Is there a material today that could act as the forward plating of my ship that could withstand such an impact?
The problem is the same with the rock hitting the ship while the former is traveling at .05c and the latter is standing still. We may use Newton's impact depth equation giving penetration depth of a projectile P in a shield S, $depth = length_P \frac{density_P}{density_S}$: at that speed, the barrier will act as a liquid and the rock, having a length of 5 cm and a typical density of 3.5 g/cm^3, will penetrate to a depth of about 17.5 cm in water (this excludes penetration-optimized shapes). At that point it will have ceded all its considerable momentum to the surrounding material, converting a significant fraction of it into compressive and friction heat, and it will explode.
In the volume of impact a plasma jet will form, still possessing a considerable momentum, and will start penetrating inwards; since the elementary momentum is given by the product of density by speed, and it is a finite quantity, the greater the density the lesser the speed.
So you want to have the densest possible material (which would be osmium, density of around 22) for the first 20-25 cm, then you need to survive the explosion of ~240 tons of TNT and temperatures briefly in excess of several hundred thousand K, plus the jet of osmium plasma that has absorbed the momentum of the impactor. This calls for some superrefrigerated phase-changing metamaterial (mostly ice-XI) and some way of distributing the impact laterally as quickly as possible, which calls for an enormous Young's modulus - basically a carbyne layer.
Finally you need to consider spallation. The shock wave will travel through the armor, and blast the opposite side even if the projectile doesn't push all the way through. You need a further layer of high density, high tensile material to block that.
I'm not too sure that all of that is going to fit in a 100cm thickness...
We overlooked something!
The thickness of 100cm refers to an impactor hitting head on. But if we build the shield as a sloped, conical glacis - a vacuodynamic shape - we reap some very important benefits:
- the collision will be at an angle, thereby wasting a large part of its energy into a shower of fragments taking away most of the momentum harmlessly.
- the penetration path will be increased by the inverse sine of the slope angle; an angle of 30° will immediately double the thickness of the material as seen by the impactor.
I think we can do this! :-)
Charged Whipple shield
A standard Whipple shield will probably not fare well against solid objects in the hundred-gram range.
But we can imagine a cubic lattice of osmium pellets connected by very strong insulating threads (e.g. Kevlar) no more than three or four centimeters long horizontally, and a dozen meters vertically; the lattice itself is as wide as the ship's front.
At takeoff, the lattice is folded and is only some centimeters thick. Then we start pumping electric charge into it (somehow). Coulomb repulsion starts driving the pellets away one from the other, until they form several layers of four-centimeter square mesh, separated by a dozen meters of empty space. When the charge is high enough, the lattice becomes increasingly rigid.
Now a 5-cm rock comes in at .05c relative speed. It impacts on one, possibly two pellets of the first layer, and explodes, forming a cone of debris still traveling at .05c. It has also absorbed a lot of electric charge, and therefore each debris particle is strongly repelled by all the others - which contributes to the cone's expansion - and by the incoming subsequent layers, which both expands the cone and slows it down. We can't pack 16 TJ of Coulombian potential in one hundred twenty meters' worth of lattice (or can we?), as the lattice would start discharging by emitting charges into space faster than we could replace them, but sure we can make it behave like a sort of electric reactive armor.
In the end, the final layer of the shield only needs to be able to deal with small-size buckshot; a layered sandwich of high-density material to absorb momentum, high-tensile material to diffuse the shock and vacuum to stop P-waves will suffice.
When slowing down at arrival, the lattice is powered down and folded back.
It's true that the total installed thickness is two orders of magnitude greater than your requirement of 100cm, but its equivalent thickness might well fall under that.
Protecting against impactors
Protecting against impact will resemble that game called Missile Defense, with the impactors arriving at a relative .05c.

But you cannot use missiles. What you do is saturate the space in front of the ship with millimetric radar, which will give you a low-noise estimate of the incoming impactors and something about their nature. It's reasonable to expect detection at about 500-600 kilometers, maybe more (high vacuum, few disturbances). You will use several radars to immediately gauge position and speed of incoming projectiles through parallax and Doppler shift (and also for redundancy). At 500 km distance traveling at .05c you have a warning time of about 30 milliseconds.
You can't safely swing a weapon mount in that time. So you use a massive phased laser array instead, to direct the equivalent of a focused megawatt of power from a supercapacitor bank into the rock, which can be expected to shatter.
This robs the inbound projectile of perhaps one percent of its energy, but importantly it reduces its size, and penetration is proportional to that. It also weakens its structure, increasing the chances that a glancing impact will remain just that - a glancing impact.
At the same time, the relative speed imparted to the impactor will be directed towards making the impact angle shallower, further reducing the damage.
If there's enough time, supplemental strikes could further reduce the damage by pulverizing the most threatening fragments.