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8/8/2019 On some mathematical equations concerning the functions zeta(s) and zeta(s,w) and some Ramanujan-type series
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1
On some mathematical equations concerning the functions ( )s and ( )ws, and someRamanujan-type series for /1 . Mathematical connections with some equations concerningthe p-adic open string for the scalar tachyon field and the zeta strings.
Michele Nardelli 2,1
1 Dipartimento di Scienze della Terra
Universit degli Studi di Napoli Federico II, Largo S. Marcellino, 10
80138 Napoli, Italy
2 Dipartimento di Matematica ed Applicazioni R. Caccioppoli
Universit degli Studi di Napoli Federico II Polo delle Scienze e delle Tecnologie
Monte S. Angelo, Via Cintia (Fuorigrotta), 80126 Napoli, Italy
Abstract
In this paper, in the Section 1, we have described some equations concerning the functions ( )s
and ( )ws, . In this Section, we have described also some equations concerning a transformationformula involving the gamma and Riemann zeta functions of Ramanujan. Furthermore, we have
described also some mathematical connections with various theorems concerning the incomplete
elliptic integrals described in the Ramanujans lost notebook. In the Section 2, we have described
some Ramanujan-type series for /1 and some equations concerning the p-adic open string for thescalar tachyon field. In this Section, we have described also some possible and interesting
mathematical connections with some Ramanujans Theorems, contained in the first letter of
Ramanujan to G. H. Hardy. In the Section 3, we have described some equations concerning the zeta
strings and the zeta nonlocal scalar fields. In conclusion, in the Section 4, we have showed some
possible mathematical connections between the arguments above mentioned, the Palumbo-Nardelli
model and the Ramanujans modular equations that are related to the physical vibrations of the
bosonic strings and of the superstrings.
1. On some equations concerning some observations concerning the functions ( )s and( )ws, [1]
In the Mathematical Analysis there exist the proof of the following formula:
=)(s1
)]([)1(21
1
2
120
22
++
+
t
s
e
dttsArcTanSint
s (1.1)
that can be rewritten also as follows:
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2
( )( )( )
( ) ( )
++
+=
0 22/2
1
1
1
2
1
11
tansin2
sdt
et
tss
ts (1.1b)
where )(s represent the Riemann zeta function.
Now we analyze in greater detail the formula (1.1)
The function ( )s is represented from the series
( ) ...1
...3
1
2
11 +++++=
sssn
s , (1.2)
as the real part of the complex variable
is +
is greater than the unity. Under the same condition, we have still that
( )( )
=
0
1
1
1x
s
e
dxx
ss , (1.3)
what is easily proved by using the following equality
( )
=0
111 dxxe
sv
svx
s. (1.4)
It is from the expression (1.3) that Riemann reached by an ingenious application of the residue
calculus, extending ( )s across all the plan and discover such interesting properties of this function.
We set ( ) szzf = , where
( ) ( )
+=
tsttp
s
arctancos, 222 , ( ) ( )
+=
tsttq
s
arctansin, 222 . (1.5)
The following three conditions:
1 The function ( )zf is holomorphic for , for each t;
2 The condition ( ) 0lim 2 =+=
itfet
t
is verified uniformly for , however great ;
3 The function ( )zf is subject to the following condition: ( ) 0lim 2 =++
=itfe
t
;
are verified in the half-plane 0> ; assuming 1> , so that the series (1.2) converges, and by
1=m , we obtain, after the application of the following formula:
( ) ( ) ( )( )
+=
mm t
dt
e
tmqdfmfvf
0 2
1
,2
2
1
, (1.6)
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( ) ( ) ( )1
arctansin121
1
2
120
22
++
+=
t
s
e
dttst
ss
, (1.7)
that is the eq. (1.1), and, after the application of the following formula,
( ) ( ) ( )
=m
dttQdfvf
0
,2 , (1.8)
for2
1= ,
( ) ( )1
2arctansin4
12
1
220
22
1
+
+
=
t
ss
e
dttst
ss
. (1.9)
Another expression for ( )s is derived from the following formula:
( ) ( )+
=
i
im
dzzFzi
vf
2
sin2
1. (1.10)
By itz +==2
1,
2
1 , we find
( )( )[ ]
( )
+
+
=
0 2
2
1
2 2arctan1cos
4
1
1
4dt
ee
tst
ss
tt
s
. (1.11)
Starting from the relationship
( ) ...4
1
3
1
2
11
2
11
1++=
sssss
with the application of the following formula
( ) ( )( )
( ) +
=
=
n
m
i
i iziz
vdttQ
ee
dzzfvf
01 ,21 , (1.12)
with2
1,1 == m , we also find
( )( )
+
+
=
0
22
1
2arctancos
4
1
12
2dt
ee
tsts
tt
s
s
s
. (1.13)
It is easy to see that the integrals definite appearing in the above expressions are analytic functions,
holomorphic for any finite value of s . On the other hand, we deduce from the eq. (1.7), for 0=s ,
