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An Approximation to Riemann Hypothesis

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08 October 2025

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09 October 2025

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Abstract
In the previous version, there was possibly a issue that in Lemma 2.2 the integrant \( |\zeta(s)|^2 \) should be rewritten as \( \zeta(s)\zeta(2a-s) \) when the integral path is moved from \( (a) \) to \( (c) \), which has been revised accordingly.
Keywords: 
;  

1. Introduction

Riemann zeta-function ζ ( s ) is originally defined as
ζ ( s ) = n = 1 1 n s , for Re s > 1 .
and it also can be expressed as the product form
ζ ( s ) = p 1 1 1 / p s , for Re s > 1 .
This formula is called Euler’s product formula, which indicates the relation between ζ ( s ) and prime numbers. About ζ ( s ) there is a well-known Riemann hypothesis, states that all the non-trivial zeros of ζ ( s ) are on the critical line Re s = 1 / 2 . The researches on the conjecture are no doubt a most time-consuming one in mathematics, refer to see the survey paper [3].
The so-called trivial zeros of ζ ( s ) are s = 2 , 4 , , and nontrivial zeros of ζ ( s ) are known all in the critical strip 0 Re s 1 .
Denote by N ( T ) the number of zeros of ζ ( σ + i t ) in the region 0 σ 1 , 0 t T , and by N 0 ( T ) the number of zeros on the critical line σ = 1 / 2 , 0 t T . Riemann hypothesis is that
N 0 ( T ) = N ( T ) .
For N ( T ) , it is known that
N ( T ) = T 2 π log T 2 π T 2 π + O ( log T ) .
And for N 0 ( T ) , Hardy firstly shown that there are infinity many zeros on the critical line, and then he and Littlewood [5] and Selberg [8] proved that
κ = N 0 ( T ) N ( T ) > 0 .
Levinson [6] proved
κ 1 3 .
and then this result has been improved successively. Conrey [2], Feng [4] proved respectively
κ 0.407 , κ 0.412 .
In this paper, we will prove that
Theorem 1.1.
N ( T ) = N 0 ( T ) + E .
where E T 1 / 2 ( log T ) 2 .
The main arguments in this paper are based the papers [6],[7] and [1], but instead of using Riemann-Siegel formula, it will be applied an auxiliary function ω ( s , T 1 , T 2 ) defined in Lemma 2.1, which will play a role of mollifier and ferry, it firstly used in [7] but here with a small modification.
In the prior version, possibly there was a issue that in Lemma 2.2 the integrant | ζ ( s ) | 2 should be rewritten as ζ ( s ) ζ ( 2 a s ) when the integral path is moved from ( a ) to ( c ) , which has been revised in this version.

2. Some Lemmas

In the following, it will be used an auxiliary function ω ( s , T 1 , T 2 ) , which defined as following.
Suppose that T T 1 T 2 2 T , λ = T 1 ϵ , for any ϵ > 0 , s 1 = λ + c + i u , ( c 0 ) , s = v + i t , define
g ( w ) = e λ Γ ( w ) λ w ,
and
ω ( s , T 1 , T 2 ) = 1 2 π T 1 T 2 g ( s 1 s ) d u .
Lemma 1.
Let σ = λ + c v , η = min | x t | | x [ T 1 , T 2 ] , there is
| ω ( s , T 1 , T 2 ) | exp ( ( ( c v ) 2 + η 2 ) / 2 σ )
Suppose Δ Δ 0 ( = ( 2 β λ log T ) 1 / 2 , β > 0 ) , if t [ T 1 + Δ , T 2 Δ ] , then
| ω ( c + i t , T 1 , T 2 ) 1 | T β .
And if t T 1 Δ , or t T 2 + Δ , then
| ω ( c + i t , T 1 , T 2 ) | T β .
