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Copyright 1999, 2000, 2001, 2002, 2003, 2004, 2005 Free Software Foundation.
Contributed by the Spaces project, INRIA Lorraine.

This file is part of the MPFR Library.

The MPFR Library is free software; you can redistribute it and/or modify it
under the terms of the GNU Lesser General Public License (either version 2.1
of the License, or, at your option, any later version) and the GNU General
Public License as published by the Free Software Foundation (most of MPFR is
under the former, some under the latter).

The MPFR Library is distributed in the hope that it will be useful, but
WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY
or FITNESS FOR A PARTICULAR PURPOSE.  See the GNU Lesser General Public
License for more details.

You should have received a copy of the GNU Lesser General Public License
along with the MPFR Library; see the file COPYING.LIB.  If not, write to
the Free Software Foundation, Inc., 51 Franklin Place, Fifth Floor, Boston, MA
02110-1301, USA.


##############################################################################
Documentation:
##############################################################################

- add a description of the algorithms used + proof of correctness

- mpfr_set_prec: add an explanation of how to speed up calculations
  which increase their precision at each step.


##############################################################################
Installation:
##############################################################################

- nothing to do currently :-)


##############################################################################
Changes in existing functions:
##############################################################################

- many functions currently taking into account the precision of the *input*
  variable to set the initial working precison (acosh, asinh, cosh, ...).
  This is nonsense since the "average" working precision should only depend
  on the precision of the *output* variable (and maybe on the *value* of
  the input in case of cancellation).
  -> remove those dependencies from the input precision.

- mpfr_get_str should support base up to 62 too.

- mpfr_can_round:
   change the meaning of the 2nd argument (err). Currently the error is
   at most 2^(MPFR_EXP(b)-err), i.e. err is the relative shift wrt the
   most significant bit of the approximation. I propose that the error
   is now at most 2^err ulps of the approximation, i.e.
   2^(MPFR_EXP(b)-MPFR_PREC(b)+err).

- mpfr_set_q first tries to convert the numerator and the denominator
  to mpfr_t. But this convertion may fail even if the correctly rounded
  result is representable. New way to implement:
  Function q = a/b.  nq = PREC(q) na = PREC(a) nb = PREC(b)
    If na < nb
       a <- a*2^(nb-na)
    n <- na-nb+ (HIGH(a,nb) >= b)
    if (n >= nq)
       bb <- b*2^(n-nq)
       a  = q*bb+r     --> q has exactly n bits.
    else
       aa <- a*2^(nq-n)
       aa = q*b+r      --> q has exaclty n bits.
  If RNDN, takes nq+1 bits. (See also the new division function).


##############################################################################
New functions to implement:
##############################################################################