( )2
10 = ,
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then, subtracting the two members1
1
s, and making tend s to the unity, taking into account the
following equality:
dtet
tC
t
++=
0 22 1
1
12
2
1
, (1.14)
we obtain
( ) =
= 1
1lim
1 ss
s Cdt
et
tt
=+
+
0 22 1
1
12
2
1
, (1.15)
and finally, by differentiating with respect to s , putting 0=s and using the following equality
=
0 2
2log1
1arctan21
dt
et
t, (1.16)
we obtain
( )
=
=0 2
2log11
1arctan20'
dt
et
t. (1.17)
We note that there exist a mathematical connection between and2
15 = , i.e. the aurea
section, by the simple formula
2879,0arccos = , (1.18)
thence we have that
2879,0
1arccos = . (1.19)
We can rewrite the eq. (1.17) also as follows:
( )
=
=
0 2 2879,0
1arccos2log1
1
1arctan20'
dt
et
t. (1.19b)
Now we consider the function
( )( ) ( )
...2
1
1
11, +
++
++=
ssswww
ws , (1.20)
which reduces to ( )s for 1=w . We must replace our general formulas
( ) ( ) swzzf += , (1.21)
where
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( ) ( )[ ]
+++=
w
tstwtp
s
arctancos, 22
2, ( ) ( )[ ]
+++=
w
tstwtq
s
arctansin, 22
2. (1.22)
Assuming the real part of w positive, applying the following formula
( ) ( ) ( ) ( )
+=
mm t
dttmqe
dfmfvf0 2
,1
1221 , (1.23)
we obtain
( ) ( )
+++
=
0 2222
1
1
1arctansin2
21, dt
ew
tstw
w
s
wws
t
sss
, (1.24)
valid expression in the whole plan and shows that ( )ws, is a uniform function admitting forsingularity at finite distance, only the pole 1=s of residue 1. We conclude, on the other hand, for
0=s ,
( ) ww =21,0 , (1.25)
then, subtracting1
1
sand for s tending to the unity,
( )
= +++=
0 2221 1
12
2
1log
1
1,lim dt
etw
t
ww
sws
ts
, (1.26)
and finally, differentiating with respect to s and then for 0=s , we have that
( )
+
=
0 2
'
1
1arctan2log
2
1,0 dt
ew
twwww
ts . (1.27)
For the following equalities,
( ) ( )xJxxxx +
+= log
2
12loglog , (1.28)
( ) ( )xJ
x
xxDx '
2
1loglog += , (1.29)
these last two expressions on reduced respectively to( )( )ww
'and ( ) 2loglog w .
Here it is possible to obtain some mathematical connections with various theorems concerning the
incomplete elliptic integrals described in the Ramanujans lost notebook.
Let ( )qu denote the Rogers-Ramanujan continued fraction defined by
( )
...11
1
1
::
3
2
5/1
++
+
+
==
q
qquu , 1
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and set 2quv = . Recall that ( )q is defined by
( ) ( )( ) ( )
( )
=
+
===0
2
222/13
;
;,:
n
nn
qqqqqfq . (1.31)
Then
( )( )
( ) ( )( )
+
++=
2
232
5
5
251
251log5log
5
8
uv
uvvu
q
dq
q
q
. (1.32)
We note that ( ) 22
15236067977,1251
==+ , i.e. the aurea section multiplied by the
number 2, and that ( )
+==+ 2
2152360679777,3251 , i.e. the aurea ratio multiplied by
the number 2 and with the minus sign.
With ( )qf , ( )q , and ( )qu defined by
( ) ( ) ( ) ( ) ( ) ( )
=
====
n
iznnnzeqqqqqfqf 24/22/132 :;1,: , izeq 2= , 0Im >z , (1.33)
by (1.31) and (1.30), respectively, and with ( ) 2/15 += , we have that
( ) ( )( )( ) =
=
q
uddt
t
tftf
0
2/
cos 22/35
5224/3
2/51
sin51
125
( ) ( )( )( ) ( )( )
=
=
qfqfq qqq
dd3534/31 54/11/5tan2
0
/5tan2
0 22/122/35 sin51
15
sin51
1
. (1.34)
Let v be defined by the following expression
( )( ) ( )( ) ( )
3
53
15
::
==
qfqf
qfqfqqvv , (1.35)
and let ( ) 2/15 += . Then
( ) ( ) ( ) ( )( )
=
=
+
q
vv
vv ddttftftftf0
5/1tan2
1
111
5
1tan2
2
15531
2
21
sin25
91
1
5
1
( ) ( )( )( )( )
( )( )( )
( )( )
+
+
+
++
=
=2/
11
11
1
1tan2
53tan
11
1153tan
2251
5
3
31
1
5
511
sin16
151
1
4
1
sin81
11
1
9
1
vvvv
v
v
vv
vv dd . (1.36)
If v is defined by the following expression
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7
( )( ) ( )( ) ( )
4
72
14
::
==
qfqf
qfqfqqvv , (1.37)
and if 7
21613 +
=c , then
( ) ( ) ( ) ( )
+
=q c
v
vc
ddttftftftf0
cos
1
1cos
2
14721
1
sin232
132161
1
28
1
. (1.38)
Let
( ) ( )( ) ( )733
14323
qfqf
qfqfqv
= and
7
249 =c ,
Then
( ) ( ) ( ) ( )
++
=q c
x
xc
ddttftftftf0
cos
1221
221cos
2
4/714721
1
sin64
213321
12
. (1.39)
1.1On some equations concerning a transformation formula involving the gamma andRiemann zeta functions of Ramanujan.
In the Ramanujans lost notebook there is a claim that provides a beautiful series transformation
involving the logarithmic derivative of the gamma function and the Riemann zeta function. To state
Ramanujans claim, it will be convenient to use the familiar notation
( )( )( )
=
+
+=
=
0 1
11':
k kxkx
xx , (1.40)
where denotes Eulers constant. We also need to recall the following functions associated with
Riemanns zeta function ( )s . Let
( ) ( ) ( )sssss
+=
2
111: 2
1
.
