t o r s o as -to achieve an integrated f . ~ u xof

PP nsutrons/cm2

per

b u r s t i n a t e s t cavity a t the center of the reactor, and, i f so, what energy y i e l d would be required and what would be the shape of t h e pulse? The nominal objectives appear to be:

a> 1-2 x

neutrons/crn2 per burst, without a t i g h t specification

on %he neutron spec-imij 2)

a buyst width i n t h e neighborhood of 10 msec o r l e s s .

Since it appears t h a t the second objective sksuld be easy t o s a t i s f y ,

we have looked a t the p o s s i b i l i t y of achieving the f i r s t without much regard f o r f a c t o r s which mighc, influence the b u r s t shape, znd have sub-

sequently estinated the b u r s t width f o r m e of s e v e r a l reactor configurations one might contemplate using.

I. Selection of S a l t The calculztions were based on use of thd salt L i F (73 mole UF4 ( 2 7 m o l e

$1,

and

for each r e a c t o r considered, the c r i t i c a l enrich-

-ment of t h e uranixq was determined. used

5)

Separated Li7 would of course be

I

Relevant properkies of the salt are:

490

Melting point, "C Specific heat of t h e melt, cal/gm 'C Density o f t h e m e l t , gm/crf13 2.

0.217

3.26 - 9.3

X

IO-" T("C)

Allowable Energy Input

We postulate that the ternperature os" the salt could be allowed t o

rise 1090째C, i . e . , nominaLl!-y frorrl 500째C t o l'jO0"C. The p r c p e r t i e s given above yleld the following val-ues a t LO00"C (average tei-ipcszture) :

I


..

.

4

_,

,t

4.33 gm/crn13 4 wsec/cm3

Density §peeific heat

I

Thus, t h e integrated f l u x t h a t can be obialned. i n t h e t e s t c a v i t y

corresponds t o a maximum energy density of

3.

4 kwsec/cn?

per burst.

Geometry -

For t h e purposes of t h i s preliminary expl-oration, we postulate s-gherical geometry, with concentric regions and dimensions as follows :

T e s t cavity (void)

15 cm radius

Ni shell

1 cm thick

fieled s a l t

Ni s h e l l

2-7 t o 60 cm t h i c k 3 cm t h i c k

Graphite s h e l l

23 crn t h i c k

case wzs examined with the thickness of t h e outer Ni cont a i n e r increased to E? cm, end t h e graphite shell omitted; this was done for a 60-cm-thick s a l t region.

4.

c

Results

integrated f l u x e s obtainable i n the t e s t cavity a r e shown f o r

!â‚Ź!he

each case i n Table 1, along with geometrical specifications and other derived r e s u l t s .

Some of these r e s u l t s e r e a l s o p l o t t e d i n Fig. 1.

The neutron spectrum for case

#s, with

92-cn-BB core ( 3 ft) is

shown i n Fig. 2, a s t h e i n t e g r a l above energy E, as a function of E,

E where the time i n t e g r a t i o n i s taken over t h e duration of t h e burst. ,

~

,

For

comparison, t h e f i s s i o n spectmm i s a l s o g.iven, narr;.ialized to 1 X IO1" neutrons.

In

case

#?, which w z s the same

8s

case #13 except t h a t the 3-cm X i

and 23-cm grhphite shells were repl.accd by a single 23-cm N i shell, both

4

t h e pezk-to-average power density ratio and t h e integrated flux i n the

2.

t e s t cavity were t h e same as i n case #I-*

Q


Table 1.

Burst

Charadterfstics

vs Core Size

Integrated Flux in Test Cavity

.

Case Number

FueP Outside Dimeter :4

4

152

1821

17.5

854

1.545

3.4

0.97

4714

1

122 112 102

1-9.7

493 398

1.423

3.1 3.0 2.8 2.7

0.95 0.94 0.92 0.91

5333

92

934 718 538 : 391

82

'272

72

3-78

62

108

27.3 32.1 41.4

2.3 2.2 1.7

0.88 0.84 0.77

6

7 8 9 10 11 a shell

Fuel Volume (liters)

Far all cases shown, catity thickness = 5 cm, graphite

Critical Enrichment ($)

21.1 22.2 24.2

235u xass 0%)

253 200 12Q

!hta1 (neutrons/cm*

1.378 1.331 1.282

333

153

R p a%

*

1.231 1.1.78 I.123

outside diameter = 30 cm, inner shell thickness = 25 cm.

shell

thickness

>lOO kev x 1QWx6)

Burst Yield (Mw set)

2084

1615 12x4

= 1 cm, outer

883 605 382


6 d


e

.

*:<<3

.. ...i..i.i.i.i... Y

b

n

<:c9

.

.

h

B,'

FIG. 2

.

. n

h


8 h estimate of the buret width was made f o r ease #2 (not l i s t e d i n Table 1) which w a s the sme as ease #l except t h a t the graphite s h e l l thickness was PO em.