If | t u | = o ( σ 2 / 3 ) , then
arg g ( s 1 s ) = t u 2 σ ( t u ) 3 6 σ 2 c ( t u ) σ + O 1 σ .
Proof. 
By Stirling’s formula, it has
Re ( log Γ ( σ + ( u t ) i ) ) = σ 1 2 log ( σ 2 + ( u t ) 2 ) 2 σ + 1 2 log ( 2 π ) ( u t ) arctan u t σ + O 1 σ
And
Re ( log ( Γ ( σ + ( u t ) i ) ) ) + Re ( log ( λ ( σ + ( u t ) i ) ) ) + λ = ( c v ) 2 2 σ ( u t ) 2 4 σ 2 ( u t ) 2 2 σ 1 2 log σ + 1 2 log ( 2 π ) + O 1 σ
Hence,
| ω ( s , T 1 , T 2 ) | e ( c v ) 2 / 2 σ 1 2 π σ T 1 T 2 e ( u t ) 2 / 2 σ d u e ( ( c v ) 2 + η 2 ) / 2 σ .
Besides, it is familiar that
e λ = 1 2 π i ( c ) Γ ( s 1 s ) λ s s 1 d s .
Hence,
1 ω ( c + i t , T 1 , T 2 ) = R 1 + R 2 ,
where
R 1 = e λ 2 π T 2 Γ ( λ + ( u t ) i ) λ ( λ + ( u t ) i ) d u ,
R 2 = e λ 2 π T 1 Γ ( λ + ( u t ) i ) λ ( λ + ( u t ) i ) d u ,
Hence, if t [ T 1 + Δ , T 2 Δ ] , then
R 1 T 2 e λ Γ ( λ + ( u t ) i ) λ ( λ + ( u t ) i ) d u λ 1 / 2 T 2 exp ( ( u t ) 2 / 2 λ ) d u T β .
and similarly,
R 2 λ 1 / 2 T 1 exp ( ( u t ) 2 / 2 λ ) d u T β .
if t T 1 Δ , or t T 2 + Δ , then
ω ( c + i t , T 1 , T 2 ) λ 1 / 2 T 1 T 2 exp ( ( u t ) 2 / 2 λ ) d u T β .
If | t u | = o ( σ 2 / 3 ) , then
I m ( log ( Γ ( s 1 s ) λ s s 1 ) ) = t u 2 σ + ( t u ) 3 3 σ 2 ( t u ) 3 2 σ 2 c ( t u ) σ + O 1 σ = t u 2 σ ( t u ) 3 6 σ 2 c ( t u ) σ + O 1 σ .
Lemma 2.
Let L = log ( T / 2 π ) , G 0 ( s ) = ζ ( s ) + ζ ( s ) / L , and 0 < a 1 / 2 , 1 < b < β 1 , u [ T 1 , T 2 ] , s 1 = λ + c + i u , then
1 2 π i a + ( u Δ ) i a + ( u + Δ ) i g ( s 1 s ) G 0 ( s ) G 0 ( 2 a s ) d s = 1 2 π i b + ( u Δ ) i b + ( u + Δ ) i g ( s 1 s ) G 0 ( s ) G 0 ( 2 a s ) d s + O ( b / T )
Proof. 
Let B be the rectangle with vertices a + ( u Δ ) i , a + ( u + Δ ) i , b + ( u Δ ) i and b + ( u + Δ ) i . Take the integral B g ( s 1 s ) G ( s ) G ( 2 a s ) d s , with the residue theorem, it has
1 2 π i b + ( u Δ ) i b + ( u + Δ ) i g ( s 1 s ) G 0 ( s ) G 0 ( 2 a s ) d s = 1 2 π i a + ( u Δ ) i a + ( u + Δ ) i g ( s 1 s ) G 0 ( s ) G 0 ( 2 a s ) d s + 1 2 π i a + ( u + Δ ) i b + ( u + Δ ) i g ( s 1 s ) G 0 ( s ) G 0 ( 2 a s ) d s + 1 2 π i b + ( u Δ ) i a + ( u Δ ) i g ( s 1 s ) G 0 ( s ) G 0 ( 2 a s ) d s + R
where R is the residue at the pole s = 1 , which is easy to know
R g ( λ + c 1 + i u ) O ( e c ) .