- modf (to extract integer and fractional parts), suggested by
	Dmitry Antipov <dmitry.antipov@mail.ru> Thu, 13 Jun 2002
- mpfr_fmod (mpfr_t, mpfr_srcptr, mpfr_srcptr, mp_rnd_t)
  [suggested by Tomas Zahradnicky <tomas@24uSoftware.com>, 29 Nov 2003]
  Kevin: Might want to be called mpfr_mod, to match mpz_mod.
  -> we probably want to allow both mpfr_fmod and mpfr_mod.
- mpfr_fms for a-b*c
  [suggested by Tomas Zahradnicky <tomas@24uSoftware.com>, 29 Nov 2003]
- 1/sqrt(x) [Regis Dupont <dupont@lix.polytechnique.fr>, 15 Sep 2004]
- dilog() [the dilogarithm: dilog(x) =  int(ln(t)/(1-t), t=1..x)]
- mpfr_printf [Sisyphus <kalinabears@iinet.net.au> Tue, 04 Jan 2005]
  for example mpfr_printf ("%.2Ff\n", x)
- wanted for Magma [John Cannon <john@maths.usyd.edu.au>, Tue, 19 Apr 2005]:
  BesselFunction(n,x) = J_n(x) [first kind]
  HypergeometricU(a,b,s) = 1/gamma(a)*int(exp(-su)*u^(a-1)*(1+u)^(b-a-1),
                                    u=0..infinity)
  JacobiThetaNullK
  PolylogP, PolylogD, PolylogDold
  JBessel
  IncompleteGamma
  KBessel, KBessel2 [2nd kind]
  JacobiTheta
  LogIntegral
  ExponentialIntegralE1
    E1(z) = int(exp(-t)/t, t=z..infinity), |arg z| < Pi
    mpfr_eint1: implement E1(x) for x > 0, and Ei(-x) for x < 0
    E1(NaN)  = NaN
    E1(+Inf) = +0
    E1(-Inf) = -Inf
    E1(+0)   = +Inf
    E1(-0)   = -Inf
  DawsonIntegral
  Psi = LogDerivative
  LogGamma
  GammaD(x) = Gamma(x+1/2)
- functions defined in the LIA-2 standard
  + minimum and maximum (5.2.2): max, min, max_seq, min_seq, mmax_seq
    and mmin_seq (mpfr_min and mpfr_max correspond to mmin and mmax);
  + rounding_rest, floor_rest, ceiling_rest (5.2.4);
  + remr (5.2.5): x - round(x/y) y;
  + rec_sqrt (5.2.6): 1 / sqrt(x);
  + error functions from 5.2.7 (if useful in MPFR);
  + power1pm1 (5.3.6.7): (1 + x)^y - 1;
  + logbase (5.3.6.12): \log_x(y);
  + logbase1p1p (5.3.6.13): \log_{1+x}(1+y);
  + rad (5.3.9.1): x - round(x / (2 pi)) 2 pi = remr(x, 2 pi);
  + axis_rad (5.3.9.1) if useful in MPFR;
  + cycle (5.3.10.1): rad(2 pi x / u) u / (2 pi) = remr(x, u);
  + axis_cycle (5.3.10.1) if useful in MPFR;
  + sinu, cosu, tanu, cotu, secu, cscu, cossinu, arcsinu, arccosu,
    arctanu, arccotu, arcsecu, arccscu (5.3.10.{2..14}):
    sin(x 2 pi / u), etc.;
  + arcu (5.3.10.15): arctan2(y,x) u / (2 pi);
  + rad_to_cycle, cycle_to_rad, cycle_to_cycle (5.3.11.{1..3}).
- From GSL, missing special functions (if useful in MPFR):
  + The Airy functions Ai(x) and Bi(x) defined by the integral representations:
   * Ai(x) = (1/\pi) \int_0^\infty \cos((1/3) t^3 + xt) dt
   * Bi(x) = (1/\pi) \int_0^\infty (e^(-(1/3) t^3) + \sin((1/3) t^3 + xt)) dt
   * Derivatives of Airy Functions
  + The Bessel functions for n integer and n fractionnal: 
   * Regular Cylindrical Bessel Functions J_n
   * Irregular Cylindrical Bessel Functions Y_n
   * Regular Modified Cylindrical Bessel Functions I_n
   * Irregular Modified Cylindrical Bessel Functions K_n
   * Regular Spherical Bessel Functions j_n: j_0(x) = \sin(x)/x, 
  j_1(x)= (\sin(x)/x-\cos(x))/x & j_2(x)= ((3/x^2-1)\sin(x)-3\cos(x)/x)/x
   *Irregular Spherical Bessel Functions y_n: y_0(x) = -\cos(x)/x,
  y_1(x)= -(\cos(x)/x+\sin(x))/x & y_2(x)= (-3/x^3+1/x)\cos(x)-(3/x^2)\sin(x)
   * Regular Modified Spherical Bessel Functions i_n:
     i_l(x) = \sqrt{\pi/(2x)} I_{l+1/2}(x)
   * Irregular Modified Spherical Bessel Functions:
     k_l(x) = \sqrt{\pi/(2x)} K_{l+1/2}(x).
  + Clausen Function:
     Cl_2(x) = - \int_0^x dt \log(2 \sin(t/2))
     Cl_2(\theta) = \Im Li_2(\exp(i \theta)) (dilogarithm).
  + Dawson Function: \exp(-x^2) \int_0^x dt \exp(t^2).     
  + Debye Functions: D_n(x) = n/x^n \int_0^x dt (t^n/(e^t - 1))
  + Elliptic Integrals:
   * Definition of Legendre Forms:
    F(\phi,k) = \int_0^\phi dt 1/\sqrt((1 - k^2 \sin^2(t)))
    E(\phi,k) = \int_0^\phi dt   \sqrt((1 - k^2 \sin^2(t)))
    P(\phi,k,n) = \int_0^\phi dt 1/((1 + n \sin^2(t))\sqrt(1 - k^2 \sin^2(t)))
   * Complete Legendre forms are denoted by 
    K(k) = F(\pi/2, k) 
    E(k) = E(\pi/2, k)
   * Definition of Carlson Forms
    RC(x,y) = 1/2 \int_0^\infty dt (t+x)^(-1/2) (t+y)^(-1)
    RD(x,y,z) = 3/2 \int_0^\infty dt (t+x)^(-1/2) (t+y)^(-1/2) (t+z)^(-3/2)
    RF(x,y,z) = 1/2 \int_0^\infty dt (t+x)^(-1/2) (t+y)^(-1/2) (t+z)^(-1/2)
    RJ(x,y,z,p) = 3/2 \int_0^\infty dt 
                          (t+x)^(-1/2) (t+y)^(-1/2) (t+z)^(-1/2) (t+p)^(-1)
  + Elliptic Functions (Jacobi)
  + N-relative exponential:
     exprel_N(x) = N!/x^N (\exp(x) - \sum_{k=0}^{N-1} x^k/k!)
  + exponential integral:
     E_2(x) := \Re \int_1^\infty dt \exp(-xt)/t^2.
     Ei_3(x) = \int_0^x dt \exp(-t^3) for x >= 0. 
     Ei(x) := - PV(\int_{-x}^\infty dt \exp(-t)/t)
  + Hyperbolic/Trigonometric Integrals
     Shi(x) = \int_0^x dt \sinh(t)/t
     Chi(x) := Re[ \gamma_E + \log(x) + \int_0^x dt (\cosh[t]-1)/t]
     Si(x) = \int_0^x dt \sin(t)/t
     Ci(x) = -\int_x^\infty dt \cos(t)/t for x > 0
     AtanInt(x) = \int_0^x dt \arctan(t)/t
     [ \gamma_E is the Euler constant ]
  + Fermi-Dirac Function:
     F_j(x)   := (1/r\Gamma(j+1)) \int_0^\infty dt (t^j / (\exp(t-x) + 1))
  + Pochhammer symbol (a)_x := \Gamma(a + x)/\Gamma(a)
    logarithm of the Pochhammer symbol
  + Gegenbauer Functions
  + Laguerre Functions
  + Eta Function: \eta(s) = (1-2^{1-s}) \zeta(s)
    Hurwitz zeta function: \zeta(s,q) = \sum_0^\infty (k+q)^{-s}.
  + Lambert W Functions, W(x) are defined to be solutions of the equation:
     W(x) \exp(W(x)) = x. 
    This function has multiple branches for x < 0 (2 funcs W0(x) and Wm1(x))
  + Trigamma Function psi'(x).
    and Polygamma Function: psi^{(m)}(x) for m >= 0, x > 0.