The Rossi a a t delayed c r i t i c a l , a&, was calcu-

lated, by use sf the DTF transport eoae, and f o n d t o be 9 x PO'

seceP.

The b u s t width was estimated approximately fmm the e x g r e s s i ~ n l

where M =

(p-I)

and p i s the r e a c t i v i t y i n doPPass.

mus, f o r p =

2 dollars, t h e burst width a t half m a f i m i s estimated t o be 0.4 msec. me r e a c t o r s smaller than case #2 w o u hive ~ narrower bursts.

5.

Discussion

Several i n t e r e s t i n g f e a t u r e s a r e apparent from these results. a)

me reactors are all f a s t , i.e.,

from 25 t o 40$ of the t o t a

integrate& flux is above 188 kev, and essential%y 81% of %he f1u.x is above P kev. b) The flux sf neutrons above 100 kev i s quite i n s e n s i t i v e t o r e a c t o r $ i z e , when t h e n o m b i z a t i o n i s for a given maxinun energy density (e.g.,

4 kwsec/c$).

mis

is so because t h e peak-to-average

~ ee 4ehe power density r a t i o rises with increasing core s i z e (see ~ a b 1)

t o t a l f l u x f a l l s o f f f a i r l y sharply w i t h decreasing core size below perhaps 30 i n . dian. e>

A s i n g l e nickel container shell, perhaps

6 i n . thick, appears L

t o be a s a t i s f a c t o r y reflector, yielding q u i t e flat power d i s t r i b u t i o n s ,

at Peast f o r the case studied.

It i s possible that some gains could be -

'

realized by optimizing the container-reflector regions of the assembly. ci)

Buss% widths.

While t h e b u r s t widths have not been calculated

with great care, the r e s u l t s obtained for one of the Largest cores studfea appear to s0m.m the expectation that the pulses of the desirea

magnitude w i l l be l e s s than 1 ansee i n widkh.


.. .<.<.2

Very

$r‘

of

PittEe

a practical

ex@mr;ion sf

attention

the

bur3t

Qf the gesmetri

spbericab

Cal

will

ve33eP Details

fsr

be

and

the

intrcackcing

as the

of

the

the~free

in

imy

any

on

by

detafPe

mre

(e .g; )

Pi&id

surface.

be ext%nded

event

the

core

su~stanti~~.'~chanic~

probably

veaseb

3hockr;.

be required. and

mechanisms, very

of

aspects

aepenaing

affected

shape

and

gas,

sl" withstanding

reactih6y

engineering

can 'be p&d&ted

cover

contrsl

to

mechanism,

location

that

wi%% therefore of

the

temperatures

capable

given

quenching

such

arrangement,

the

been

can be significantly

fueb,

by pressurizing

heave to

A thick

The

QF cy'bindrical)~,

somewhat

SQ far

reactor.

Piquiel

e of I

has

rapidly,

in

wil$.

partictiar

of

require

the

t%evices

coneiderab.Je

6. swary A first prohu2e

0 I

2-3 e

intense,

This

&h.meter, of

about

a third than

at

the

sham

having

IL m3ec.

the

per

of burst

can be accomplished a vohme

700 Mw set-

of

possibilfty

bursts

neutrons/cm2

x 10""

cavity.

..

look

ri?haxis

of

about

91ae neutrons above

100

of neutron3

using

a molten-sa.ILt

indicates

can be achieved with

a core

200

liter33

are

essentially

kev.

that in

reactor fluxes

of

a centr&l

perhaps 3.1~2 with aU.

test

30 %n. in

outer

a burst

yield

above

7333e3tim3.tea buret

ts

31 kev,

wrath is

&pad fess


One of the above reactors, operating i n b u r s t mode with a m a x i m

energy density of

4 %Iw

s e c l l i t e r , may be compared with a similar r e a c t o r

operating a t constant ,power with a maxim power density sf

and with a coolant temperature r i s e , AT, equal t o P080'C residence time of the f u e l i n the core, i n seconds.

4 Wj'liter

times the

The implication i s

of course t h a t a r e a c t o r Like case #lo, f o r example, a t a power Bevel of 608 W ,w o a d pmillace a totab (fast) f l u i n the t e s t cavity of 2

x 1 0 ~ ~

neutssas/cm2sec. The power density of

4 Mw/liter

is probably a t t a i n a b l e .

One is

l e d t o speculate that such a reactor, w i t h cooling adequate f o r 600-Mw

operation, could be operated i n pulsed mode w i t h a pulse repetitlorn rate

of' l / s e c .

Since t h e pulses could then not be i n i t i a t e d from a very low

neutron Eevel, it is d a u b t r n that pulses as short as those c i t e d above could be achieved.

We have not yet estimated what pulse shape might be

obtained a t such a h i

r e p e t i t i o n r a t e , but t h e s e appear ta be sC%m

i n t e r e s t i n g p o s s i b i l i t i e s here worth f'urtlner investigation. -%

L

..,.,

>


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