Then Riemanns -function is defined by
8/8/2019 On some mathematical equations concerning the functions zeta(s) and zeta(s,w) and some Ramanujan-type series
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8/8/2019 On some mathematical equations concerning the functions zeta(s) and zeta(s,w) and some Ramanujan-type series
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9
log
0=
dxx
ee xx, 0, > . (1.48)
We now describe a proof of Theorem 1. Our first goal is to establish an integral representation for
the far left side of (1.42). Replacing z by n in (1.45) and summing on n ,
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10
Letting log2
1=n and /2 tx = in (1.55), we deduce that
=
=+
+
0 0 /222
2
3 21
1
2
1
1
12
1
log2
1cos
4
1
2
11dttetedtt
tit
t tt
( )( ) ( ) ( )
+
+
=
0 2/222/2 21
1
111
/2dt
teteteetttt
. (1.56)
Hence, combining (1.54) and (1.56), in order to prove that the far left side of (1.42) equals the far
right side of (1.42), we see that it suffices to show that
( ) ( )
( )
=
+
=
+
0 0
2/
2
/
2/20
2
1
1
11
221
1du
u
e
ueu
dt
t
e
tet
u
u
t
t
, (1.57)
where we made the change of variable /2 tu = . In fact, more generally, we show that
( )( )
=
+
02
2log2
1
2
1
1
1adu
u
e
ueu
ua
u , (1.58)
so that if we set ( )2/1=a in (1.58), we deduce (1.57).Consider the integral, for 0>t ,
( ) ( ) ( )
++
=
+
+
=
0log
2
12log
2
1log
2
1log
22
11
1
1:,
a
tttttdu
u
ee
u
e
uetaF
tuuatu
u ,
(1.59)
where we applied (1.46) and (1.48). Upon the integration of (1.30), it is easily gleaned that, as
0t ,
( ) ttt loglog , (1.60)
where denotes Eulers constant. Using this in (1.59), we find, upon simplification, that, as 0t ,
( ) ( ) atttttaF log212log
21log, + . (1.61)
Hence,
( ) ( )ataFt
2log2
1,lim
0=
. (1.62)
Letting t approach 0 in (1.59), taking the limit under the integral sign on the right-hand side using
Lebesgues dominated convergence theorem, and employing (1.62), we immediately deduce (1.58).
As previously discussed, this is sufficient to prove the equality of the first and third expressions in
(1.42), namely,
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11
( )( )
= +
+
=
+
0 2
2
31 1
log2
1cos
4
1
2
11
2
2logdt
t
tit
tnn
. (1.63)
Lastly, using (1.63) with replaced by and employing the relation 1=
, we conclude that
( )( ) =
+
+
=
+
=
dtt
tit
tnn
2
2
031 1
log2
1cos
4
1
2
11
2
2log
( )=
+
+
=
dt
t
titt
2
2
03 1
/1log2
1cos
41
211
( )dt
t
tit
t2
2
03 1
log2
1cos
4
1
2
11
+
+
=
. (1.64)
Hence, the equality of the second and third expressions in (1.42) has been demonstrated, and so the
proof is complete.
2. On some Ramanujan-type series for /1 [2]
Ramanujans series representations for /1 depend upon Clausens product formulas forhypergeometric series and Ramanujans Eisenstein series
( )
= =
11241:
kk
k
q
kqqP , 1
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12
{ } ( )
=
+
+=0
2/12
2515542
k
k
kAk
, (2.2)
( ) ( )
=
+=0 4
13201
8
kkk
kBk
. (2.3)
For 13=n ,if kA and kB , 0k , are defined by the formula (2.1b), then
( ) ( )kk
k
kBk
20 18
1232601
72
=
+=
. (2.4)
The last two identities was recorded by Ramanujan in the fundamental paper Modular equations
and approximations to (1914).
Proof of (2.2).
From Ramanujans second notebook (Notebooks 2 volumes 1957), we see that
( ) ( ) ( ) ( ) ( )( ) ( )( ){ }
=
=
++=
+1 1
55522
10
10
2
2
11324
1
130
11
k kk
k
k
k
qxqxqxqxqqq
kq
q
kq
( ) ( ) ( )( ) ( )( ){ }2/1
55 111 qxqxqxqx ++ . (2.5)
With the help of (2.1) we can rewrite (2.4) in the form
( ) ( ) ( ) ( ) ( ) ( ) ( )( ) ( )( ){ }++= 55522210 1132
15 qxqxqxqxqqqPqP
( ) ( ) ( )( ) ( )( ){ }2/1
55 111 qxqxqxqx ++ . (2.6)
Now we set 5/= eq and use, following Ramanujan, the following expressions
nn xx /11 = , nn znz =/1 , (2.7)
( ) ( )qxFqzz 212 ;1;2
1,
2
1:: =
== , (2.8)
to deduce that ( ) 55/1 1 xxqx == , ( ) 55 xqx = , and ( ) ( ) 5
525/2 55 zee == .
Thus, from (2.6), we find that
( ) ( ) ( ){ } ( )( ) =++= 5555255/252 1212
112355 xxxxzePeP
( ){ } ( )( )555525 1412
11435 xxxxz ++= . (2.9)
The eq. (2.9), putting ( )555 14 xxX = , can be rewritten also as follows
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( ) ( ) ( ){ } ( )( ) =++= 5555255/252 1212
112355 xxxxzePeP
{ } ( )5525 12
135 XXz ++= . (2.9b)
But, the singular modulus 5x is given by
3
52
15
2
1
=x , (2.10)
so that
5495 =X and 255 =X . (2.11)
Thus, from (2.9), we find that
( ) ( ) ( ) 255/2522
151555 zePeP
+=
. (2.12)
Next, setting 5=n in the following equation
( ) ( )
nePenP
nn 6/22=+
, (2.13)
we find that
( ) ( )
565 5/252 =+ ePeP . (2.14)
Adding (2.12) and (2.14), we deduce that
( ) 25522
15
5
15
5
3zeP
++=
. (2.15)
Now, employing the following expression
=
=
=
0
23
2 ;1,1;2
1,
2
1,
2
1
k
k
kXAXFz ,2
10 x , (2.16)
in (2.15), we deduce the identity
( )
=
++=
0
5
52
2
15
5
15
5
3
k
k
kXAeP
. (2.17)
Next, setting 5=n in the following equation
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14
( ) ( ) ( )
=
+=
0
2 1321k
k
nkn
nXAkxeP
, (2.18)
we find that
( ) ( ) ( ) ( ) ( )
=
=
+=+=
0 0
555
52 132521321k k
k
k
k
k XAkXAkxeP . (2.19)
Using (2.17) and (2.19), we arrive at (2.2).