On the upper side and the lower side, as | Im ( s 1 s ) | = Δ , by Lemma 2.1, it has
| g ( s 1 s ) | 1 / T β
Besides, by the functional equation, it is easy to know
| G ( v + ( u ± Δ ) i ) G ( 2 a ( v + ( u ± Δ ) i ) ) | T b , ( a v b ) .
Hence, the two integrals on the upper side and the lower side of B
1 2 π i a + ( u ± Δ ) i b + ( u ± Δ ) i g ( s 1 s ) G 0 ( s ) G 0 ( 2 a s ) d s b / T ,
and the Lemma is followed.
Lemma 3.
Suppose that 0 < α < β 2 . For r > 0 , let
J ( r ) = 1 2 π T 1 T 2 u Δ u + Δ t 2 π α e ( t u ) 2 / 2 σ exp i t log t r e c ( t u ) i σ d t d u
Then for T 1 Δ r T 2 + Δ ,
J ( r ) r 2 π α r 1 / 2 σ 1 / 2 e π i / 4 .
And if r < T 1 Δ , or r > T 2 + Δ , and Δ Δ 0 T ϵ , then
J ( r ) = O ( 1 ) .
Proof. 
Denote by
F ( u ) = u Δ u + Δ t 2 π α e ( t u ) 2 / 2 σ exp i t log t r e c ( t u ) i σ d t
And let t = u ( 1 + x ) ,then
F ( u ) = u 2 π α u e i u ρ F 1 ( u ) ,
where ρ = log ( u / r ) 1 ,
F 1 ( u ) = Δ / u Δ / u exp A ( x ) + B ( x ) i d x ,
A ( x ) = α log ( 1 + x ) ( u x ) 2 / 2 σ , B ( x ) = u ( 1 + x ) log ( 1 + x ) + u x ρ c u x / σ .
By Gauss’s integration, it is easy to follow
F 1 ( u ) 1 u 2 π σ 1 + α σ / u 2 i σ / u exp ( 1 + ρ c / σ i α / u ) 2 u 2 ( u / σ + α / u i )
and
F ( u ) u 2 π α e i u ρ 2 π σ 1 + α σ / u 2 i σ / u exp ( log ( u / r ) c / σ i α / u ) 2 σ 2 ( 1 + α σ / u 2 i σ / u )
If r [ T 1 Δ , T 2 + Δ ] , let u = r ( 1 + x ) , then
F ( u ) r 2 π α 2 π σ exp x 2 ( σ r i ) 2 ( 1 + x ) α
and
1 2 π T 1 / r 1 T 2 / r 1 F ( u ) r d x r 2 π r 2 π α 2 π σ · π ( σ + α r i ) / 2 exp α 2 ( σ + α + r i ) 2 ( σ + α ) 2 + r 2 ) r 2 π α r 1 / 2 σ e π i / 4
If r < T 1 Δ , or r > T 2 + Δ , and if Δ Δ 0 T ϵ , then
| F ( u ) | T α + 1 / 2 exp Δ T c σ 2 σ 2 T α + 1 / 2 β O ( 1 / T ) .

3. The Proof of Theorem 1.1

Proof. 
