arb/doc/source/acb_dirichlet.rst

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.. _acb-dirichlet:
**acb_dirichlet.h** -- Dirichlet L-functions, zeta functions, and related functions
===================================================================================
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*Warning: the interfaces in this module are experimental and may change
without notice.*
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This module allows working with values of Dirichlet characters, Dirichlet L-functions,
and related functions. Working with Dirichlet characters is documented in
:ref:`dirichlet`.
A Dirichlet L-function is the analytic continuation of an L-series
.. math ::
L(s,\chi) = \sum_{k=1}^\infty \frac{\chi(k)}{k^s}
where `\chi(k)` is a Dirichlet character.
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The code in other modules for computing the Riemann zeta function,
Hurwitz zeta function and polylogarithm will possibly be migrated to this
module in the future.
Roots of unity
-------------------------------------------------------------------------------
.. type:: acb_dirichlet_roots_struct
.. type:: acb_dirichlet_roots_t
.. function:: void acb_dirichlet_roots_init(acb_dirichlet_roots_t roots, ulong n, slong num, slong prec)
Initializes *roots* with precomputed data for fast evaluation of roots of
unity `e^{2\pi i k/n}` of a fixed order *n*. The precomputation is
optimized for *num* evaluations.
For very small *num*, only the single root `e^{2\pi i/n}` will be
precomputed, which can then be raised to a power. For small *prec*
and large *n*, this method might even skip precomputing this single root
if it estimates that evaluating roots of unity from scratch will be faster
than powering.
If *num* is large enough, the whole set of roots in the first quadrant
will be precomputed at once. However, this is automatically avoided for
large *n* if too much memory would be used. For intermediate *num*,
baby-step giant-step tables are computed.
.. function:: void acb_dirichlet_roots_clear(acb_dirichlet_roots_t roots)
Clears the structure.
.. function:: void acb_dirichlet_root(acb_t res, const acb_dirichlet_roots_t roots, ulong k, slong prec)
Computes `e^{2\pi i k/n}`.
Truncated L-series and power sums
-------------------------------------------------------------------------------
.. function:: void acb_dirichlet_powsum_term(acb_ptr res, arb_t log_prev, ulong * prev, const acb_t s, ulong k, int integer, int critical_line, slong len, slong prec)
Sets *res* to `k^{-(s+x)}` as a power series in *x* truncated to length *len*.
The flags *integer* and *critical_line* respectively specify optimizing
for *s* being an integer or having real part 1/2.
On input *log_prev* should contain the natural logarithm of the integer
at *prev*. If *prev* is close to *k*, this can be used to speed up
computations. If `\log(k)` is computed internally by this function, then
*log_prev* is overwritten by this value, and the integer at *prev* is
overwritten by *k*, allowing *log_prev* to be recycled for the next
term when evaluating a power sum.
.. function:: void acb_dirichlet_powsum_sieved(acb_ptr res, const acb_t s, ulong n, slong len, slong prec)
Sets *res* to `\sum_{k=1}^n k^{-(s+x)}`
as a power series in *x* truncated to length *len*.
This function stores a table of powers that have already been calculated,
computing `(ij)^r` as `i^r j^r` whenever `k = ij` is
composite. As a further optimization, it groups all even `k` and
evaluates the sum as a polynomial in `2^{-(s+x)}`.
This scheme requires about `n / \log n` powers, `n / 2` multiplications,
and temporary storage of `n / 6` power series. Due to the extra
power series multiplications, it is only faster than the naive
algorithm when *len* is small.
.. function:: void acb_dirichlet_powsum_smooth(acb_ptr res, const acb_t s, ulong n, slong len, slong prec)
Sets *res* to `\sum_{k=1}^n k^{-(s+x)}`
as a power series in *x* truncated to length *len*.