- from gnumeric (www.gnome.org/projects/gnumeric/doc/function-reference.html):
  - beta
  - betaln
  - degrees
  - radians
  - sqrtpi

- mpfr_frexp(mpfr_t rop, mp_exp_t *n, mpfr_t op, mp_rnd_t rnd) suggested by
  Steve Kargl <sgk@troutmask.apl.washington.edu> Sun, 7 Aug 2005

##############################################################################
Efficiency:
##############################################################################

- speed up const_euler for large precision [for x=1.1, prec=16610, it takes
	75% of the total time of eint(x)!]
- speed up mpfr_atan for large arguments (to speed up mpc_log)
	[from Mark Watkins on Fri, 18 Mar 2005]
  Also mpfr_atan(x) seems slower (by a factor of 2) for x near from 1.
  Example on a Athlon for 10^5 bits: x=1.1 takes 3s, whereas 2.1 takes 1.8s.
  The current implementation does not give monotonous timing for the following:
  mpfr_random (x); for (i = 0; i < k; i++) mpfr_atan (y, x, GMP_RNDN);
  for precision 300 and k=1000, we get 1070ms, and 500ms only for p=400!
- implement range reduction in sin/cos/tan for large arguments
	(currently too slow for 2^1024), and/or implement Mark Watkins's
	algorithm:
  My suggestion for a long-term fix to these sin/cos problems when one
  of them is close to zero is the following:
  Give input inp:
  1) Reduce inp to the interval 0 to Pi/2
  2) If inp is less than Pi/4, compute sin(inp) via a power series around 0.
  3) If inp is more than Pi/4, compute s=Pi/2-inp to the working precision
     (most of the possible cancellation will occur here --- or in step 1)
     and calculate cos(inp) as a power series (in s) around Pi/2 --- thus
     the output is near zero precisely when the s-input is near zero,
     avoiding most cancellation problems.
  4) Having sin or cos, compute the other via the sqrt. This will not cause
     cancellation problems because the computed sin or cos is not near 1.
- combined mpfr_sinh_cosh() [Geoff Bailey, 20 Apr 2005]
- improve generic.c to work for number of terms <> 2^k
- rewrite mpfr_greater_p... as native code.
- inline mpfr_neg? Problems with NAN flags:
   #define mpfr_neg(_d,_x,_r)                          \
    (__builtin_constant_p ((_d)==(_x)) && (_d)==(_x) ? \
     ((_d)->_mpfr_sign = -(_d)->_mpfr_sign, 0)       : \
      mpfr_neg ((_d), (_x), (_r)))  */