Let h ( s ) = π s / 2 Γ ( s / 2 ) , then the functional equation of ζ ( s ) can be written as
h ( s ) ζ ( s ) = h ( 1 s ) ζ ( 1 s )
By Stirling’s formula, it has
log h ( s ) = 1 2 ( s 1 ) log s 2 π s 2 + C 0 + O 1 s
Let f ( s ) = log h ( s ) , then
f ( s ) = h ( s ) h ( s ) = 1 2 log s 2 π + O 1 s
and for larger t
f ( s ) + f ( 1 s ) = log t 2 π + O 1 s
Taking logarithm of equation (3.1), and then derivative, it follows
h ( s ) ζ ( s ) ( f ( s ) + f ( 1 s ) ) = h ( s ) ζ ( s ) h ( 1 s ) ζ ( 1 s )
We note that the right side of (3.5) is a sum of two conjugative complex numbers as s = 1 / 2 + i t , so the zeros of the right side of (3.5) occur if and only if
arg ( h ( s ) ζ ( s ) ) π / 2 mod π
On the left side of (3.5), clearly, h ( s ) is never zero, and by (3.4), so these zeros are just the zeros of ζ ( 1 / 2 + i t ) .
Moreover, let χ ( s ) = h ( 1 s ) / h ( s ) , then ζ ( s ) = χ ( s ) ζ ( 1 s ) , and
ζ ( s ) = χ ( s ) { ( f ( s ) + f ( 1 s ) ) ζ ( 1 s ) + ζ ( 1 s ) }
By (3.6), the zeros of ζ ( 1 / 2 + i t ) are the ones
arg ( h ( 1 s ) { ( f ( s ) + f ( 1 s ) ) ζ ( 1 s ) + ζ ( 1 s ) } ) π / 2 mod π
on σ = 1 / 2 , equivalently,
arg ( h ( s ) { ( f ( s ) + f ( 1 s ) ) ζ ( s ) + ζ ( s ) } ) π / 2 mod π
on σ = 1 / 2 . Write L ( s ) = f ( s ) + f ( 1 s ) , and denote by
G ( s ) = ζ ( s ) + ζ ( s ) / L ( s )
The investigation above means
N 0 ( T ) = 1 π Δ 0 T arg ( h G ( 1 / 2 + i t ) )
By(3.2), it can be known that
Δ 0 T arg ( h ( 1 / 2 + i t ) ) = T 2 log T 2 π T 2 + O ( log T )
So, the main task to determine N 0 ( T ) is to calculate Δ 0 T arg ( G ( 1 / 2 + i t ) ) . Let L = log ( T / 2 π ) , U T , and let D be the rectangle with the vertices 1 / 2 + i T , c + i T , c + i ( T + U ) , 1 / 2 + i ( T + U ) , ( c 3 ) . First of all, we might as well assume there are no zeros of G ( s ) on the boundary of D, then by the principle of argument, the change of arg G ( s ) around D is equal to 2 π times N G ( D ) , the number of zeros of G ( s ) in D.
On the right side of D
| G ( c + i t ) 1 | n 2 n c + O ( 1 / L ) 1 / 3
so, arg G ( s ) change less than π . On the lower side and the upper side of D, by a known result [9, § 9.4 ], a extension of Jessen’s theorem, taking account on the order of G ( s ) , we can know that arg G ( s ) = O ( L ) as 0 < σ 3 , and arg G ( σ + i t ) = O ( 2 σ ) as σ 3 , hence, for any 0 b c , it has
b c arg G ( σ + i T ) d σ , b c arg G ( σ + i ( T + U ) ) d σ O ( L )
So,
Δ T T + U arg ( G ( 1 / 2 + i t ) ) = 2 π N G ( D ) + O ( log T )
Now the work is turned into to evaluate N G ( D ) .
Let 1 / 2 a = O ( 1 / L ) , and C be the rectangle with vertices a + i T , c + i T , c + i ( T + U ) , a + i ( T + U ) . Taking the integral C log G ( s ) d s , by the Littlewood’s Lemma [9, § 9.9 ], it has
T T + U log | G ( a + i t ) | d t T T + U log | G ( c + i t ) | d t + a c arg G ( σ + i ( T + U ) ) d σ a c arg G ( σ + i T ) d σ = 2 π dist
where dist is the sum of the distances of the zeros of G ( s ) from the left.