This function performs partial sieving by adding multiples of 5-smooth *k*
into separate buckets. Asymptotically, this requires computing 4/15
of the powers, which is slower than *sieved*, but only requires
logarithmic extra space. It is also faster for large *len*, since most
power series multiplications are traded for additions.
A slightly bigger gain for larger *n* could be achieved by using more
small prime factors, at the expense of space.
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Riemann zeta function and Riemann-Siegel formula
-------------------------------------------------------------------------------
The Riemann-Siegel (RS) formula is implemented closely following
J. Arias de Reyna [Ari2011]_.
For `s = \sigma + it` with `t > 0`, the expansion takes the form
.. math ::
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\zeta(s) = \mathcal{R}(s) + X(s) \overline{\mathcal{R}}(1-s), \quad X(s) = \pi^{s-1/2} \frac{\Gamma((1-s)/2)}{\Gamma(s/2)}
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where
.. math ::
\mathcal{R}(s) = \sum_{k=1}^N \frac{1}{k^s} + (-1)^{N-1} U a^{-\sigma} \left[ \sum_{k=0}^K \frac{C_k(p)}{a^k} + RS_K \right]
.. math ::
U = \exp\left(-i\left[ \frac{t}{2} \log\left(\frac{t}{2\pi}\right)-\frac{t}{2}-\frac{\pi}{8} \right]\right), \quad
a = \sqrt{\frac{t}{2\pi}}, \quad N = \lfloor a \rfloor, \quad p = 1-2(a-N).
The coefficients `C_k(p)` in the asymptotic part of the expansion
are expressed in terms of certain auxiliary coefficients `d_j^{(k)}`
and `F^{(j)}(p)`.
Because of artificial discontinuities, *s* should be exact inside
the evaluation.
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.. function:: void acb_dirichlet_zeta_rs_f_coeffs(acb_ptr f, const arb_t p, slong n, slong prec)
Computes the coefficients `F^{(j)}(p)` for `0 \le j < n`.
Uses power series division. This method breaks down when `p = \pm 1/2`
(which is not problem if *s* is an exact floating-point number).
.. function:: void acb_dirichlet_zeta_rs_d_coeffs(arb_ptr d, const arb_t sigma, slong k, slong prec)
Computes the coefficients `d_j^{(k)}` for `0 \le j \le \lfloor 3k/2 \rfloor + 1`.
On input, the array *d* must contain the coefficients for `d_j^{(k-1)}`
unless `k = 0`, and these coefficients will be updated in-place.
.. function:: void acb_dirichlet_zeta_rs_bound(mag_t err, const acb_t s, slong K)
Bounds the error term `RS_K` following Theorem 4.2 in Arias de Reyna.
.. function:: void acb_dirichlet_zeta_rs_r(acb_t res, const acb_t s, slong K, slong prec)
Computes `\mathcal{R}(s)` in the upper half plane. Uses precisely *K*
asymptotic terms in the RS formula if this input parameter is positive;
otherwise chooses the number of terms automatically based on *s* and the
precision.
.. function:: void acb_dirichlet_zeta_rs(acb_t res, const acb_t s, slong K, slong prec)
Computes `\zeta(s)` using the Riemann-Siegel formula. Uses precisely
*K* asymptotic terms in the RS formula if this input parameter is positive;
otherwise chooses the number of terms automatically based on *s* and the
precision.
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.. function:: void acb_dirichlet_zeta(acb_t res, const acb_t s, slong prec)
Computes `\zeta(s)` using an automatic choice of algorithm.
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.. function:: void acb_dirichlet_zeta_bound(mag_t res, const acb_t s)
Computes an upper bound for `|\zeta(s)|` quickly. On the critical strip (and
slightly outside of it), formula (43.3) in [Rad1973]_ is used.
To the right, evaluating at the real part of *s* gives a trivial bound.
To the left, the functional equation is used.
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.. function:: void acb_dirichlet_eta(acb_t res, const acb_t s, slong prec)
Sets *res* to the Dirichlet eta function
`\eta(s) = \sum_{k=1}^{\infty} (-1)^k / k^s = (1-2^{1-s}) \zeta(s)`,
also known as the alternating zeta function.