Proof of (2.3).
Employing the following expression
( )
=
=
=
0
22
23
2 121
1;1,1;
4
3,
2
1,
4
1
21
1
k
k
k
kWB
xWF
xz ,
2221
2
10 4/1x , (2.20)
in (2.15), we find that
( )( )
( ) ( )
=
=
++=
++=
0 0
2
5
2
5
5
52 154
53
5
31
2
15
215
15
5
3
k k
k
k
kk
k
kWBWB
xeP
, (2.21)
where
2
1
1
2
5
5
5 =
=X
XW . (2.22)
Next, setting 5=n in the following equation
( ) ( ) ( )
=
+++=
0
22
1
2/1131
k
k
nk
n
nnkn WBX
XXkeP
, (2.23)
we find that
( ) ( ) ( ) ( ) kkkk
k
n
k
k
n
nn WBkWBX
XXkeP
2
5
0
252 18
253
2
531
1
2/113
++=
+++=
=
. (2.24)
From (2.21) and (2.24), we readily arrive at (2.3). Thus, we complete the proof. The proof of (2.3b)
is similar.
2.1 On some equations concerning the p-adic open string for the scalar tachyon field. [3] [4]As a free action in p-adic field theory one can take the following functional
( ) =pQfDfdxfS (2.25)
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15
where ( )xff = is a function RQf p : , dx is the Haar measure and D is the Vladimirov
operator or its generalizations. Boundary value problems for homogeneous solutions of nonlinear
equations of motion corresponding to the p-adic string,
pe = . (2.26)
Here is the dAlembert operator and the field and its argument are real-valued.
The dynamics of the open p-adic string for the scalar tachyon field is described by the non-linear
pseudodifferential equation
pp =21
, (2.27)
where 22211
...
=dxxt
, 0xt= , is the dAlembert operator and p is a prime number,
,...5,3,2=p . In what follows p is any positive integer. We consider only real solutions of
equations (2.27), since only real solutions have physical meaning. In the one-dimensional case (d =
1) we use the change
( ) ( )ptt ln2=
and write equation (2.27) in the following equivalent form:
pte =2
2
1
. (2.28)
Equation (2.28) is a non-linear integral equation of the following form:
( ) ( ) ( )
= tde pt
21 , Rt . (2.29)
Solutions of equation (2.29) are sought in the class of measurable functions ( )t such that
( ) ( ){ }21exp tCt for any 0> , Rt . (2.30)
The following boundary-value problems for the solutions of equation (2.29) have physical
meaning:
( ) 0lim =
tt
, ( ) 1lim =
tt
(2.31)
ifp is even, and
( ) 1lim =
tt
, ( ) 1lim =
tt
(2.32)
ifp is odd.
Assertion 1
If is a solution of equation (2.29) such that
( ) att
=lim ,
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16
then 0=a or 1=a if p is even and 0=a or 1=a if p is odd, ( ) 0'lim = tp
t . If 0a ,
then ( ) 0'lim = tt .
We deduce from equation (2.29) the following chain of equalities:
( ) ( )[ ] ( ) ( ) ( )
=====
22 1lim
1limlimlim u
t
t
t
pp
t
p
teutdeatt
( )
== adueut u
t
2
lim1
, (2.34)
whence 0=a or 1=a ifp is even and 1,0 =a ifp is odd. Further, we have
( ) ( ) ( )( ) ( ) ( )
=== duueutdett u
t
t
t
p
t
22 1lim2
1lim2'lim
( )
===
= 00
22lim
2 22aduueaduueut uu
t
. (2.35)
If 0a , then ( ) 0'lim = tt , since
( ) ( ) ( ) ( ) ( ) 0'lim'lim'lim 11 ===
tpattpt
t
pp
t
p
t . (2.36)
We passed to the limit under the integral sign, using Lebesgues theorem and estimate (2.30). We
shall write ba if the integers a and b are both even or both odd, and ba if one of them iseven and the other is odd.
Hermite polynomials are defined to be the polynomials
( ) ( )22
1 xn
nxn
n edx
dexH
= , ,...,1,0=n (2.37)
whence ( ) 10 =xH , ( ) xxH 21 = , ( ) 242
2 = xxH , ( ) ,...1283
3 xxxH = . They form a complete
orthogonal system in the Hilbert space 12L , and
( ) ( )
== !21
22
1nxdxHH
n
nn . (2.38)
Any 12Lf can be expanded in Hermite polynomials:
( ) ( )( )
=
=0
1!2
,n
n
nn
n
xHHfxf in 12L , (2.39)
and the Parseval-Steklov equality holds:
( )
=
=0
2
1
2
1 !21,
nnn n
Hff . (2.40)
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17
The expansion in powers ofx has the form
( ) =
=n
nmm
m
mnn xcnxH0
,! , ,...,1,0=n (2.41)
In particular, we have
!
2,
nc
n
nn = ,( )
!
10,2
nc
n
n
= ,
( )!
