CuBQL (say: "cubicle") is a (mostly) header-only CUDA/C++ library for the easy and efficient GPU-construction and -traversal of bounding volume hierarchies (BVHes), with the ultimate goal of providing the tools and infrastructure to realize a wide range of (GPU-accelerated) spatial queries over various geometric primitives.
CuBQL is largely inspired by two libraries: the standard template
library (STL
), and cub
. Like those two libraries cuBQL largely
relies on header-only CUDA/C++ code, and on the use of templates and
lambda functions to make sure that certain key operations (like
traversing a BVH) can work for different primititive, different data
type and dimensionality (e.g., float3
vs int2
), multiple different
but similar geometric queries (e.g., find closest point
vs
k-nearest neighbor (kNN)
vs signed distance functions (SDF)
, etc).
Throughout cuBQL, the main driving goal are robustness, generality, and ease of use: each builder for each BVH type should always work for all input types and dimensionality, and even for numerically challenging input data.
CuBQL offers four separate layers of functionality:
-
Abstract BVH Type
layer: defines the basic (GPU friendly) type(s) for different kinds of BVHes. In particular, the cuBQL bvh types is templated over what geometric space the BVH is to be built over; i.e., you can realize not only BVHes overfloat3
data, but also BVHes overint4
,double2
, etc (cuBQL spans the entire space of {int,float,double,long}x{2,3,4,N}). -
BVH builders
layer: provides a set of primarily GPU-side (but also some simple host side) builder(s) for the underlying BVH type(s). This level offers multiple different builders with different speed/quality tradeoffs (though the defaultgpuBuilder
should work well for most cases). -
BVH Traversal Templates
layer: though different types of geometric queries are often similar in concept, nevertheless they often slightly differ in detail. Instead of only providing a fixed set of very specific geometric queries cuBQL focusses on providing a set of traversal templates that, though the use of lambda functions, can easily be modified in their details. E.g., both a kNN and a find closest point query will build on the sameshrinking radius query
, with just different way of processing a given candidate primitive encountered during traversal. -
Various (specific) Geometric Queries
, realized with the underlying layers. cuBQL provides these queries more as samples than anything else, fully assuming that many users will have requirements that the existing samples will not capture---but which these samples's use of the traversal templates should show how to realize.
The main BVH type of this library is a binary BVH, where each node
contains that node's bounding box, as well as two ints, count
and
offset
.
template<typename /*ScalarType*/T,
int /*Dimensionality*/D>
struct BinaryBVH {
struct CUBQL_ALIGN(16) Node {
box_t<T,D> bounds;
uint64_t offset : 48;
uint64_t count : 16;
};
Node *nodes;
uint32_t numNodes;
uint32_t *primIDs;
uint32_t numPrims;
};
The count
value is 0 for inner nodes, and for leaf nodes specifies
the number of primitives in this leaf. For inner nodes, the offset
indexes into the BinaryBVH::nodes[]
array (the current node's two
children are at nodes[offset]
, and nodes[offset+1]
, respectively);
for leaf nodes it points into the BinaryBVH::primIDs[]
array (i.e.,
that leaf contains primID[offset+0]
, primID[offset+1]
, etc).
A WideBVH<N>
type (templated over BVH width) is supported as
well. WideBVH'es always have a fixed branching factor of N (i.e., a
fixed number of N
children in each inner node); however, some of
these may be 'null' (marked as not valid). Note that most builders
will only work for binary BVHes; these can then "collapsed" into
Wide-BVHes.
Though most of the algorithms and data types in this library could
absolutely be templated over both dimensionality and underlying data
type (i.e., a BVH over double4
data rather than float3
), for sake
of readability in this particular implementation this has not been
done (yet?). If this is a feature you would like to have, please let
me know.
The main workhorse of this library is a CUDA-accelerated and on device
parallel BVH builder (with spatial median splits). The primary
feature of the BVH builder is its simplicity; i.e., it is still
"reasonably fast", but it is much simpler than other variants. Though
performance will obviously vary for different data types, data
distributions, etc..., right now this builder builds a BinaryBVH over
10 million uniformly distributed random points in under 13ms; that's
not the fastest builder I have, but IMHO quite reasonable for most
applications. In addition to this cuBQL::gpuBuilder()
there are also
various other builders, including a regular morton/radix builder, a
wide GPU builder (for BVHes with branching factors greater than 2), a
surface-area-heuristic (SAH) builder, and a modified morton/radix
builder that for numerically challenging inputs is significantly more
robust than a regular morton/radix builder.