By (3.9), it is easy to know
T T + U log G ( c + i t ) d t = T T + U log ζ ( c + i t ) d t + O ( 1 / L )
and it is familiar that
log ζ ( s ) = n Λ ( n ) n s log n
So
T T + U log | G ( c + i t ) | d t 1 .
With (3.12), the rest is to calculate the first integral of (3.14).
By the concavity of logarithm, it has
T T + U log | G ( a + i t ) | d t = 1 2 T T + U log | G ( a + i t ) | 2 d t 1 2 U log 1 U T T + U | G ( a + i t ) | 2 d t
At first, we simplify G ( s ) as
G 0 ( s ) = ζ ( s ) + ζ ( s ) L .
Then
G ( s ) = G 0 ( s ) + E ( s ) .
E ( s ) = 1 L ( s ) 1 L ζ ( s ) 1 L 3 ζ ( s ) .
And
T 1 T 2 | G ( a + i t ) | 2 d t = T 1 T 2 | G 0 ( a + i t ) | 2 d t + 2 Re T 1 T 2 G 0 ( a + i t ) E ( a i t ) d t + T 1 T 2 | E ( a + i t ) | 2 d t
By Cauchy’s inequality
T 1 T 2 G 0 ( a + i t ) E ( a i t ) d t T 1 T 2 | G 0 ( a + i t ) | 2 d t T 1 T 2 | E ( a + i t ) | 2 d t 1 / 2
The third integral in the right side of (3.16) is much smaller than the first one, which will be actually calculated later, hence
T 1 T 2 | G ( a + i t ) | 2 d t = ( 1 + ϵ ) T 1 T 2 | G 0 ( a + i t ) | 2 d t .
Let
ω 1 ( s ) = 1 2 π i | u t | Δ g ( s 1 s ) d s 1 .
From Lemma 2.1, it is known that ω 1 ( s ) is the domination of ω ( s , T 1 , T 2 ) , and which is a positive real number apart from a small error term.
Moreover, let
ϕ ( s ) = ω 1 1 / 2 ( s ) .
Then it has
arg ϕ ( v + T 1 i ) = o ( 1 ) , arg ϕ ( v + T 2 i ) = o ( 1 ) .
And
a c arg ϕ ( v + T 1 i ) d v o ( c ) , a c arg ϕ ( v + T 2 i ) d v o ( c ) .
Moreover, by Lemma 2.1, there is
T 1 T 2 log | ϕ ( c + i t ) | d t T b .
(3.19) and (3.20) indicate that function ϕ ( s ) may be used as a mollifier.
Let
G ( s ) = G 0 ( s ) ϕ ( s ) .
In the following we will replace G ( s ) by G ( s ) , and let
I = T 1 T 2 | G ( s ) | 2 d t
Then,
I = T 1 T 2 | G 0 ( s ) | 2 ω 1 ( s ) d t = 1 2 π T 1 T 2 t Δ t + Δ g ( s 1 s ) d u | G 0 ( a + i t ) | 2 d t = 1 2 π T 1 T 2 u Δ u + Δ g ( s 1 s ) | G 0 ( a + i t ) | 2 d t d u + R 1 + R 2 R 3 R 4
where
R 1 = 1 2 π T 1 T 1 + Δ u Δ T 1 g ( s 1 s ) d u | G 0 ( a + i t ) | 2 d t , R 2 = 1 2 π T 2 Δ T 2 u + Δ T 1 g ( s 1 s ) d u | G 0 ( a + i t ) | 2 d t , R 3 = 1 2 π T 1 Δ T 1 T 1 u + Δ g ( s 1 s ) d u | G 0 ( a + i t ) | 2 d t , R 4 = 1 2 π T 2 T 2 + Δ u Δ T 2 g ( s 1 s ) d u | G 0 ( a + i t ) | 2 d t .