121,12
nc
n
n
=+ ,
( )( )!1
122,2
=
nc
n
n ,( )
( )!1314
3,12
=+
nc
n
n . (2.42)
The integral representation for the modified Hermite polynomials has the form:
( ) ( ) ( )
=
deHxVt
nn
22/22 , ,...1,0=n . (2.43)
Let 2/12Lf . It follows from (2.28) that1
2Lf ,
( )( )
( )
=
=
==0 0 !!2n n
nnn
nn
n
xVbxf
n
xHa in 12L . (2.44)
We denote by K the linear integral operator in equation (2.29):
( )( ) ( ) ( )
detK t21
. (2.45)
Lemma 1
The operator K assigns to every function ( )t f satisfying condition (2.30) an entire function
( )( )zKf with the estimate
( )( )
+
22 11
exp tyC
zKf
, iytz += . (2.46)
The proof follows immediately from (2.30):
( )( ) ( ) ( )
+==
deeC
deeCzKf ttyt 21222221
+
22 11
exp tyC
. (2.47)
Lemma 2
The operator K assigns to2Lf , 20
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18
The proof follows from the Cauchy-Bunyakovskii inequality (applied to ( )( )zKf ) and the followingestimates:
( )( ) ( )
+
dzzefzKf
222/
2
12exp1 2
( ){ } ( ){ } =
+
+
2/1
222
2/1
22 2422exp1
242exp1
dttyfdtzf
( )
2/12
22
2
22exp
1
2exp
+=
dt
tyf . (2.49)
We can rewrite the above equation also as follows:
( )( ) ( ) =
+
dzzefzKf
222/
212exp
1 2
( )
2/12
22
2
22exp
1
2exp
+=
dt
tyf . (2.49b)
Lemma 3
The operator 22: LLK , 20
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19
If 12Lf , then its image ( )( )tKf can be expanded in the Taylor series
( )( )
=
=0 !n
n
nn
tatKf , ( )
1, nn Hfa = , (2.52)
which converges uniformly on every compact set in R . If 2/12Lf , then
( )( )( )
=
=0 !2n
n
nn
n
tHbtKf in
1
2L , ( )1, nn HKfb = , (2.53)
and
( ) ( ) ,,,2/11 nn
VfHKf = ,...1,0=n . (2.54)
By lemma 3, the function ( )( )tKf is the trace of an entire function ( )( )zKf for 0=y . Hence, it canbe expanded in the Taylor series with the coefficients
( )( ) ( ) ( ) ( )( ) ( ) ( )
=
=
= === 00022
111
tn
tn
t
t
n
n
tn
n
dtHefdedt
dftKf
dt
d
( )( ) ( ) ( ) nnt
n
naHfdeHf ===
1,1
1 2
. (2.55)
Here we used equality (2.37). Further, if 2/12Lf , then (2.53) holds by (2.44), since1
2LKf by
Lemma 3. Equalities (2.54) can be proved as follows:
( ) ( )2/12/11
,,, nnn VfHKfHKf == . (2.56)
Here we used formula (2.43), which implies that nn HKV
= , where K is the operator adjoint to
K.
Let be a solution of equation (2.29) belonging to 12L , whence Kp
= . Putting ( )1
, nn Ha = ,
we deduce from (2.39) and (2.40) that
( )( )
=
=
0
!2n
n
nn
n
tHat in 12L ,
=
=
0
22
!2n
n
n
n
a . (2.57)
The function ( )tp is the trace of the entire function ( ) ( )( )zKzA = , for which (2.48) holds with1= :
( )2
1
zezA , Cz . (2.58)
By Lemma 4, it can be expanded in the Taylor series (2.52):
( )
=
=0 !n
n
n
p
n
tat . (2.59)
The integral equation (2.29) is equivalent to the following boundary-value problem for the heat
equation:
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20
ttx uu4
1= , 10 x , Rt and, further, its
analytic continuation with respect to ( )tx, to the complex domain CT + , where +T is the righthalf-plane 0Re >=x .
Equation (2.29) takes the form
( ) ( ) ( )
=
det tq
212 , ,...2,1=q . (2.64)
If ( )t is a solution of equation (2.64), then ( )t and ( )0tt+ also are solutions of this equation
(for all 0t ).
Assertion 2
If ( )t is a solution of equation (2.64) such that (2.63) holds, then
( )( )
( )
+
12
121exp
124
112
2
2
xqx
qxxd
x
t
xq
q
q
q
(2.65)
for all ( )12/1 > qx .
We remember that if S is a measurable subset of Rn
with the Lebesgue measure, and and g are
measurable real- or complex-valued functions on S, then Hlder inequality is
( ) ( ) ( )( ) ( )( ) qS
qp
S
p
Sdxxgdxxfdxxgxf
/1/1
. (2.65b)
Denoting the left-hand side of inequality (2.65) by ( )txJ , , using the boundary conditions (2.61), theproperties of solutions of the heat equation and Holders inequality, we obtain the following chain
of relations for all ( )12/1 > qx :
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21
( ) ( )( )
( )( )
( )
+
+=
dx
t
xd
x
t
xtxJ
q
1exp
1
1exp
1,
22
2
( )( )
( ) ( ) ( )( )
=
+
+
d
qxx
xqxt
qx
t
x 21
12exp
2exp
1
122
( )[ ] ( ) ( )
( )( )
q
q dqxx
xqxtJt
x
2
11
2
2
1
121
12exp
1
1
+
+=
, (2.66)
whence
( )
( )
( )( ) qqqxqx
qxx
xx
xJ
2
11
4
1
2
11
12
121
1
+
+
, (2.67)
which implies that (2.65) holds.Now we can rewrite the eq. (2.65) also as follows:
( )
( )
( )( )
+
+
qqq
xqx
qxx
xx
xJ
2
11
4
1
2
11
12
121
1
( )( )
( )
+
12
121exp
124
112
2
2
xqx
qxxd
x
t
xq
q
q
q
. (2.67b)
Corollary
For 1=x estimate (2.65) with ,...3,2=q takes the form
( ) ( ){ }
22
122exp
1 241
22
q
qdt q
q
. (2.68)
With regard the possible mathematical connections, we note that it is possible to obtain some
interesting and new relationships evidencing some Ramanujans Theorems. The first letter of
Ramanujan to G. H. Hardy, contain the bare statements of about 120 theorems, mostly formal
identities extracted from his note-books. We take, for the connections regarding this section, the
following identities:
( )
( ) ( )
+
+
++
+
=
++
++
+
++
0 2
2
2
2
12
1
2
11
2
1
2...