For all builders, the overall build process is always the same: Create an array of bounding boxes (one box per primitive), and call the builder with a pointer to this array, and the number of primitives. For GPU-side builders this array has to live in device (or managed) memory; for host side builds it has to be in host memory. Obiously, device side builders will create node and primitmive ID arrays in device memory, the host builder will create these in host memory.
Given such an array, the builder (in this case, for float3
data)
gets invoked as follows:
#include "cuBQL/bvh.h"
...
box3f *d_boxes = 0;
int numBoxes = 0;
userCodeForGeneratingPrims(&d_boxes,&numBoxes, ...);
...
cuBQL::BinaryBVH<float,3> bvh;
cuBQL::BuildConfig buildParams;
cuBQL::gpuBuilder(bvh,d_boxes,numBoxes,buildParams);
...
Builds for other data types (such as, e.g., <int,4>
or <double,2>`)
work exactly the same way (though obviously, the scalar type and dimensionality of the
boxes has to be the same as that for the BVH).
The builder will not modify the d_boxes[]
array; after the build is
complete the bvh.primIDs[]
array contains ints referring to indices
in this array. This builder will properly handle "invalid prims" and
"empty boxes": Primitives that are not supposed to be included in the
BVH can simply use a box for which lower.x > upper.x
; such
primitives will be detected during the build, and will simply get
excluded from the build process - i.e., they will simply not appear in
any of the leaves, but also not influence any of the (valid) bounding
boxes. However, behavior for NaNs, denorms, etc. is not
defined. Zero-volume primitives (ie, those with box.lower == box.upper
) are considered valid primitives, and will get included in
the BVH.
The BuildConfig
class can be used to influence things like whether
the BVH should be built with a surface area heuristic (SAH) cost
metric (more expensive build, but faster queries for some types of
inputs and query operations), or how coarse vs how fine the BVH should
be built (ie, at which point to make a leaf).
A few notes:
-
For GPU builders one can optionally also pass a
cudaStream_t
if desired. All operations, synchronization, and memory allocs should happen in that stream. -
By default the GPU side builder(s) will allocate device memory; but it is also be possible to make them use managed memory or async device memory by passing the appropriate
cuBQL::GpuMemoryResource
to the builder. -
Following the same pattern as other libraries like tinyOBJ or STB, this library can be used in a header-only form: By default a included header file will only pull in the type and function declarations, but specifying
CUBQL_GPU_BUILDER_IMPLEMENTATION
to 1 will also pull in the implementation, so using this in one of one's source files allows the user to compile the builders with exactly the cmd-line flags, CUDA architecture, etc, that he or she desires. Alternatively (and purely optionally), when usingcmake
one can also link to one (or more) of specific pre-defined targets such as, for example,cuBQL_cuda_float3
orcuBQL_host_int4
that will then build that specific device and type specific builder(s).
CuBQL is the fourth one of different libraries that all aimed at providing fast, GPU-accelerated geometric queries. Throughout these previous predecessor libraries, a common theme that emerged was that whatever exact implementation the library provided, the user(s) typically required something that, though similar, was often just a little bit different. For example, a "find closest point point" kernel on point data is very similar to "find closest surface point" (on a set of triangles), but the actual point-to-primitive test is nevertheless different. Similarly, k-nearest-neighbor (kNN) queries might want to exclude certain points (e.g., based on surface normal for photon mapping), or a "find all points that overlap this box" kernel might only actually require the number of points vs another use case that might require the actual primitive IDs, etc.