By the mean-value theorems (cf. [9, Ch.7]), it has
R 1 T 1 T 1 + Δ | G 0 ( a + i t ) | 2 d t Δ L ,
similarly,
R i Δ L , i = 2 , 3 , 4 .
Then, by Lemma 2.2, it has
I = 1 2 π i T 1 T 2 b + ( u Δ ) i b + ( u + Δ ) i g ( s 1 s ) G ( s ) G ( 2 a s ) d s + O ( Δ L )
Moreover, by the functional equation of ζ ( z ) , it has
ζ ( 2 a ( b + i t ) ) = χ ( 2 a ( b + i t ) ) ζ ( 1 + b 2 a i t )
ζ ( 2 a ( b + i t ) ) = χ ( 2 a ( b + i t ) ) ( L ζ ( 1 + b 2 a + i t ) ) + ζ ( 1 + b 2 a + i t ) )
and
G ( 2 a ( b + i t ) ) = χ ( 2 a ( b + i t ) ) ζ ( 1 + b 2 a + i t ) L
and it is easy to know
χ ( 2 a ( b + i t ) ) = t 1 / 2 + b 2 a exp π i 4 + i t log t 2 π e
Hence,
I = I 1 + I 2 + O ( Δ L ) .
where
I 1 = 1 2 π T 1 T 2 u Δ u + Δ g ( s 1 s ) χ ( 2 a ( b + i t ) ) ζ ( b + i t ) ζ ( 1 + b 2 a + i t ) L d t d u
I 2 = 1 2 π T 1 T 2 u Δ u + Δ g ( s 1 s ) χ ( 2 a ( b + i t ) ) ζ ( b + i t ) L ζ ( 1 + b 2 a + i t ) L d t d u
Expanding ζ ( s ) and ζ ( s ) as Dirichlet’s series, and by the Lemma 2.1, it has
I 1 = e ( c b ) 2 2 σ 1 L y 1 log y y b x 1 1 x b J ( 2 π x y ) , I 2 = e ( c b ) 2 2 σ 1 L 2 y 1 log y y b x 1 log x x b J ( 2 π x y ) .
where b = b + 1 2 a , and J ( r ) is same as in Lemma 2.3.
Dividing I 1 and I 2 into three parts respectively,
I 1 = I 1 , 1 + I 1 , 2 + I 1 , 3 = 2 π x y < T 1 Δ + T 1 Δ 2 π x y T 2 + Δ + 2 π x y > T 2 + Δ ,
I 2 = I 2 , 1 + I 2 , 2 + I 2 , 3 = 2 π x y < T 1 Δ + T 1 Δ 2 π x y T 2 + Δ + 2 π x y > T 2 + Δ .
Then by Lemmas 1,2,3,1
I 1 , 1 1 L 2 π x y T 1 Δ log y x b y b = o ( 1 ) I 1 , 3 1 L 2 π x y > T 2 + Δ log y x b y b = o ( 1 ) I 2 , 1 1 L 2 2 π x y T 1 Δ log x log y x b y b = o ( 1 ) I 2 , 3 1 L 2 2 π x y > T 2 + Δ log x log y x b y b = o ( 1 )
and
I 1 , 2 = e ( c b ) 2 2 σ 1 L T 1 Δ 2 π x y T 2 + Δ x 1 2 a log y , I 2 , 2 = e ( c b ) 2 2 σ 1 L 2 T 1 Δ 2 π x y T 2 + Δ x 1 2 a log x log y .
Let
H ( n ) = 1 L 1 x y n x 1 2 a log y 1 L 2 1 x y n x 1 2 a log x log y
It is easy to follow that
H ( n ) n L 2 ( 1 a ) n 1 2 a ( 1 2 a ) 3 log 2 n 2 ( 1 2 a ) log n ( 1 2 a ) 2 1 ( 1 2 a ) 3
Let 1 2 a = 1 / L , then
H ( n ) ( e 2.5 ) n L
Take c = b + ( 2 σ log ( ( e 2.5 ) L / 2 π ) ) 1 / 2 , T 1 = T , T 2 = T + U , then it has
I = U + O ( Δ )
and
T T + U | G ( a + i t ) | 2 d t = U + O ( Δ ) .