11
21
1
11
abba
abba
dx
a
x
b
x
a
x
b
x
, (2.69)
( )( )( ) ( )
+++++=
+++0106324222 ...12
1...111
1rrrr
dxxrxrx
, (2.70)
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22
If 2 = , then
+=
+
0 2
4/1
0 2
4/1
141
141
22
dxe
xedx
e
xex
x
x
x
, (2.71)
5/242
2
15
2
55
...111
1
eee
+
+=
+++
, (2.72)
5/2
5
2/5
4/3
5452
2
15
12
1551
5
...111
1
eee
+
+
=+++
. (2.73)
We note that the eqs. (2.49b), (2.51b) and (2.68) can be related with the expression (2.69) and
(2.70). Indeed, we have:
( )( ) ( ) =
+
dzzefzKf
222/
212exp
1 2
( )
2/12
22
2
22exp
1
2
exp
+=
dt
tyf
( )
( ) ( )
+
+
++
+
=
++
++
+
++
0 2
2
2
2
12
1
2
11
2
1
2...
11
21
1
11
abba
abba
dx
a
x
b
x
a
x
b
x
, (2.74)
( )( ) ( ) =
+
dzzefzKf
222/
212exp
1 2
( )
2/12
22
222exp1
2exp
+=
dttyf
( )( )( ) ( )
+++++=
+++0106324222 ...12
1
...111
1
rrrrdx
xrxrx , (2.75)
( )( )
= dttKfeKf
t 22 2
( )
+
=
dedtef
t 22
22
42
21
( )
( ) ( )
+
+
++
+
=
+
+
++
+
++
0 2
2
2
2
12
1
2
11
2
1
2...
11
21
1
11
abba
abba
dx
a
x
b
x
a
x
b
x
, (2.76)
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23
( )( )
= dttKfeKf
t 22 2
( )
+
=
dedtef
t 22
22
42
21
( )( )( ) ( )
+++++
=
+++0 106324222
...12
1
...111
1
rrrr
dx
xrxrx
, (2.77)
( ) ( ){ }
22
122exp
1 241
22
q
qdt q
q
( )
( ) ( )
+
+
++
+
=
++
++
+
++
0 2
2
2
2
12
1
2
11
2
1
2...
11
21
1
11
abba
abba
dx
a
x
b
x
a
x
b
x
, (2.78)
( ) ( ){ }
22
122exp
1 24 122
q
qdt q
q
( )( )( ) ( )
+++++=
+++0106324222 ...12
1
...111
1
rrrrdx
xrxrx . (2.79)
3. On some equations concerning the zeta strings and the zeta nonlocal scalar fields [5]
The exact tree-level Lagrangian for effective scalar field which describes open p-adic string
tachyon is
++
=
+
12
2
2 1
1
2
1
1
1 pp
pp
p
p
g
L , (3.1)
where p is any prime number,22
+= t is the D-dimensional dAlambertian and we adopt
metric with signature ( )++ ... . Now, we want to show a model which incorporates the p-adicstring Lagrangians in a restricted adelic way. Let us take the following Lagrangian
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24
+
++=
==
1 1 1 1
1222 1
1
2
111
n n n n
n
nnnn
ngn
nCL
LL . (3.2)
Recall that the Riemann zeta function is defined as
( )
==1 1
11
n pss
pns , is += , 1> . (3.3)
Employing usual expansion for the logarithmic function and definition (3.3) we can rewrite (3.2) in
the form
( )
++
= 1ln
22
112
gL , (3.4)
where 1= 2220
2kkkr
, (3.5)
where ( ) ( ) ( )dxxek ikx
=~
is the Fourier transform of ( )x .
Dynamics of this field is encoded in the (pseudo)differential form of the Riemann zeta function.
When the dAlambertian is an argument of the Riemann zeta function we shall call such
string a zeta string. Consequently, the above is an open scalar zeta string. The equation of
motion for the zeta string is
( )( ) +> =
=
2
2
220 1
~
22
1
2 kkixk
Ddkk
ker
(3.6)
which has an evident solution 0= .
For the case of time dependent spatially homogeneous solutions, we have the following equation of
motion
( ) ( ) ( )
( )
( )tt
dkk
k
et ktikt
=
=
+>
1
~
22
1
2 00
2
0
2
2
0
0
. (3.7)
With regard the open and closed scalar zeta strings, the equations of motion are
( )( )
( )
=
=
n
n
nn
ixk
Ddkk
ke
1
2
12 ~
22
1
2
, (3.8)
( )( )
( )( )
( )
( )
+
+
+=
=
1
11
2
12
112
1~
42
1
4
2
n
n
nn
nixk
Dn
nndkk
ke
, (3.9)
and one can easily see trivial solution 0== .
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25
The exact tree-level Lagrangian of effective scalar field , which describes open p-adic string
tachyon, is:
+
+
=+
122
2
1
1
2
1
1
2pm
p
D
p
p
p
p
p
p
g
mp
L , (3.10)
where p is any prime number,22
+= t is the D-dimensional dAlambertian and we adopt
metric with signature ( )++ ... , as above. Now, we want to introduce a model which incorporatesall the above string Lagrangians (3.10) with p replaced by Nn . Thence, we take the sum of all
Lagrangians nL in the form
+
=
++
=
++
==
1
12
1
2
2 1
1
2
1
1
2
n
nm
n n
D
nnnn
nn
n
n
g
mCCL n
L , (3.11)
whose explicit realization depends on particular choice of coefficients nC , masses nm and coupling
constants ng .