Note that the alternating character `\{1,-1\}` is not itself
a Dirichlet character.
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Hurwitz zeta function precomputation
-------------------------------------------------------------------------------
.. type:: acb_dirichlet_hurwitz_precomp_struct
.. type:: acb_dirichlet_hurwitz_precomp_t
.. function:: void acb_dirichlet_hurwitz_precomp_init(acb_dirichlet_hurwitz_precomp_t pre, const acb_t s, int deflate, ulong A, ulong K, ulong N, slong prec)
Precomputes a grid of Taylor polynomials for fast evaluation of
`\zeta(s,a)` on `a \in (0,1]` with fixed *s*.
*A* is the initial shift to apply to *a*, *K* is the number of Taylor terms,
*N* is the number of grid points. The precomputation requires *NK*
evaluations of the Hurwitz zeta function, and each subsequent evaluation
requires *2K* simple arithmetic operations (polynomial evaluation) plus
*A* powers. As *K* grows, the error is at most `O(1/(2AN)^K)`.
We require that *A*, *K* and *N* are all positive. Moreover, for a finite
error bound, we require `K+\operatorname{re}(s) > 1`.
To avoid an initial "bump" that steals precision
and slows convergence, *AN* should be at least roughly as large as `|s|`,
e.g. it is a good idea to have at least `AN > 0.5 |s|`.
If *deflate* is set, the deflated Hurwitz zeta function is used,
removing the pole at `s = 1`.
.. function:: void acb_dirichlet_hurwitz_precomp_clear(acb_dirichlet_hurwitz_precomp_t pre)
Clears the precomputed data.
.. function:: void acb_dirichler_hurwitz_precomp_choose_param(ulong * A, ulong * K, ulong * N, const acb_t s, double num_eval, slong prec)
Chooses precomputation parameters *A*, *K* and *N* to minimize
the cost of *num_eval* evaluations of the Hurwitz zeta function
at argument *s* to precision *prec*.
If it is estimated that evaluating each Hurwitz zeta function from
scratch would be better than performing a precomputation, *A*, *K* and *N*
are all set to 0.
.. function:: void acb_dirichlet_hurwitz_precomp_bound(mag_t res, const acb_t s, ulong A, ulong K, ulong N)
Computes an upper bound for the truncation error (not accounting for
roundoff error) when evaluating `\zeta(s,a)` with precomputation parameters
*A*, *K*, *N*, assuming that `0 < a \le 1`.
For details, see :ref:`algorithms_hurwitz`.
.. function:: void acb_dirichlet_hurwitz_precomp_eval(acb_t res, const acb_dirichlet_hurwitz_precomp_t pre, ulong p, ulong q, slong prec)
Evaluates `\zeta(s,p/q)` using precomputed data, assuming that `0 < p/q \le 1`.
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Dirichlet character evaluation
-------------------------------------------------------------------------------
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.. function:: void acb_dirichlet_chi(acb_t res, const dirichlet_group_t G, const dirichlet_char_t chi, ulong n, slong prec)
Sets *res* to `\chi(n)`, the value of the Dirichlet character *chi*
at the integer *n*.
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.. function:: void acb_dirichlet_chi_vec(acb_ptr v, const dirichlet_group_t G, const dirichlet_char_t chi, slong nv, slong prec)
Compute the *nv* first Dirichlet values.
.. function:: void acb_dirichlet_pairing(acb_t res, const dirichlet_group_t G, ulong m, ulong n, slong prec)
.. function:: void acb_dirichlet_pairing_char(acb_t res, const dirichlet_group_t G, const dirichlet_char_t a, const dirichlet_char_t b, slong prec)
Sets *res* to the value of the Dirichlet pairing `\chi(m,n)` at numbers `m` and `n`.
The second form takes two characters as input.