Let U = T , by (3.15), it follows
T T + U log | G ( a + i t ) | d t T 2 log 1 + O ( Δ ) T O ( Δ ) .
With (3.12), (3.14), (3.19),(3.20) and (3.23), and recall that a = 1 / 2 1 / L , it follows
2 π N G ( D ) O ( Δ ) 1 / 2 a T 1 / 2 L 2 .
i.e.
Δ 2 T T arg G ( 1 / 2 + i t ) O ( T 1 / 2 L 2 ) .
and
( N ( 2 T ) N ( T ) ) ( N 0 ( 2 T ) N 0 ( T ) ) O ( T 1 / 2 L 2 ) .
Then let T be T / 2 k , 1 k log 2 ( T ) , and summing. This proves Theorem 1.1 in the case that there are no zeros of G ( s ) on the boundary of D.
For the rest case, let N 1 and N 2 be the numbers of zeros of G ( s ) on the left side of D, σ = 1 / 2 , and in D with σ > 1 / 2 , respectively. Indent the left side of D with small semicircles with centers at the zeros and lying in σ 1 / 2 . Let N 1 be the number of distinct zeros in the N 1 zeros. Let V j be the variation in arg G in the jth interval between the successive semicircles. Then by the principle of argument, it has
j V j π N 1 = 2 π N 2 + O ( L ) ,
Let W j be the variation of argument of
h ( s ) ( f ( s ) + f ( 1 s ) ) G ( s )
in the jth interval, where W j is taken for increasing t, while V j is taken for decreasing t. With (3.2) and (3.24), it has
j W j = Im ( f ) | T T + U j V j = Im ( f ) | T T + U ( 2 π N 2 + π N 1 ) + O ( L )
By (3.8), in the jth open interval, the number of zeros of ζ ( 1 / 2 + i t ) is at least
( W j / π ) 1 .
and in all the open intervals, the number of zeros is at least
1 π j W j N 1 1 = 1 π Im ( f ) | T T + U ( 2 N 2 + N 1 ) N 1 1 + O ( L ) = 1 π Im ( f ) | T T + U 2 N G ( D ) + N 1 N 1 + O ( L )
Moreover, by (3.7), we can know that on the side σ = 1 / 2 , a zero of G ( s ) is also a zero of ζ ( s ) , and so a zero of ζ ( s ) , with multiplicity one greater, so there are N 1 + N 1 such zeros of ζ ( 1 / 2 + i t ) , adding to (3.26), in total, it has
N 0 ( T + U ) N 0 ( T ) 1 π Im ( f ) | T T + U 2 N G ( D ) + 2 N 1 + O ( L ) .
By (3.11), we can know
1 π Im ( f ) | T T + U = N ( T + U ) N ( T ) + O ( L ) .
i.e.
( N ( T + U ) N ( T ) ) ( N 0 ( T + U ) N 0 ( T ) ) O ( T 1 / 2 L 2 ) .
Besides, we know that on the critical line a zero of G ( s ) is also a zero of ζ ( s ) , and so a zero of ζ ( s ) , with multiplicity one greater. Hence
( m 1 ) N G ( D ) .
where sum is over the distinct zeros of ζ ( s ) on the left side of D, m is the multiplicity of a zero.
And so,
m 2 m 2 N G ( D ) O ( T 1 / 2 L 2 ) .
This means that the non-trivial zeros of ζ ( s ) are all on the critical line, and all are simple, with at most O ( T 1 / 2 L 2 ) ones excepted.

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1
In Lemma 2.3, for the simplicity, arg ( f ) is only taken c ( u t ) / σ
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