Based on this experience cuBQL
decided to not only provide a set of
very specific geometric kernels, but to also provide a set of what
it calls traversal templates
that can be used to easily generate
different variants of queries using lamdba functions. For example,
both kNN (with or without culling by surface normal) and find closest
point (on points or on triangles) in principle work the same way, by
performing a ball-shaped query where the radius of that ball shrinks
during traversal, based on what primitive(s) have already been
found. What exactly the query wants to do with a given primitmive that
the traversal encounters depends on the actual query code, but as long
as the traversal knows what range it has to look for after a given
primitmive has been processed it does not actually need to know what
specific operation that query need to do.q
In cuBQL, this pattern is realized through what we call a "shrinking
radius query": In this query, the user provides a query point (as the
origin of that query), a (intital) maximum search radius, and a lambda
function (ie, a "callback") that it wants to get called for any
"candidate" primitive encountered by the traversal. This lambda can
then do whatever that type of query needs to do with that primitive,
and can additionally return a new maximum query radius that the
traversal can then use for subsequent traversal steps. To do this, the
user would simply define a lambda function that implements the
specific per-primitive callback code, and pass that to a
cuBQL::shrinkingRadiusQuery::forEachPrim(...)
traversal template:
inline __device__
void myQuery(bvh3f myBVH,
MyPrim *myPrims,
vec3f myQueryPoint,
...)
{
auto myQueryLambda = [...](int primID) -> float {
...
};
cuBQL::shrinkingRadiusQuery::forEachPrim
(myQueryLambda,myQueryPoint,myBVH, ...);
}
For example, a find closest point
kernel can then be realized
by having the lamdba callback simply keep track of the currently
closest point:
void findClosestPoint(...)
{
float closestDist = INFINITY;
int closestID = -1;
auto myQueryLambda = [&closestDist,&closestID,...](int primID) -> float {
float dist = distance(queryPoint,myPrims[primID]);
if (dist < closestDist)
{ closestDist = dist; closestID = primID; }
return closestDist;
};
}
Note that this same patters works for both point-to-point or point-to-triangular-surface
data! Also, the exact same pattern works for float3
data as for int2
, etc.
As described above, by far the main focus of cuBQL is the BVH builders, and the traversal templates, for users to be able to write their own specific queries. In addition, cuBQL also contains a small(!) set of very specific queries such as find closest point among float3 points, find closest surface point on triangle-mesh surface, k-nearest (float3 point) neighbor, etc. These should be considered more "samples" (for how to use the builder and traversal templates), but can of course also be used directly for those that require that exact kernel.
- all of the cuBQL library are under
~/cuBQL/
~/cuBQL/bvh.h
defines the various BVH types~/cuBQL/builder/cuda.h
and~/cuBQL/builder/host.h
provides the (header-only) source for the various builder(s)~/cuBQL/traversal/...
provides the traversal templates
- various specific queries are under
~/cuBQL/queries/
(also all header-only) - some specific sample codes are under
~/samples/
, and some tools for more comprehensive testing are under~/testing/
Most users should only every need what is under ~/cuBQL/
, in fact
most should only need the builder(s) and possibly traversal
templates. Everything else should predominantly be viewed as examples
of how to use those.
To use cuBQL
, you need:
- CUDA, version 12 and up. In theory some versions of CUDA 11 should work too, but using 12.2 and upwards is highly recommended.
cmake
As all of cuBQL's BVH builders and traversers can be used in a
header-only form, cuBQL can be used from within any compiler and build
system, by simply providing the proper include paths and including the
cuBQL/bvh.h
or other header files as required.
However, we strongly suggest to use cmake
, include cuBQL as a cmake
add_subdirectory(...)
, and then target_link_libraries(...)
with
the desired cuBQL cmake target.
- in your own CUDA sources (say,
userMain.cu
):
#define CUBQL_GPU_BUILDER_IMPLEMENTATION 1
#include <cuBQL/bvh.h>
...
void foo(...) {
cuBQL::gpuBuilder(...)
}
- in your own
CMakeLists.txt
:
add_subdirectory(<pathTo>/cuBQL)
add_executable(userExec ...
userMain.cu ...)
target_link_libraries(userExec ...
cuBQL)
In this case, the 'cuBQL' target that we link to is only a cmake
INTERFACE
target that merely sets up the right include paths, but
does not build any actual library.
- in your own CUDA sources (say,
userMain.cu
):
// do NOT define CUBQL_GPU_BUILDER_IMPLEMENTATION
#include <cuBQL/bvh.h>
...
void foo(...) {
cuBQL::gpuBuilder(...)
}
- in your own
CMakeLists.txt
:
add_subdirectory(<pathTo>/cuBQL)
add_executable(userExec ...
userMain.cu ...)
target_link_libraries(userExec ...
cuBQL_cuda_float3)