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Dirichlet character Gauss, Jacobi and theta sums
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-------------------------------------------------------------------------------
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.. function:: void acb_dirichlet_gauss_sum_naive(acb_t res, const dirichlet_group_t G, const dirichlet_char_t chi, slong prec)
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.. function:: void acb_dirichlet_gauss_sum_factor(acb_t res, const dirichlet_group_t G, const dirichlet_char_t chi, slong prec)
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.. function:: void acb_dirichlet_gauss_sum_order2(acb_t res, const dirichlet_char_t chi, slong prec)
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.. function:: void acb_dirichlet_gauss_sum_theta(acb_t res, const dirichlet_group_t G, const dirichlet_char_t chi, slong prec)
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.. function:: void acb_dirichlet_gauss_sum(acb_t res, const dirichlet_group_t G, const dirichlet_char_t chi, slong prec)
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.. function:: void acb_dirichlet_gauss_sum_ui(acb_t res, const dirichlet_group_t G, ulong a, slong prec)
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Sets *res* to the Gauss sum
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.. math::
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G_q(a) = \sum_{x \bmod q} \chi_q(a, x) e^{\frac{2i\pi x}q}
- the *naive* version computes the sum as defined.
- the *factor* version writes it as a product of local Gauss sums by chinese
remainder theorem.
- the *order2* version assumes *chi* is real and primitive and returns
`i^p\sqrt q` where `p` is the parity of `\chi`.
- the *theta* version assumes that *chi* is primitive to obtain the Gauss
sum by functional equation of the theta series at `t=1`. An abort will be
raised if the theta series vanishes at `t=1`. Only 4 exceptional
characters of conductor 300 and 600 are known to have this particularity,
and none with primepower modulus.
- the default version automatically combines the above methods.
- the *ui* version only takes the Conrey number *a* as parameter.
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.. function:: void acb_dirichlet_jacobi_sum_naive(acb_t res, const dirichlet_group_t G, const dirichlet_char_t chi1, const dirichlet_char_t chi2, slong prec)
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.. function:: void acb_dirichlet_jacobi_sum_factor(acb_t res, const dirichlet_group_t G, const dirichlet_char_t chi1, const dirichlet_char_t chi2, slong prec)
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.. function:: void acb_dirichlet_jacobi_sum_gauss(acb_t res, const dirichlet_group_t G, const dirichlet_char_t chi1, const dirichlet_char_t chi2, slong prec)
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.. function:: void acb_dirichlet_jacobi_sum(acb_t res, const dirichlet_group_t G, const dirichlet_char_t chi1, const dirichlet_char_t chi2, slong prec)
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.. function:: void acb_dirichlet_jacobi_sum_ui(acb_t res, const dirichlet_group_t G, ulong a, ulong b, slong prec)
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Computes the Jacobi sum
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.. math::
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J_q(a,b) = \sum_{x \bmod q} \chi_q(a, x)\chi_q(b, 1-x)
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- the *naive* version computes the sum as defined.
- the *factor* version writes it as a product of local Jacobi sums
- the *gauss* version assumes `ab` is primitive and uses the formula
`J_q(a,b)G_q(ab) = G_q(a)G_q(b)`
- the default version automatically combines the above methods.
- the *ui* version only takes the Conrey numbers *a* and *b* as parameters.
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.. function:: void acb_dirichlet_chi_theta_arb(acb_t res, const dirichlet_group_t G, const dirichlet_char_t chi, const arb_t t, slong prec)
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.. function:: void acb_dirichlet_ui_theta_arb(acb_t res, const dirichlet_group_t G, ulong a, const arb_t t, slong prec)
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Compute the theta series `\Theta_q(a,t)` for real argument `t>0`.
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Beware that if `t<1` the functional equation
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.. math::
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t \theta(a,t) = \epsilon(\chi) \theta\left(\frac1a, \frac1t\right)
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should be used, which is not done automatically (to avoid recomputing the
Gauss sum).