Now, we consider the following case
hnn
nC
+
=
2
1, (3.12)
where h is a real number. The corresponding Lagrangian reads
+
+= +
=
++
=
1
1
1
22 12
1 2
n
nh
n
hm
D
hn
nn
g
mL
(3.13)
and it depends on parameter h . According to the Euler product formula one can write
+
=
=p
hmn
hm
p
n2
2
21
2
1
1
. (3.14)
Recall that standard definition of the Riemann zeta function is
( ) +
=
==
1 1
11
n pss
pns , is += , 1> , (3.15)
which has analytic continuation to the entire complex s plane, excluding the point 1=s , where it
has a simple pole with residue 1. Employing definition (3.15) we can rewrite (3.13) in the form
++
+=
+
=
+
1
1
22 122
1
n
nhD
hn
nh
mg
mL
. (3.16)
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26
Here
+ h
m22
acts as a pseudodifferential operator
( )
( )
( )dkkhm
kexh
m
ixk
D
~
22
1
22
2
2
+=
+
, (3.17)
where ( ) ( ) ( )dxxek ikx
=~
is the Fourier transform of ( )x .
We consider Lagrangian (3.16) with analytic continuations of the zeta function and the power series
+
+
1
1
nh
n
n , i.e.
++
+=
+
=
+
1
1
22 122
1
n
nhD
hn
nACh
mg
mL
, (3.18)
where AC denotes analytic continuation.Potential of the above zeta scalar field (3.18) is equal to hL at 0= , i.e.
( ) ( )
+=
+
=
+
1
12
2 12 n
nhD
hn
nACh
g
mV
, (3.19)
where 1h since ( ) =1 . The term with -function vanishes at ,...6,4,2 =h . The equationof motion in differential and integral form is
+
=
=
+
122 n
nhnAChm
, (3.20)
( )( )
+
=
=
+
12
2 ~
22
1
n
nh
R
ixk
DnACdkkh
m
ke
D
, (3.21)
respectively.
Now, we consider five values of h , which seem to be the most interesting, regarding the
Lagrangian (3.18): ,0=h ,1=h and 2=h . For 2=h , the corresponding equation of motion
now read:
( )
( )( )
( )
+=
=
DR
ixk
Ddkk
m
ke
m32
2
2
1
1~2
22
12
2
. (3.22)
This equation has two trivial solutions: ( ) 0=x and ( ) 1=x . Solution ( ) 1=x can be also
shown taking ( ) ( )( )Dkk 2~
= and ( ) 02 = in (3.22).For 1=h , the corresponding equation of motion is:
( )( )
( ) =
=
DR
ixk
Ddkk
m
ke
m22
2
21
~1
22
11
2
. (3.23)
where ( )12
11 = .
The equation of motion (3.23) has a constant trivial solution only for ( ) 0=x .For 0=h , the equation of motion is
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27
( )( ) =
=
D
R
ixk
Ddkk
m
ke
m
1
~
22
1
2 2
2
2
. (3.24)
It has two solutions: 0= and 3= . The solution 3= follows from the Taylor expansion of theRiemann zeta function operator
( )( )( )
+=
122 2!
00
2 n
nn
mnm
, (3.25)
as well as from ( ) ( ) ( )kk D 32~
= .
For 1=h , the equation of motion is:
( ) ( ) ( ) =
+DR
ixk
D dkkm
ke
2
2
2
1ln2
1~122
1
, (3.26)
where ( ) =1 gives ( ) =1V .In conclusion, for 2=h , we have the following equation of motion:
( )( )
( )
=
+
DR
ixk
Ddw
w
wdkk
m
ke
0
2
2
2
2
1ln~2
22
1. (3.27)
Since holds equality
( ) ( )
===
1
0 1 2211ln
n ndw
w
w
one has trivial solution 1= in (3.27).
Now, we want to analyze the following case:2
2 1
n
nCn
= . In this case, from the Lagrangian (3.11),
we obtain:
+
+
=
121
22
1 2
222mmg
mL
D
. (3.28)
The corresponding potential is:
( )( )
2
124
731
=
g
mV
D
. (3.29)
We note that 7 and 31 are prime natural numbers, i.e. 16 n with n =1 and 5, with 1 and 5 that are
Fibonaccis numbers. Furthermore, the number 24 is related to the Ramanujan function that has 24
modes that correspond to the physical vibrations of a bosonic string. Thence, we obtain:
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28
( )( )
2
124
731
=
g
mV
D ( )
++
+
42710
421110log
'
142
'
cosh
'cos
log42
'
'4
0
'
2
2
wtitwe
dxex
txw
anti
w
wt
wx
. (3.29b)
The equation of motion is:
( )[ ]( )2
2
221
11
21
2
+=
+
mm
. (3.30)
Its weak field approximation is:
022
12 22
=
+
mm
, (3.31)
which implies condition on the mass spectrum
22
12 2
2
2
2
=
+
m
M
m
M . (3.32)
From (3.32) it follows one solution for 02
>M at22
79.2 mM and many tachyon solutions when22 38mM < .
We note that the number 2.79 is connected with2
15 = and
2
15 += , i.e. the aurea section
and the aurea ratio. Indeed, we have that:
78,2772542,22
15
2
1
2
152
2
=
+
+.