- mpf_t uses a scheme where the number of limbs actually present can
  be less than the selected precision, thereby allowing low precision
  values (for instance small integers) to be stored and manipulated in
  an mpf_t efficiently.

  Perhaps mpfr should get something similar, especially if looking to
  replace mpf with mpfr, though it'd be a major change.  Alternately
  perhaps those mpfr routines like mpfr_mul where optimizations are
  possible through stripping low zero bits or limbs could check for
  that (this would be less efficient but easier).


##############################################################################
Miscellaneous:
##############################################################################

- rename mpf2mpfr.h to gmp-mpf2mpfr.h?
  (will wait until mpfr is fully integrated into gmp :-)

- from Kevin Ryde <user42@zip.com.au>:
   Also for pi.c, a pre-calculated compiled-in pi to a few thousand
   digits would be good value I think.  After all, say 10000 bits using
   1250 bytes would still be small compared to the code size!
   Store pi in round to zero mode (to recover other modes).

- add a new rounding mode: rounding away from 0. This can be easily
  implemented as follows: round to zero, and if the result is inexact,
	add one ulp to the mantissa.
- add a new rounding mode: round to nearest, with ties away from zero
  (will be in 754r, could be used by mpfr_round)
- add a new roundind mode: round to odd. If the result is not exactly
	representable, then round to the odd mantissa. This rounding
	has the nice property that for k > 1, if:
	y = round(x, p+k, TO_ODD)
        z = round(y, p, TO_NEAREST_EVEN), then
        z = round(x, p, TO_NEAREST_EVEN)
  so it avoids the double-rounding problem.

- check/define the sign of infinity for gamma(-integer)

- add tests of the ternary value for constants

- When doing Extensive Check (--enable-assert=full), since all the
  functions use a similar use of MACROS (ZivLoop, ROUND_P), it should 
  be possible to do such a scheme:
    For the first call to ROUND_P when we can round.
    Mark it as such and save the approximated rounding value in 
    a temporary variable.
    Then after, if the mark is set, check if:
      - we still can round.
      - The rounded value is the same.
  It should be a complement to tgeneric tests.

##############################################################################
Portability:
##############################################################################

- [Kevin about texp.c long strings]
  For strings longer than c99 guarantees, it might be cleaner to
  introduce a "tests_strdupcat" or something to concatenate literal
  strings into newly allocated memory.  I thought I'd done that in a
  couple of places already.  Arrays of chars are not much fun.



##############################################################################
Possible future MPF / MPFR integration:
##############################################################################

- mpf routines can become "extern inline"s calling mpfr equivalents,
  probably just with GMP_RNDZ hard coded, since that's what mpf has
  always done.

- Want to preserve the mpf_t structure size, for binary compatibility.
  Breaking compatibility would cause lots of pain and potential subtle
  breakage for users.  If the fields in mpf_t are not enough then
  extra space under _mp_d can be used.

- mpf_sgn has been a macro directly accessing the _mp_size field, so a
  compatible representation would be required.  At worst that field
  could be maintained for mpf_sgn, but not otherwise used internally.

  mpf_sgn should probably throw an exception if called with NaN, since
  there's no useful value it can return, so it might want to become a
  function.  Inlined copies in existing binaries would hopefully never
  see a NaN, if they only do old-style mpf things.

- mpfr routines replacing mpf routines must be reentrant and thread
  safe, since of course that's what has been documented for mpf.

- mpfr_random will not be wanted since there's no corresponding
  mpf_random and new routines should not use the old style global
  random state.