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We call *theta series* of a Dirichlet character the quadratic series
.. math::
\Theta_q(a) = \sum_{n\geq 0} \chi_q(a, n) n^p x^{n^2}
where `p` is the parity of the character `\chi_q(a,\cdot)`.
For `\Re(t)>0` we write `x(t)=\exp(-\frac{\pi}{N}t^2)` and define
.. math::
\Theta_q(a,t) = \sum_{n\geq 0} \chi_q(a, n) x(t)^{n^2}.
Dirichlet L-functions
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-------------------------------------------------------------------------------
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.. function:: void acb_dirichlet_root_number_theta(acb_t res, const dirichlet_group_t G, const dirichlet_char_t chi, slong prec)
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.. function:: void acb_dirichlet_root_number(acb_t res, const dirichlet_group_t G, const dirichlet_char_t chi, slong prec)
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Sets *res* to the root number `\epsilon(\chi)` for a primitive character *chi*,
which appears in the functional equation (where `p` is the parity of `\chi`):
.. math::
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\left(\frac{q}{\pi}\right)^{\frac{s+p}2}\Gamma\left(\frac{s+p}2\right) L(s, \chi) = \epsilon(\chi) \left(\frac{q}{\pi}\right)^{\frac{1-s+p}2}\Gamma\left(\frac{1-s+p}2\right) L(1 - s, \overline\chi)
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- The *theta* variant uses the evaluation at `t=1` of the Theta series.
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- The default version computes it via the gauss sum.
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.. function:: void acb_dirichlet_l_hurwitz(acb_t res, const acb_t s, const acb_dirichlet_hurwitz_precomp_t precomp, const dirichlet_group_t G, const dirichlet_char_t chi, slong prec)
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Computes `L(s,\chi)` using decomposition in terms of the Hurwitz zeta function
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.. math::
L(s,\chi) = q^{-s}\sum_{k=1}^q \chi(k) \,\zeta\!\left(s,\frac kq\right).
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If `s = 1` and `\chi` is non-principal, the deflated Hurwitz zeta function
is used to avoid poles.
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If *precomp* is *NULL*, each Hurwitz zeta function value is computed
directly. If a pre-initialized *precomp* object is provided, this will be
used instead to evaluate the Hurwitz zeta function.
.. function:: void acb_dirichlet_l_euler_product(acb_t res, const acb_t s, const dirichlet_group_t G, const dirichlet_char_t chi, slong prec)
.. function:: void _acb_dirichlet_euler_product_real_ui(arb_t res, ulong s, const signed char * chi, int mod, int reciprocal, slong prec)
Computes `L(s,\chi)` directly using the Euler product. This is
efficient if *s* has large positive real part. As implemented, this
function only gives a finite result if `\operatorname{re}(s) \ge 2`.
An error bound is computed via :func:`mag_hurwitz_zeta_uiui`.
If *s* is complex, replace it with its real part. Since
.. math ::
\frac{1}{L(s,\chi)} = \prod_{p} \left(1 - \frac{\chi(p)}{p^s}\right)
= \sum_{k=1}^{\infty} \frac{\mu(k)\chi(k)}{k^s}
and the truncated product gives all smooth-index terms in the series, we have
.. math ::
\left|\prod_{p < N} \left(1 - \frac{\chi(p)}{p^s}\right) - \frac{1}{L(s,\chi)}\right|
\le \sum_{k=N}^{\infty} \frac{1}{k^s} = \zeta(s,N).
The underscore version specialized for integer *s* assumes that `\chi` is
a real Dirichlet character given by the explicit list *chi* of character
values at 0, 1, ..., *mod* - 1. If *reciprocal* is set, it computes
`1 / L(s,\chi)` (this is faster if the reciprocal can be used directly).