Furthermore, we have also that:
( ) ( ) 79734,2179314566,0618033989,27/257/14 =+=+
4. Mathematical connections
We have the following new possible mathematical connections: between eqs. (1.7), (1.17) and
(1.19b) with eq. (3.6)
( ) ( ) ( )1
arctansin12
1
1
2
12
0
22
++
+=
t
s
e
dttst
s
s
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29
( )
( ) +> =
=
2
2
220 1
~
22
1
2 kkixk
Ddkk
ker
, (4.1)
( )
=
=0
22log1
1
1arctan20'
dt
e
tt
( )
( ) +> =
=
2
2
220 1
~
22
1
2 kkixk
Ddkk
ker
, (4.2)
( )
=
=
0 2 2879,0
1arccos2log1
1
1arctan20'
dt
et
t
( )
( ) +> =
=
2
2
220 1
~
22
1
2 kkixk
Ddkk
ker
. (4.3)
We have further possible mathematical connections between eqs. (1.56) and (1.64) with eq. (3.6):
=
=
+
+
0 0 /222
2
3 21
1
2
1
1
12
1
log2
1cos
4
1
2
11dt
tetedt
t
tit
ttt
( )( ) ( ) ( )
+
+
=
0 2/222/2 21
1
111
/2dt
teteteetttt
( )
( ) +>
=
=
2
2
22
0 1
~
22
1
2kk
ixk
Ddkk
ker
, (4.4)
( )( ) =
+
+
=
+
=
dtt
tit
tnn
2
2
031 1
log2
1cos
4
1
2
11
2
2log
( )dt
t
tit
t2
2
03 1
log2
1cos
4
1
2
11
+
+
=
( )( )
+>
=
=
2
2
220 1
~
22
1
2 kk
ixk
D
dkkk
er
, (4.5)
With regard , we have these possible mathematical connections between eqs (4.4) and (4.5) with
some Ramanujans equations ((2.69) and (2.70)). Indeed:
=
=
+
+
0 0 /222
2
3 21
1
2
1
1
12
1
log2
1cos
4
1
2
11dt
tetedt
t
tit
ttt
( )( ) ( ) ( )
+
+
=
02/222/2
21
1
111
/2dt
teteteetttt
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30
( )
( ) +> =
=
2
2
220 1
~
22
1
2 kkixk
Ddkk
ker
( )
( ) ( )
+
+
++
+
=
+
+
++
+
++
0 2
2
2
2
12
1
2
11
2
1
2...
11
21
1
11
abba
abba
dx
a
x
b
x
a
x
b
x
, (4.6)
=
=
+
+
0 0 /222
2
3 21
1
2
1
1
12
1
log2
1cos
4
1
2
11dt
tetedt
t
tit
ttt
( )( ) ( ) ( )
+
+
=
0 2/222/2 21
1
111
/2dt
teteteetttt
( )
( ) +> =
=
2
2
220 1
~22
12 kk
ixkD
dkkker
( )( )( ) ( )
+++++=
+++0106324222 ...12
1
...111
1
rrrrdx
xrxrx . (4.7)
We have also some possible mathematical connections with the eqs. (1.19b), (1.34), (1.36) and eq.
(3.6). Indeed:
( )
=
=
0 2 2879,0
1arccos2log1
1
1arctan20'
dt
et
t
( ) ( )
( )( ) ==
q
uddt
t
tftf
0
2/
cos 22/35
5224/3
2/51
sin51
125
( ) ( )( )( ) ( )( )
=
=
qfqfq qqq
dd3534/31 54/11/5tan2
0
/5tan2
0 22/122/35 sin51
15
sin51
1
( )
( ) +> =
=
2
2
220 1
~
22
1
2 kkixk
Ddkk
ker
, (4.8)
( )
== 0
2 2879,0
1arccos2log11
1arctan20' dtet t
( ) ( ) ( ) ( )( )
=
=
+
q
vv
vv ddttftftftf0
5/1tan2
1
111
5
1tan2
2
15531
2
21
sin25
91
1
5
1
( ) ( )( )( )( )
( )( )( )
( )( )
+
+
+
++
=
=2/
11
11
1
1tan2
53tan
11
1153tan
2251
5
3
31
1
5
511
sin16
151
1
4
1
sin81
11
1
9
1
vvvv
v
v
vv
vv dd
( )
( ) +>
=
=
2
2
22
0 1
~
22
1
2kk
ixk
Ddkk
ker
. (4.9)
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31
In conclusion, we have also some possible mathematical connections between the eqs. (1.32) and
(1.39) with the following equation
++
+=
4
2710
4
21110log
142
8
3
, related to
and with the physical vibrations of the superstrings. Thence, we have:
( )( )
( ) ( )( )
+
++=
2
232
5
5
251
251log5log
5
8
uv
uvvu
q
dq
q
q
++
+=
4
2710
4
21110log
142
8
3
, (4.10)
( ) ( ) ( ) ( )
++
=q c
x
xc
ddttftftftf0
cos
1221
221cos
2
4/714721
1
sin64
213321
12
++
+=
4
2710
4
21110log
142
8
3
. (4.11)
Acknowledgments
I would like to thank Prof. Branko Dragovich of Institute of Physics of Belgrade (Serbia) for his
availability, useful discussion and friendship
References
[1] Bruce C. Berndt and Atul Dixit Transformation formula involving the gamma and
Riemann zeta functions in Ramanujans lost notebook H98230-07-01-0088
[2] Nayandeep Deka Baruah and Bruce C. Berndt Eisenstein series and Ramanujan-type
Series for1/ Math. Reviews Class.N: 33C05, 33E05, 11F11, 11R29
[3] B. Dragovich, A. Yu. Khrennikov, S. V. Kozyrev and I. V. volovich On p-adic
8/8/2019 On some mathematical equations concerning the functions zeta(s) and zeta(s,w) and some Ramanujan-type series
32/32
Mathematical Physics arXiv:0904.4205v1 Apr 2009
[4] V. S. Vladimirov On the equation of the p-adic open string for the scalar tachyon field
arXiv:math-ph/0507018v1 Jul 2005
[5] Branko Dragovich: Zeta Strings arXiv:hep-th/0703008v1 1 Mar 2007.