.. function:: void acb_dirichlet_l(acb_t res, const acb_t s, const dirichlet_group_t G, const dirichlet_char_t chi, slong prec)
Computes `L(s,\chi)` using a default choice of algorithm.
.. function:: void acb_dirichlet_l_jet(acb_ptr res, const acb_t s, const dirichlet_group_t G, const dirichlet_char_t chi, int deflate, slong len, slong prec)
Computes the Taylor expansion of `L(s,\chi)` to length *len*,
i.e. `L(s), L'(s), \ldots, L^{(len-1)}(s) / (len-1)!`.
If *deflate* is set, computes the expansion of
.. math ::
L(s,\chi) - \frac{\sum_{k=1}^q \chi(k)}{(s-1)q}
instead. If *chi* is a principal character, then this has the effect of
subtracting the pole with residue `\sum_{k=1}^q \chi(k) = \phi(q) / q`
that is located at `s = 1`. In particular, when evaluated at `s = 1`, this
gives the regular part of the Laurent expansion.
When *chi* is non-principal, *deflate* has no effect.
.. function:: void _acb_dirichlet_l_series(acb_ptr res, acb_srcptr s, slong slen, const dirichlet_group_t G, const dirichlet_char_t chi, int deflate, slong len, slong prec)
.. function:: void acb_dirichlet_l_series(acb_poly_t res, const acb_poly_t s, const dirichlet_group_t G, const dirichlet_char_t chi, int deflate, slong len, slong prec)
Sets *res* to the power series `L(s,\chi)` where *s* is a given power series, truncating the result to length *len*.
See :func:`acb_dirichlet_l_jet` for the meaning of the *deflate* flag.
Hardy Z-functions
-------------------------------------------------------------------------------
For convenience, setting both *G* and *chi* to *NULL* in the following
methods selects the Riemann zeta function.
Currently, these methods require *chi* to be a primitive character.
.. function:: void acb_dirichlet_hardy_theta(acb_ptr res, const acb_t t, const dirichlet_group_t G, const dirichlet_char_t chi, slong len, slong prec)
Computes the phase function used to construct the Z-function.
We have
.. math ::
\theta(t) = -\frac{t}{2} \log(\pi/q) - \frac{i \log(\epsilon)}{2}
+ \frac{\log \Gamma((s+\delta)/2) - \log \Gamma((1-s+\delta)/2)}{2i}
where `s = 1/2+it`, `\delta` is the parity of *chi*, and `\epsilon`
is the root number as computed by :func:`acb_dirichlet_root_number`.
The first *len* terms in the Taylor expansion are written to the output.
.. function:: void acb_dirichlet_hardy_z(acb_t res, const acb_t t, const dirichlet_group_t G, const dirichlet_char_t chi, slong len, slong prec)
Computes the Hardy Z-function, also known as the Riemann-Siegel Z-function
`Z(t) = e^{i \theta(t)} L(1/2+it)`, which is real-valued for real *t*.
The first *len* terms in the Taylor expansion are written to the output.
.. function:: void _acb_dirichlet_hardy_theta_series(acb_ptr res, acb_srcptr t, slong tlen, const dirichlet_group_t G, const dirichlet_char_t chi, slong len, slong prec)
.. function:: void acb_dirichlet_hardy_theta_series(acb_poly_t res, const acb_poly_t t, const dirichlet_group_t G, const dirichlet_char_t chi, slong len, slong prec)
Sets *res* to the power series `\theta(t)` where *t* is a given power series, truncating the result to length *len*.
.. function:: void _acb_dirichlet_hardy_z_series(acb_ptr res, acb_srcptr t, slong tlen, const dirichlet_group_t G, const dirichlet_char_t chi, slong len, slong prec)
.. function:: void acb_dirichlet_hardy_z_series(acb_poly_t res, const acb_poly_t t, const dirichlet_group_t G, const dirichlet_char_t chi, slong len, slong prec)
Sets *res* to the power series `Z(t)` where *t* is a given power series, truncating the result to length *len*.